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rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20169"/></rdf:Seq></items></channel><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20268" xmlns="http://purl.org/rss/1.0/"><title>Northern North Atlantic sea-surface height and ocean heat content variability</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20268</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Northern North Atlantic sea-surface height and ocean heat content variability</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sirpa Häkkinen, Peter B. Rhines, Denise L. Worthen</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-15T05:21:22.253747-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20268</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20268</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20268</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The evolution of nearly 20 years of altimetric sea surface height (SSH) is investigated to understand its association with decadal to multidecadal variability of the North Atlantic heat content. Altimetric SSH is dominated by an increase of about 14cm in the Labrador and Irminger Seas from 1993 to 2011, while the opposite has occurred over the Gulf Stream region over the same time period. During the altimeter period the observed 0-700 meter ocean heat content (OHC) in the subpolar gyre mirrors the increased SSH by its dominantly positive trend. Over a longer period, 1955-2011, fluctuations in the subpolar OHC reflect Atlantic Multidecadal Variability (AMV) and can be attributed to advection driven by the wind stress 'gyre mode' bringing more subtropical waters into the subpolar gyre. The extended subpolar warming evident in SSH and OHC during the altimeter period represents transition of the AMV from cold to warm phase. In addition to the dominant trend, the first empirical orthogonal function (EOF) SSH time series shows an abrupt change 2009-2010 reaching a new minimum in 2010. The change coincides with the change in the Meridional Overturning Circulation (MOC) at 26.5N as observed by the RAPID project, and with extreme behavior of the wind-stress gyre mode and of atmospheric blocking. While the general relationship between northern warming and AMOC volume transport remains undetermined, the meridional heat- and salt transport carried by AMOC's arteries are rich with decade-to-century timescale variability.</p></div>
]]></content:encoded><description>

The evolution of nearly 20 years of altimetric sea surface height (SSH) is investigated to understand its association with decadal to multidecadal variability of the North Atlantic heat content. Altimetric SSH is dominated by an increase of about 14cm in the Labrador and Irminger Seas from 1993 to 2011, while the opposite has occurred over the Gulf Stream region over the same time period. During the altimeter period the observed 0-700 meter ocean heat content (OHC) in the subpolar gyre mirrors the increased SSH by its dominantly positive trend. Over a longer period, 1955-2011, fluctuations in the subpolar OHC reflect Atlantic Multidecadal Variability (AMV) and can be attributed to advection driven by the wind stress 'gyre mode' bringing more subtropical waters into the subpolar gyre. The extended subpolar warming evident in SSH and OHC during the altimeter period represents transition of the AMV from cold to warm phase. In addition to the dominant trend, the first empirical orthogonal function (EOF) SSH time series shows an abrupt change 2009-2010 reaching a new minimum in 2010. The change coincides with the change in the Meridional Overturning Circulation (MOC) at 26.5N as observed by the RAPID project, and with extreme behavior of the wind-stress gyre mode and of atmospheric blocking. While the general relationship between northern warming and AMOC volume transport remains undetermined, the meridional heat- and salt transport carried by AMOC's arteries are rich with decade-to-century timescale variability.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20267" xmlns="http://purl.org/rss/1.0/"><title>Observations of wave energy fluxes and swash motions on a low-sloping, dissipative beach</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20267</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Observations of wave energy fluxes and swash motions on a low-sloping, dissipative beach</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rafael M. C. Guedes, Karin R. Bryan, Giovanni Coco</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-15T05:11:40.043515-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20267</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20267</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20267</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Field observations of swash and ocean waves show that runup saturation at infragravity frequencies (&lt; 0.05 Hz) can occur under mild offshore energy conditions if the beach slope is sufficiently gentle. Infragravity saturation was observed for higher-frequency (&gt; 0.025–0.035 Hz) infragravity waves, where typically less than 5% of the (linear) energy flux was reflected from the beach and where, similar to the sea-swell band, the swash energy was independent of offshore wave energy. The infragravity frequency range of saturation was determined by the tide, with saturation extending to lower frequencies at low tide when the local beach face slope over the concave-shaped profile was gentler. Runup was strongly dominated by infragravity frequencies, which accounted on average for 96% of the runup variance, and its energy levels were entirely consistent with strong infragravity wave dissipation observed in the surfzone, particularly when including the nonlinear contributions to the wave energy fluxes. The infragravity wave dissipation was strongly associated with breaking of sea-swell waves, which abruptly decreased nonlinear transfers to infragravity frequencies and made infragravity dissipation prevail over forcing within the breaking region. Our observations show evidence of nonlinear interactions involving infragravity and high-frequency, harmonic waves, and suggest that these harmonics could play a role in the wave energy balance near the shoreline on low-sloping, dissipative beaches.</p></div>
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Field observations of swash and ocean waves show that runup saturation at infragravity frequencies (&lt; 0.05 Hz) can occur under mild offshore energy conditions if the beach slope is sufficiently gentle. Infragravity saturation was observed for higher-frequency (&gt; 0.025–0.035 Hz) infragravity waves, where typically less than 5% of the (linear) energy flux was reflected from the beach and where, similar to the sea-swell band, the swash energy was independent of offshore wave energy. The infragravity frequency range of saturation was determined by the tide, with saturation extending to lower frequencies at low tide when the local beach face slope over the concave-shaped profile was gentler. Runup was strongly dominated by infragravity frequencies, which accounted on average for 96% of the runup variance, and its energy levels were entirely consistent with strong infragravity wave dissipation observed in the surfzone, particularly when including the nonlinear contributions to the wave energy fluxes. The infragravity wave dissipation was strongly associated with breaking of sea-swell waves, which abruptly decreased nonlinear transfers to infragravity frequencies and made infragravity dissipation prevail over forcing within the breaking region. Our observations show evidence of nonlinear interactions involving infragravity and high-frequency, harmonic waves, and suggest that these harmonics could play a role in the wave energy balance near the shoreline on low-sloping, dissipative beaches.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20266" xmlns="http://purl.org/rss/1.0/"><title>Sea ice freeboard in McMurdo Sound, Antarctica, derived by surface-validated ICESat laser altimeter data</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20266</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea ice freeboard in McMurdo Sound, Antarctica, derived by surface-validated ICESat laser altimeter data</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Daniel Price, Wolfgang Rack, Christian Haas, Pat. J. Langhorne, Oliver Marsh</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-13T23:52:50.592282-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20266</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20266</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20266</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Previous investigations have linked changes in the multiyear sea ice area of McMurdo Sound, Antarctica, from 1213 km<sup>2</sup> in 2003 to 4923 km<sup>2</sup> in 2005, to the passage of large tabular icebergs preventing the annual sea ice breakout. This maximum coverage then gradually diminished, by 2009 covering 1453 km<sup>2</sup>. This investigation employs the use of the ICESat laser altimeter to derive freeboard of sea ice in McMurdo Sound from 2003-2009 and hence infer thickness changes over this time period. Two techniques for freeboard retrieval are compared. Method-1 (M-1) follows those previously presented in the literature using the lowest elevations to construct an estimate of sea surface height. However the lack of leads in the study area motivated the development of Method-2 (M-2) which utilizes tide models. Each year is divided into two investigation periods from September to December and February to June, and these investigations were further segmented by sea ice type, first-year and multiyear. Both applied methods reveal a statistically significant linear increase in multiyear sea ice freeboard. For M-1 the mean freeboard increased over the study period from 0.53 m to 1.00 m and for M-2 from 0.46 m to 0.95 m. Evidence is presented that the multiyear sea ice freeboard increase is strongly linked to the development and incorporation of a sub-ice platelet layer. No statistically significant trends were observed for first-year sea ice. ICESat derived freeboards over first-year and multiyear sea ice areas compare within one standard deviation of airborne measured freeboard in November 2009.</p></div>
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Previous investigations have linked changes in the multiyear sea ice area of McMurdo Sound, Antarctica, from 1213 km2 in 2003 to 4923 km2 in 2005, to the passage of large tabular icebergs preventing the annual sea ice breakout. This maximum coverage then gradually diminished, by 2009 covering 1453 km2. This investigation employs the use of the ICESat laser altimeter to derive freeboard of sea ice in McMurdo Sound from 2003-2009 and hence infer thickness changes over this time period. Two techniques for freeboard retrieval are compared. Method-1 (M-1) follows those previously presented in the literature using the lowest elevations to construct an estimate of sea surface height. However the lack of leads in the study area motivated the development of Method-2 (M-2) which utilizes tide models. Each year is divided into two investigation periods from September to December and February to June, and these investigations were further segmented by sea ice type, first-year and multiyear. Both applied methods reveal a statistically significant linear increase in multiyear sea ice freeboard. For M-1 the mean freeboard increased over the study period from 0.53 m to 1.00 m and for M-2 from 0.46 m to 0.95 m. Evidence is presented that the multiyear sea ice freeboard increase is strongly linked to the development and incorporation of a sub-ice platelet layer. No statistically significant trends were observed for first-year sea ice. ICESat derived freeboards over first-year and multiyear sea ice areas compare within one standard deviation of airborne measured freeboard in November 2009.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20249" xmlns="http://purl.org/rss/1.0/"><title>The relationship between oxygen, nitrate and phosphate in the world ocean based on potential temperature</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20249</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The relationship between oxygen, nitrate and phosphate in the world ocean based on potential temperature</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Miho Ishizu, Kelvin J. Richards</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-13T15:15:22.026382-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20249</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20249</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20249</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Research Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The relationship between the biogeochemical major elements P/C/N/O<sub>,</sub> in the world ocean has been recognized as being elusive. Here we demonstrate that this elusiveness is caused by the difficulty of separating waters of different origin. These difficulties are reduced if the potential temperature of the water is considered. We employ data obtained from the World Ocean Circulation Experiment Hydrographic Program of oxygen, nitrate and phosphate. By stratifying these data with respect to potential temperature clear regression lines emerge between oxygen and nitrate/phosphate. The correlation coefficients are -0.95 and -0.95, respectively. The advantage of using potential temperature (rather than potential or neutral density) comes about because of the strong dependency of oxygen saturation with respect to temperature. In most of the global ocean the ratio of O<sub>2</sub>/P/N is found to be close to the Redfield ratio. The exception is colder waters originating in the nutrient rich surface water of the Southern Ocean and North Pacific. From the data alone it is difficult to determine if the non-Redfield ratios are brought about by different stoichiometry or ocean mixing, but our results put strong constraints on mixing and the biogeochemistry in the global ocean.</p></div>
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The relationship between the biogeochemical major elements P/C/N/O, in the world ocean has been recognized as being elusive. Here we demonstrate that this elusiveness is caused by the difficulty of separating waters of different origin. These difficulties are reduced if the potential temperature of the water is considered. We employ data obtained from the World Ocean Circulation Experiment Hydrographic Program of oxygen, nitrate and phosphate. By stratifying these data with respect to potential temperature clear regression lines emerge between oxygen and nitrate/phosphate. The correlation coefficients are -0.95 and -0.95, respectively. The advantage of using potential temperature (rather than potential or neutral density) comes about because of the strong dependency of oxygen saturation with respect to temperature. In most of the global ocean the ratio of O2/P/N is found to be close to the Redfield ratio. The exception is colder waters originating in the nutrient rich surface water of the Southern Ocean and North Pacific. From the data alone it is difficult to determine if the non-Redfield ratios are brought about by different stoichiometry or ocean mixing, but our results put strong constraints on mixing and the biogeochemistry in the global ocean.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20265" xmlns="http://purl.org/rss/1.0/"><title>Recent changes in the exchange of sea ice between the Arctic Ocean and the Canadian Arctic Archipelago</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20265</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Recent changes in the exchange of sea ice between the Arctic Ocean and the Canadian Arctic Archipelago</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Stephen L. Howell, Trudy Wohlleben, Mohammed Dabboor, Chris Derksen, Alexander Komarov, Larissa Pizzolato</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-07T02:49:38.236023-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20265</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20265</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20265</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Sea ice is exchanged between the Arctic Ocean and Canadian Arctic Archipelago (CAA) but has not been quantified over long time periods. The corresponding mechanisms responsible for recent variability and change also remain unidentified. To address this, we estimated the sea ice area flux between the Arctic Ocean and the M'Clure Strait and Queen Elizabeth Islands (QEI) from 1997-2012 for the months of May to November. Over the period, there was a mean flux of -1x10<sup>3</sup> km<sup>2</sup> (±21×10<sup>3</sup> km<sup>2</sup>) at the M'Clure Strait and mean flux of +8×10<sup>3</sup> km<sup>2</sup> (±8×10<sup>3</sup> km<sup>2</sup>) at the QEI (positive and negative flux signs correspond to Arctic Ocean ice inflow and outflow, respectively). The M'Clure Strait had a mean flux of +5×10<sup>3</sup> km<sup>2</sup> from May to September and a mean flux of -7×10<sup>3</sup> km<sup>2</sup> from October to November. The QEI gates had a mean flux of +4×10<sup>3</sup> km<sup>2</sup> from August to September with negligible ice exchange from May to July and October to November. More frequent high sea level pressure anomalies over the Beaufort Sea and Canadian Basin since 2007 have reduced Arctic Ocean multi-year ice (MYI) inflow into the M'Clure Strait. The presence of MYI in the CAA originating from the Arctic Ocean has been maintained by inflow at the QEI, which has increased since 2005. These recent increases in Arctic Ocean MYI inflow into the QEI can be attributed to increased open water area within the CAA that have provided more leeway for inflow to occur.</p></div>
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Sea ice is exchanged between the Arctic Ocean and Canadian Arctic Archipelago (CAA) but has not been quantified over long time periods. The corresponding mechanisms responsible for recent variability and change also remain unidentified. To address this, we estimated the sea ice area flux between the Arctic Ocean and the M'Clure Strait and Queen Elizabeth Islands (QEI) from 1997-2012 for the months of May to November. Over the period, there was a mean flux of -1x103 km2 (±21×103 km2) at the M'Clure Strait and mean flux of +8×103 km2 (±8×103 km2) at the QEI (positive and negative flux signs correspond to Arctic Ocean ice inflow and outflow, respectively). The M'Clure Strait had a mean flux of +5×103 km2 from May to September and a mean flux of -7×103 km2 from October to November. The QEI gates had a mean flux of +4×103 km2 from August to September with negligible ice exchange from May to July and October to November. More frequent high sea level pressure anomalies over the Beaufort Sea and Canadian Basin since 2007 have reduced Arctic Ocean multi-year ice (MYI) inflow into the M'Clure Strait. The presence of MYI in the CAA originating from the Arctic Ocean has been maintained by inflow at the QEI, which has increased since 2005. These recent increases in Arctic Ocean MYI inflow into the QEI can be attributed to increased open water area within the CAA that have provided more leeway for inflow to occur.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20264" xmlns="http://purl.org/rss/1.0/"><title>Detection of linear trends in multi-sensor time series in presence of auto-correlated noise: Application to the chlorophyll-a SeaWiFS and MERIS datasets and extrapolation to the incoming Sentinel 3 - OLCI mission</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20264</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Detection of linear trends in multi-sensor time series in presence of auto-correlated noise: Application to the chlorophyll-a SeaWiFS and MERIS datasets and extrapolation to the incoming Sentinel 3 - OLCI mission</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Bertrand Saulquin, Ronan Fablet, Antoine Mangin, Grégoire Mercier, David Antoine, Odile Fanton d'Andon</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-07T02:43:39.132645-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20264</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20264</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20264</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The detection of long-term trends in geophysical time series is a key issue in climate change studies. This detection is affected by many factors: the size of the trend to be detected, the length of the available datasets, and the noise properties. Although the noise auto-correlation observed in geophysical time series does not bias the trend estimate, it affects the estimation of its uncertainty and consequently the ability to detect, or not, a significant trend. Ignoring the noise auto-correlation level typically leads to an over-detection of significant trends.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Satellite time series have been providing remote observations of the sea surface for several decades. Due to satellite lifetime, usually between 5 and 10 years, these time series do not cover the same period and are acquired by different sensors with different characteristics. These differences lead to unknown level shifts (biases) between the datasets, which affect the trend detection.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>In this work, we develop a generic framework to detect and evaluate linear trends and level shifts in multi-sensor time series of satellite chlorophyll-a concentrations, as provided by the MERIS and SeaWiFS ocean color missions. We also discuss the optimization of the observation networks, in terms of needed time overlap between successive time series in order to reduce the uncertainty on the detection of long-term trends. For the incoming Sentinel-3 - OLCI mission that should be launched at the end of 2014, we propose a global map of the duration of this future time series necessary to actually enhance the trend detection performed with the joint SeaWiFS-MERIS analysis.</p></div>
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The detection of long-term trends in geophysical time series is a key issue in climate change studies. This detection is affected by many factors: the size of the trend to be detected, the length of the available datasets, and the noise properties. Although the noise auto-correlation observed in geophysical time series does not bias the trend estimate, it affects the estimation of its uncertainty and consequently the ability to detect, or not, a significant trend. Ignoring the noise auto-correlation level typically leads to an over-detection of significant trends.
Satellite time series have been providing remote observations of the sea surface for several decades. Due to satellite lifetime, usually between 5 and 10 years, these time series do not cover the same period and are acquired by different sensors with different characteristics. These differences lead to unknown level shifts (biases) between the datasets, which affect the trend detection.
In this work, we develop a generic framework to detect and evaluate linear trends and level shifts in multi-sensor time series of satellite chlorophyll-a concentrations, as provided by the MERIS and SeaWiFS ocean color missions. We also discuss the optimization of the observation networks, in terms of needed time overlap between successive time series in order to reduce the uncertainty on the detection of long-term trends. For the incoming Sentinel-3 - OLCI mission that should be launched at the end of 2014, we propose a global map of the duration of this future time series necessary to actually enhance the trend detection performed with the joint SeaWiFS-MERIS analysis.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20263" xmlns="http://purl.org/rss/1.0/"><title>Effects of exopolymers on particle size distributions of suspended cohesive sediments</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20263</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Effects of exopolymers on particle size distributions of suspended cohesive sediments</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Guoping Zhang, Hang Yin, Zhenyu Lei, Allen H. Reed, Yoko Furukawa</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-07T02:38:37.507247-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20263</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20263</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20263</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The effects of exopolymers on the particle size distributions (PSD) of suspended cohesive sediments were investigated in laboratory using four abundant clay minerals, kaolinite, illite, Na-montmorillonite, and Ca-montmorillonite, and two exopolymers, xanthan and guar, at six different exopolymer to clay ratios (E/C) (i.e., 0, 1, 2, 5, 10, and 20 wt.%) to represent the compositional variability of cohesive sediments in natural waters. Results show that the clay-exopolymer suspensions possess multimodal PSD. Statistical deconvolution of the PSD curves indicates that the suspensions consist of four discrete particle groups, primary particles, flocculi, microflocs, and macroflocs, all of which exhibit a unimodal lognormal distribution. Furthermore, such deconvolution quantifies the mean size and fraction of each particle group, leading to a more quantitative understanding of PSD kinetics of these sediments. Both clay surface charges and exopolymer polarity as well as the E/C affect the PSD kinetics. While neutral guar causes flocculation for all four clay minerals, anionic xanthan only induces flocculation for kaolinite with very low surface charges, but not for the other three clay minerals with relatively high charges. The fraction of each particle group also varies with the E/C, and such complex changes depend upon the interfacial interactions between clay particles and exopolymer molecules. For each exopolymer, critical E/C exist that can lead to a maximum or minimum fraction of microflocs or macroflocs. The role of exopolymer bridging, Coulomb force, and hydrogen bond in affecting the PSD kinetics of cohesive sediments is also discussed.</p></div>
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The effects of exopolymers on the particle size distributions (PSD) of suspended cohesive sediments were investigated in laboratory using four abundant clay minerals, kaolinite, illite, Na-montmorillonite, and Ca-montmorillonite, and two exopolymers, xanthan and guar, at six different exopolymer to clay ratios (E/C) (i.e., 0, 1, 2, 5, 10, and 20 wt.%) to represent the compositional variability of cohesive sediments in natural waters. Results show that the clay-exopolymer suspensions possess multimodal PSD. Statistical deconvolution of the PSD curves indicates that the suspensions consist of four discrete particle groups, primary particles, flocculi, microflocs, and macroflocs, all of which exhibit a unimodal lognormal distribution. Furthermore, such deconvolution quantifies the mean size and fraction of each particle group, leading to a more quantitative understanding of PSD kinetics of these sediments. Both clay surface charges and exopolymer polarity as well as the E/C affect the PSD kinetics. While neutral guar causes flocculation for all four clay minerals, anionic xanthan only induces flocculation for kaolinite with very low surface charges, but not for the other three clay minerals with relatively high charges. The fraction of each particle group also varies with the E/C, and such complex changes depend upon the interfacial interactions between clay particles and exopolymer molecules. For each exopolymer, critical E/C exist that can lead to a maximum or minimum fraction of microflocs or macroflocs. The role of exopolymer bridging, Coulomb force, and hydrogen bond in affecting the PSD kinetics of cohesive sediments is also discussed.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20261" xmlns="http://purl.org/rss/1.0/"><title>Creation and tidal advection of a cold salinity front in Storfjorden. Part 2: Supercooling induced by turbulent mixing of cold water</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20261</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Creation and tidal advection of a cold salinity front in Storfjorden. Part 2: Supercooling induced by turbulent mixing of cold water</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Miles G. McPhee, Ragnheid Skogseth, Frank Nilsen, Lars H. Smedsrud</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-06T11:04:16.860356-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20261</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20261</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20261</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Measurements near the edge of fast ice in Freemansundet, Svalbard, reveal mixing processes associated with tidal advection of a sharp front in salinity, including possible supercooling induced by double diffusion in a fully turbulent water column. The front translated back and forth with the semidiurnal tide between an area of mobile (drifting) ice in Storfjorden proper, and the narrow sound covered by fast ice. Water on each side of the front was near its salinity-determined freezing temperature. Instruments deployed about 400 m into the sound from the fast ice edge measured current, temperature, conductivity, and turbulence quantities through several tidal cycles. Turbulence data illustrate that as the steep horizontal salinity (density) gradient advected past the measurement site, vertical shear near the fast-ice base induced marked flood/ebb asymmetry in turbulent mixing. As fresher water entered the sound on the flood phase, inward transport of denser water near the upper boundary was retarded, leading to statically unstable conditions and enhanced turbulence. The opposite occurred during ebb tide, as denser water under-ran lighter. Transient episodes of supercooling accompanied frontal passage on both flood and ebb phases. The most likely explanation for a zone of supercooled water within the strongly mixed frontal region is that during mixing of fresher, slightly warmer (but still at freezing) water from outside with saltier, colder water in the sound, the former constituent lost heat faster than gaining salt. This interpretation (differing turbulent diffusivities for heat and salt) challenges strict application of Reynolds analogy for highly turbulent shear flow.</p></div>
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Measurements near the edge of fast ice in Freemansundet, Svalbard, reveal mixing processes associated with tidal advection of a sharp front in salinity, including possible supercooling induced by double diffusion in a fully turbulent water column. The front translated back and forth with the semidiurnal tide between an area of mobile (drifting) ice in Storfjorden proper, and the narrow sound covered by fast ice. Water on each side of the front was near its salinity-determined freezing temperature. Instruments deployed about 400 m into the sound from the fast ice edge measured current, temperature, conductivity, and turbulence quantities through several tidal cycles. Turbulence data illustrate that as the steep horizontal salinity (density) gradient advected past the measurement site, vertical shear near the fast-ice base induced marked flood/ebb asymmetry in turbulent mixing. As fresher water entered the sound on the flood phase, inward transport of denser water near the upper boundary was retarded, leading to statically unstable conditions and enhanced turbulence. The opposite occurred during ebb tide, as denser water under-ran lighter. Transient episodes of supercooling accompanied frontal passage on both flood and ebb phases. The most likely explanation for a zone of supercooled water within the strongly mixed frontal region is that during mixing of fresher, slightly warmer (but still at freezing) water from outside with saltier, colder water in the sound, the former constituent lost heat faster than gaining salt. This interpretation (differing turbulent diffusivities for heat and salt) challenges strict application of Reynolds analogy for highly turbulent shear flow.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20262" xmlns="http://purl.org/rss/1.0/"><title>An integrated approach to the heat and water mass dynamics of a large bay: High-resolution simulations of Funka Bay, Japan</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20262</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">An integrated approach to the heat and water mass dynamics of a large bay: High-resolution simulations of Funka Bay, Japan</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Satoshi Nakada, Yoichi Ishikawa, Toshiyuki Awaji, Teiji In, Koji Koyamada, Masamichi Watanobe, Hiroya Okumura, Yoshinori Nishida, Sei-Ichi Saitoh</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-06T11:02:35.764353-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20262</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20262</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20262</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">ABSTRACT</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Heat and water mass transports tagged by water type in a bay were investigated using daily outputs from a high-resolution land–sea coupled model. The modeled circulation and water property distribution were similar to those reported by observations. In this paper, the heat angle is introduced to accurately define the roles of the lateral heat flux (<em>LF</em>) into the bay and the net surface heat flux on temperature changes in the bay water. As a result, ocean phenomena in the bay can be categorized by using the heat angle in an intensive <em>LF</em> regime on short-period timescales and a gradual <em>LF</em> regime on intra-seasonal timescales. Our close examination revealed that the velocity fields can be classified into three flow patterns: a twin vortex accompanied by positive <em>LF</em>, a clockwise flow with negative <em>LF</em>, and an anticlockwise flow with both <em>LF</em>s. These patterns occur in both intensive and gradual <em>LF</em> regimes. Intensive wind-driven <em>LF</em> forced by atmospheric disturbances was often observed from summer to autumn in 2008 accompanying the intrusion of southern subtropical Tsugaru warm water that was colder than the deep bay water (<em>LF</em> &lt; 0) and subarctic Oyashio water that was warmer than the surface bay water (<em>LF</em> &gt; 0), but both were hardly found in 2009. This thermal contrast affects the interannual difference in the stratification inherent in the bay. Our integrated analysis method is useful for prompt and robust understanding of the thermal and dynamic states in a bay based on ocean simulation data.</p></div>
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Heat and water mass transports tagged by water type in a bay were investigated using daily outputs from a high-resolution land–sea coupled model. The modeled circulation and water property distribution were similar to those reported by observations. In this paper, the heat angle is introduced to accurately define the roles of the lateral heat flux (LF) into the bay and the net surface heat flux on temperature changes in the bay water. As a result, ocean phenomena in the bay can be categorized by using the heat angle in an intensive LF regime on short-period timescales and a gradual LF regime on intra-seasonal timescales. Our close examination revealed that the velocity fields can be classified into three flow patterns: a twin vortex accompanied by positive LF, a clockwise flow with negative LF, and an anticlockwise flow with both LFs. These patterns occur in both intensive and gradual LF regimes. Intensive wind-driven LF forced by atmospheric disturbances was often observed from summer to autumn in 2008 accompanying the intrusion of southern subtropical Tsugaru warm water that was colder than the deep bay water (LF &lt; 0) and subarctic Oyashio water that was warmer than the surface bay water (LF &gt; 0), but both were hardly found in 2009. This thermal contrast affects the interannual difference in the stratification inherent in the bay. Our integrated analysis method is useful for prompt and robust understanding of the thermal and dynamic states in a bay based on ocean simulation data.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20260" xmlns="http://purl.org/rss/1.0/"><title>Generalized Linear Modeling of the El Niño/Southern Oscillation with Application to Seasonal Forecasting and Climate Change Projections</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20260</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Generalized Linear Modeling of the El Niño/Southern Oscillation with Application to Seasonal Forecasting and Climate Change Projections</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. Stevenson, B. Rajagopalan, B. Fox-Kemper</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-06T11:02:28.734949-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20260</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20260</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20260</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>A new framework for simulating the El Niño/Southern Oscillation (ENSO) using a generalized linear model (GLM) is provided. The GLM provides a versatile and computationally inexpensive method for investigating ENSO dynamics, by conditioning an ENSO index on an arbitrary set of input variables. Here, the system state (El Niño/neutral/La Niña) at previous times is combined with the first few principal components of SST and thermocline depth. Despite having relatively few degrees of freedom, the model accurately reproduces 20th century SST time series, seasonal variance, power spectra and autocorrelation functions for both the eastern and western Pacific. The GLM also has good overall forecast skill, especially at sub-yearly lead times; performance is competitive with models currently used for operational ENSO forecasting. The model is then used to examine changes to El Niño/La Niña statistics under CO<sub>2</sub> increases, by using the GLM to represent simulations run with the NCAR Community Climate System Model, versions 3.5 and 4. GLM simulations of 21st century CCSM4 changes to El Niño/La Niña magnitudes show insignificant results, despite a slight increase in El Niño persistence. GLM fits conditioned on millennial stabilized CCSM3.5 simulations with varying CO<sub>2</sub> levels, however, show a weakening and shortening of El Niño events as CO<sub>2</sub> concentration increases, while La Niña events become markedly stronger and do not change significantly in length. The reduction in El Niño persistence in CCSM3.5 is consistent with previous results showing that at higher CO<sub>2</sub> levels, a stronger seasonal cycle creates a Southern Hemisphere ‘seasonal footprint’ leading to more efficient El Niño termination.</p></div>
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A new framework for simulating the El Niño/Southern Oscillation (ENSO) using a generalized linear model (GLM) is provided. The GLM provides a versatile and computationally inexpensive method for investigating ENSO dynamics, by conditioning an ENSO index on an arbitrary set of input variables. Here, the system state (El Niño/neutral/La Niña) at previous times is combined with the first few principal components of SST and thermocline depth. Despite having relatively few degrees of freedom, the model accurately reproduces 20th century SST time series, seasonal variance, power spectra and autocorrelation functions for both the eastern and western Pacific. The GLM also has good overall forecast skill, especially at sub-yearly lead times; performance is competitive with models currently used for operational ENSO forecasting. The model is then used to examine changes to El Niño/La Niña statistics under CO2 increases, by using the GLM to represent simulations run with the NCAR Community Climate System Model, versions 3.5 and 4. GLM simulations of 21st century CCSM4 changes to El Niño/La Niña magnitudes show insignificant results, despite a slight increase in El Niño persistence. GLM fits conditioned on millennial stabilized CCSM3.5 simulations with varying CO2 levels, however, show a weakening and shortening of El Niño events as CO2 concentration increases, while La Niña events become markedly stronger and do not change significantly in length. The reduction in El Niño persistence in CCSM3.5 is consistent with previous results showing that at higher CO2 levels, a stronger seasonal cycle creates a Southern Hemisphere ‘seasonal footprint’ leading to more efficient El Niño termination.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20255" xmlns="http://purl.org/rss/1.0/"><title>Modeling particle aggregation using size class and size spectrum approaches</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20255</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Modeling particle aggregation using size class and size spectrum approaches</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Adrian B. Burd</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-05T11:13:56.650001-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20255</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20255</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20255</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Particle aggregation plays an important role in many marine biogeochemical processes such as determining the vertical flux of particulate material and trace metal scavenging. Models of particle aggregation vary in complexity and in this paper I compare the behavior of a detailed size-spectrum model with that of a series of simple, two size-class models with different representations of aggregation, all of which have appeared in the literature. The simplest model uses a first-order representation of aggregation kinetics, while two other models have non-linear representations of aggregation. The simplest model is unable to reproduce the dynamic or steady-state behavior of the size-spectrum model. Results from the two non-linear size-class models show better agreement with the behavior of the size-spectrum model. I find that the mode of aggregation and the dependence of aggregation on particle size are crucial for understanding the differences between the models.</p></div>
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Particle aggregation plays an important role in many marine biogeochemical processes such as determining the vertical flux of particulate material and trace metal scavenging. Models of particle aggregation vary in complexity and in this paper I compare the behavior of a detailed size-spectrum model with that of a series of simple, two size-class models with different representations of aggregation, all of which have appeared in the literature. The simplest model uses a first-order representation of aggregation kinetics, while two other models have non-linear representations of aggregation. The simplest model is unable to reproduce the dynamic or steady-state behavior of the size-spectrum model. Results from the two non-linear size-class models show better agreement with the behavior of the size-spectrum model. I find that the mode of aggregation and the dependence of aggregation on particle size are crucial for understanding the differences between the models.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20257" xmlns="http://purl.org/rss/1.0/"><title>Assessing the quality of sea surface temperature observations from drifting buoys and ships on a platform-by-platform basis</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20257</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Assessing the quality of sea surface temperature observations from drifting buoys and ships on a platform-by-platform basis</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Christopher P. Atkinson, Nick A. Rayner, Jonah Roberts-Jones, Robert O. Smith</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-05T11:13:49.895397-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20257</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20257</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20257</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This study investigates how the quality of sea surface temperature (SST) observations made by drifting buoys (drifters) and ships for 1996-2010 can be improved through retrospective quality control (QC) against a reference field. The observations used are a blend of delayed mode data taken from the International Comprehensive Ocean-Atmosphere Data Set (versions 2.0 and 2.5) and real time data obtained from the Global Telecommunication System. A comparison of drifter and ship measurements on a platform-by-platform basis to high quality SST estimates from the ATSR Reprocessing for Climate (ARC) project reveals drifter observations are generally of good quality but frequently suffer from gross errors, whilst ship observations are generally of worse quality and show a diverse range of measurement errors. QC procedures are developed which similarly assess drifter and ship SST observations through comparison with the Met Office Operational SST and Sea Ice Analysis (OSTIA). These procedures make use of seasonal background error variance estimates now available for OSTIA. Drifter observations displaying some commonly observed gross errors are flagged and ship callsigns whose observations are deemed unreliable are blacklisted. Validation of the QC outcomes against ARC and Argo demonstrates that this retrospective QC improves the quality of drifter and ship observations, though some limitations are discussed.</p></div>
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This study investigates how the quality of sea surface temperature (SST) observations made by drifting buoys (drifters) and ships for 1996-2010 can be improved through retrospective quality control (QC) against a reference field. The observations used are a blend of delayed mode data taken from the International Comprehensive Ocean-Atmosphere Data Set (versions 2.0 and 2.5) and real time data obtained from the Global Telecommunication System. A comparison of drifter and ship measurements on a platform-by-platform basis to high quality SST estimates from the ATSR Reprocessing for Climate (ARC) project reveals drifter observations are generally of good quality but frequently suffer from gross errors, whilst ship observations are generally of worse quality and show a diverse range of measurement errors. QC procedures are developed which similarly assess drifter and ship SST observations through comparison with the Met Office Operational SST and Sea Ice Analysis (OSTIA). These procedures make use of seasonal background error variance estimates now available for OSTIA. Drifter observations displaying some commonly observed gross errors are flagged and ship callsigns whose observations are deemed unreliable are blacklisted. Validation of the QC outcomes against ARC and Argo demonstrates that this retrospective QC improves the quality of drifter and ship observations, though some limitations are discussed.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20256" xmlns="http://purl.org/rss/1.0/"><title>Spatial variability of the wave bottom boundary layer over movable rippled beds</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20256</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Spatial variability of the wave bottom boundary layer over movable rippled beds</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. Rodríguez-Abudo, D. L. Foster, M. Henriquez</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-05T11:10:42.587098-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20256</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20256</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20256</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Observations of the spatially dependent velocity field over movable bedforms subjected to slightly skewed and asymmetric regular wave forcing were collected. The dynamics between the ripple elements is dominated by coherent vortices, characterized by the swirling strength, and evidenced in the temporal and spectral characterization. Within the boundary layer, spectral energy in the second harmonic (3<em>f</em><sub>0</sub>) is amplified at the ripple slopes and is consistent with the location of the expected strongest pressure gradients. First- and second-moment velocity statistics were used to address the spatial variability of the intra-ripple hydrodynamics. Estimates of displacement and momentum thicknesses (δ* and δ<em><sub>mom</sub></em>), are smaller than suggested by the higher harmonics, but consistently highlight areas of adverse and favorable pressure gradients. Shear stress and roughness estimates were inferred by fitting a logarithmic model to first- and second-moment statistics of the velocity field. The maximum Shields parameter was observed to peak at the stoss slope of asymmetric ripples during the strongest and shorter half-wave period (onshore). First-moment roughness estimates are similar in magnitude to bedload parameterizations provided by <em>Li et al</em>. [1997], and about a factor of 3 larger than second-moment estimates. Assessment of the vertical transfer of horizontal momentum derived using a Reynolds decomposition, suggests that stresses inferred from the logarithmic law using first-moment velocity statistics appropriately reproduce the mean momentum transfer for the longer and weaker offshore half-wave period.</p></div>
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Observations of the spatially dependent velocity field over movable bedforms subjected to slightly skewed and asymmetric regular wave forcing were collected. The dynamics between the ripple elements is dominated by coherent vortices, characterized by the swirling strength, and evidenced in the temporal and spectral characterization. Within the boundary layer, spectral energy in the second harmonic (3f0) is amplified at the ripple slopes and is consistent with the location of the expected strongest pressure gradients. First- and second-moment velocity statistics were used to address the spatial variability of the intra-ripple hydrodynamics. Estimates of displacement and momentum thicknesses (δ* and δmom), are smaller than suggested by the higher harmonics, but consistently highlight areas of adverse and favorable pressure gradients. Shear stress and roughness estimates were inferred by fitting a logarithmic model to first- and second-moment statistics of the velocity field. The maximum Shields parameter was observed to peak at the stoss slope of asymmetric ripples during the strongest and shorter half-wave period (onshore). First-moment roughness estimates are similar in magnitude to bedload parameterizations provided by Li et al. [1997], and about a factor of 3 larger than second-moment estimates. Assessment of the vertical transfer of horizontal momentum derived using a Reynolds decomposition, suggests that stresses inferred from the logarithmic law using first-moment velocity statistics appropriately reproduce the mean momentum transfer for the longer and weaker offshore half-wave period.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20258" xmlns="http://purl.org/rss/1.0/"><title>The impact of rapid coastline changes and sea level rise on the tides in the Bohai Sea, China</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20258</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The impact of rapid coastline changes and sea level rise on the tides in the Bohai Sea, China</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">H. E. Pelling, K. Uehara, J. A. M. Green</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-05T11:01:15.192073-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20258</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20258</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20258</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The tidal regime in the Bohai Sea, China, is investigated using observations and an established numerical tidal model. The area has recently experienced rapid coastline changes due to natural developments of the Yellow River delta and large-scale anthropogenic land reclamation. These morphological changes are not reflected in most global bathymetric databases and are thus rarely incorporated into investigations of the Bohai Sea. It is shown that there have indeed been significant changes in the tidal regime in the Bohai Sea over the last 35 years, with <em>M<sub>2</sub></em> amplitudes changing up to 20 cm in some parts. The model captures some of these changes when the appropriate bathymetries are used. Furthermore, the simulations show that the tides in the Bohai Sea have become more sensitive to future sea level rise and the way in which it is implemented in the model (i.e. whether or not flood defenses are included).These sensitivity changes are due to the recent coastal developments.</p></div>
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The tidal regime in the Bohai Sea, China, is investigated using observations and an established numerical tidal model. The area has recently experienced rapid coastline changes due to natural developments of the Yellow River delta and large-scale anthropogenic land reclamation. These morphological changes are not reflected in most global bathymetric databases and are thus rarely incorporated into investigations of the Bohai Sea. It is shown that there have indeed been significant changes in the tidal regime in the Bohai Sea over the last 35 years, with M2 amplitudes changing up to 20 cm in some parts. The model captures some of these changes when the appropriate bathymetries are used. Furthermore, the simulations show that the tides in the Bohai Sea have become more sensitive to future sea level rise and the way in which it is implemented in the model (i.e. whether or not flood defenses are included).These sensitivity changes are due to the recent coastal developments.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20259" xmlns="http://purl.org/rss/1.0/"><title>Variability and trends of ocean acidification in the Southern California Current System: A timeseries from Santa Monica Bay</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20259</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Variability and trends of ocean acidification in the Southern California Current System: A timeseries from Santa Monica Bay</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">A. Leinweber, N. Gruber</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-05T10:53:18.690536-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20259</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20259</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20259</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>We investigate the temporal variability and trends of pH and of the aragonite saturation state, Ω<em><sub>arag</sub></em>, in the southern California Current System on the basis of a 6 year timeseries from Santa Monica Bay, using bi-weekly observations of dissolved inorganic carbon and combined calculated and measured alkalinity. Median values of pH and Ω<em><sub>arag</sub></em> in the upper 20 m are comparable to observations from the subtropical gyres, but the temporal variability is at least a factor of 5 larger, primarily driven by short-term upwelling events and mesoscale processes. Ω<em><sub>arag</sub></em> and pH decrease rapidly with depth, such that the saturation horizon is reached already at 130 m, on average, but it occasionally shoals to as low as 30 m. No statistically significant linear trends emerge in the upper 100 m, but Ω<em><sub>arag</sub></em> and pH decrease, on average, at rates of -0.009 ± 0.006 yr<sup>-1</sup> and -0.004 ± 0.003 yr<sup>-1</sup> in the 100 to 250 m depth range. These are somewhat larger, but not statistically different from the expected trends based on the recent increase in atmospheric CO<sub>2</sub>. About half of the variability in the deseasonalized data can be explained by the El Niño Southern Oscillation (ENSO), with warm phases (El Niño) being associated with above normal pH and Ω<em><sub>arag</sub></em>. The observed variability and trend in Ω<em><sub>arag</sub></em> and pH is well captured by a multiple linear regression model on the basis of a small number of readily observable independent variables. This permits the estimation of these variables for related sites in the region.</p></div>
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We investigate the temporal variability and trends of pH and of the aragonite saturation state, Ωarag, in the southern California Current System on the basis of a 6 year timeseries from Santa Monica Bay, using bi-weekly observations of dissolved inorganic carbon and combined calculated and measured alkalinity. Median values of pH and Ωarag in the upper 20 m are comparable to observations from the subtropical gyres, but the temporal variability is at least a factor of 5 larger, primarily driven by short-term upwelling events and mesoscale processes. Ωarag and pH decrease rapidly with depth, such that the saturation horizon is reached already at 130 m, on average, but it occasionally shoals to as low as 30 m. No statistically significant linear trends emerge in the upper 100 m, but Ωarag and pH decrease, on average, at rates of -0.009 ± 0.006 yr-1 and -0.004 ± 0.003 yr-1 in the 100 to 250 m depth range. These are somewhat larger, but not statistically different from the expected trends based on the recent increase in atmospheric CO2. About half of the variability in the deseasonalized data can be explained by the El Niño Southern Oscillation (ENSO), with warm phases (El Niño) being associated with above normal pH and Ωarag. The observed variability and trend in Ωarag and pH is well captured by a multiple linear regression model on the basis of a small number of readily observable independent variables. This permits the estimation of these variables for related sites in the region.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20247" xmlns="http://purl.org/rss/1.0/"><title>Insights into brine dynamics and sea-ice desalination from a 1D model study of gravity drainage</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20247</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Insights into brine dynamics and sea-ice desalination from a 1D model study of gravity drainage</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Philipp J. Griewank, Dirk Notz</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T02:30:29.740239-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20247</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20247</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20247</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>We study gravity drainage using a new one-dimensional, multi-phase sea-ice model. A parametrization of gravity drainage based on the convective nature of gravity drainage is introduced, whose free parameters are determined by optimizing model output against laboratory measurements of sea-ice salinity evolution. Optimal estimates of the free parameters as well as the parametrization performance remain stable for vertical grid resolutions from 1 to 30 mm. We find a strong link between sea-ice growth rate and bulk salinity for constant boundary conditions, but only a weak link for more realistic boundary conditions. We also demonstrate that surface warming can trigger brine convection over the whole ice layer. Over a growth season, replacing the convective parametrization with constant initial salinities leads to an overall 3 % discrepancy of stored energy, thermal resistance, and salt release. We also derive from our convective parametrization a simplified, numerically cheap and stable gravity-drainage parametrization. This parametrization results in an approximately 1 % discrepancy of stored energy, thermal resistance, and salt release compared to the convective parametrization. A similarly low discrepancy to our complex parametrization can be reached by simply prescribing a depth-dependent salinity profile.</p></div>
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We study gravity drainage using a new one-dimensional, multi-phase sea-ice model. A parametrization of gravity drainage based on the convective nature of gravity drainage is introduced, whose free parameters are determined by optimizing model output against laboratory measurements of sea-ice salinity evolution. Optimal estimates of the free parameters as well as the parametrization performance remain stable for vertical grid resolutions from 1 to 30 mm. We find a strong link between sea-ice growth rate and bulk salinity for constant boundary conditions, but only a weak link for more realistic boundary conditions. We also demonstrate that surface warming can trigger brine convection over the whole ice layer. Over a growth season, replacing the convective parametrization with constant initial salinities leads to an overall 3 % discrepancy of stored energy, thermal resistance, and salt release. We also derive from our convective parametrization a simplified, numerically cheap and stable gravity-drainage parametrization. This parametrization results in an approximately 1 % discrepancy of stored energy, thermal resistance, and salt release compared to the convective parametrization. A similarly low discrepancy to our complex parametrization can be reached by simply prescribing a depth-dependent salinity profile.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20254" xmlns="http://purl.org/rss/1.0/"><title>Physical drivers of interannual chlorophyll variability in the eastern subtropical North Atlantic</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20254</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Physical drivers of interannual chlorophyll variability in the eastern subtropical North Atlantic</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. V. Pastor, J. B. Palter, J.L. Pelegrí, J. P. Dunne</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T02:24:32.560533-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20254</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20254</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20254</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Interannual chlorophyll variability and its driving mechanisms are evaluated in the eastern subtropical North Atlantic, where elevated surface chlorophyll concentrations regularly extend more than 1500 km into the central subtropical North Atlantic and modulate the areal extent of the North Atlantic's lowest chlorophyll waters. We first characterize the considerable interannual variability in the size of the high chlorophyll region using SeaWiFS satellite data. We then evaluate the relationship between satellite chlorophyll and Sea Surface Height (SSH), which are anticorrelated in the study region, most likely as a result of the inverse relationship between SSH and nutricline depth. To put these results in a longer temporal context, we study a hindcast simulation of a global ocean model with biogeochemistry (GFDL's MOM4.1 with TOPAZ biogeochemistry), after evaluating the model's skill at simulating chlorophyll and SSH relative to observations. In the simulation, the variability seen during the satellite era appears to be imbedded in a much larger multidecadal modulation. The drivers of such variability are assessed by evaluating all the terms in the nutrient budget of the euphotic zone. Because diffusive processes are not a dominant control on nutrient supply, stratification is not a good indicator of nutrient supply. Rather, vertical advection of nutrients, strongly tied to Ekman pumping, is the leading driver of variability in the size of the high chlorophyll region and the productivity within the study area.</p></div>
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Interannual chlorophyll variability and its driving mechanisms are evaluated in the eastern subtropical North Atlantic, where elevated surface chlorophyll concentrations regularly extend more than 1500 km into the central subtropical North Atlantic and modulate the areal extent of the North Atlantic's lowest chlorophyll waters. We first characterize the considerable interannual variability in the size of the high chlorophyll region using SeaWiFS satellite data. We then evaluate the relationship between satellite chlorophyll and Sea Surface Height (SSH), which are anticorrelated in the study region, most likely as a result of the inverse relationship between SSH and nutricline depth. To put these results in a longer temporal context, we study a hindcast simulation of a global ocean model with biogeochemistry (GFDL's MOM4.1 with TOPAZ biogeochemistry), after evaluating the model's skill at simulating chlorophyll and SSH relative to observations. In the simulation, the variability seen during the satellite era appears to be imbedded in a much larger multidecadal modulation. The drivers of such variability are assessed by evaluating all the terms in the nutrient budget of the euphotic zone. Because diffusive processes are not a dominant control on nutrient supply, stratification is not a good indicator of nutrient supply. Rather, vertical advection of nutrients, strongly tied to Ekman pumping, is the leading driver of variability in the size of the high chlorophyll region and the productivity within the study area.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20250" xmlns="http://purl.org/rss/1.0/"><title>Seasonal mixed layer dynamics in an eddy-resolving ocean Circulation Model</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20250</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seasonal mixed layer dynamics in an eddy-resolving ocean Circulation Model</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Andreas Schiller, Ken R. Ridgway</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T02:23:12.800259-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20250</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20250</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20250</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Mean and seasonal mixed layer depths (MLDs) derived from an eddy-resolving Ocean General Circulation Model with a horizontal resolution of (1/10)° are validated with climatological observations. Associated heat budgets on seasonal time scales are analyzed for six boundary current regions with high eddy kinetic energy (Somali Current, Agulhas Current region, Kuroshio, East Australian Current, Gulf Stream, Brazil-Malvinas/Falkland Confluence). In all of these regions and on seasonal time scales, (a) horizontal advection significantly contributes to the mixed layer heat budget (MLHB) on eddy scales and locally exceeds ±5 °C/month; (b) lateral mixing (calculated as a residual term) is similar in size to surface net heat flux, horizontal advection and vertical entrainment in defining the mixed layer temperature; (c) seasonal vertical entrainment has a cooling effect on mixed layer temperature throughout the year in the regions investigated; and (d) a phase lag between MLD and changes in mixed layer heat content exists such that local cooling (warming) in the mixed layer precedes maxima (minima) in MLD by 1-3 months. A rather complex picture emerges where the MLHB in ocean boundary currents on larger spatial scales is determined by net surface heat fluxes and entrainment, whereas local, eddy-related advection and stirring modulate the large-scale signals.</p></div>
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Mean and seasonal mixed layer depths (MLDs) derived from an eddy-resolving Ocean General Circulation Model with a horizontal resolution of (1/10)° are validated with climatological observations. Associated heat budgets on seasonal time scales are analyzed for six boundary current regions with high eddy kinetic energy (Somali Current, Agulhas Current region, Kuroshio, East Australian Current, Gulf Stream, Brazil-Malvinas/Falkland Confluence). In all of these regions and on seasonal time scales, (a) horizontal advection significantly contributes to the mixed layer heat budget (MLHB) on eddy scales and locally exceeds ±5 °C/month; (b) lateral mixing (calculated as a residual term) is similar in size to surface net heat flux, horizontal advection and vertical entrainment in defining the mixed layer temperature; (c) seasonal vertical entrainment has a cooling effect on mixed layer temperature throughout the year in the regions investigated; and (d) a phase lag between MLD and changes in mixed layer heat content exists such that local cooling (warming) in the mixed layer precedes maxima (minima) in MLD by 1-3 months. A rather complex picture emerges where the MLHB in ocean boundary currents on larger spatial scales is determined by net surface heat fluxes and entrainment, whereas local, eddy-related advection and stirring modulate the large-scale signals.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20252" xmlns="http://purl.org/rss/1.0/"><title>Sea ice thickness retrieval algorithms based on in-situ surface elevation and thickness values for application to altimetry</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20252</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea ice thickness retrieval algorithms based on in-situ surface elevation and thickness values for application to altimetry</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Burcu Ozsoy-Cicek, Stephen Ackley, Hongjie Xie, Donghui Yi, Jay Zwally</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T02:15:38.848196-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20252</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20252</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20252</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>In situ measurements of sea ice thickness (<em>I</em>), snow depth (<em>S</em>) and snow freeboard (<em>F<sub>sn</sub></em>) from drilling profile lines from fifteen cruises into the Southern Ocean, Antarctica, were analyzed. <em>I</em> was calculated from in situ <em>F<sub>sn</sub></em> and <em>S</em> using an isostatic approach. <em>I</em> was also directly estimated from <em>F<sub>sn</sub></em> as can be obtained from laser altimetry. The Root-mean-square difference (RMSD) between observed and calculated <em>I</em> reduces, and the correlation between <em>F<sub>sn</sub></em> and <em>I</em> increases substantially, when 1) using values averaged over the survey lines (~50m) instead of single drill hole measurements (~1m), and 2) treating positive and negative sea ice freeboard (<em>F<sub>i</sub></em>) separately. For small <em>F<sub>i</sub></em>, however, <em>S</em> approximates <em>F<sub>sn</sub></em> pointing towards an isostatic balance also between <em>S</em> and <em>I</em>. Our linear regression analysis between the in situ measurements suggests a direct conversion of <em>F<sub>sn</sub></em> into <em>I</em> using a region-specific set of equations. RMSD values are similar to those obtained employing isostatic balance models and treating positive and negative <em>F<sub>i</sub></em> separately. However, more data would have been needed to obtain significant differences between most of the various models suggested. Still our new approach gives a viable alternative for Antarctic<em> I</em> retrieval from altimetric measurements of <em>F<sub>sn</sub></em> alone. Correlation between in situ observations of <em>F<sub>sn</sub></em> and <em>S</em> is high. RMSD between observed and calculated <em>S</em> is small. This suggests estimation of <em>S</em> from altimetric <em>F<sub>sn</sub></em> measurements. Such <em>S</em> has an estimated precision of ~5cm, and is neither affected by snow wetness or grain size, nor limited to <em>S</em> &lt; 50cm.</p></div>
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In situ measurements of sea ice thickness (I), snow depth (S) and snow freeboard (Fsn) from drilling profile lines from fifteen cruises into the Southern Ocean, Antarctica, were analyzed. I was calculated from in situ Fsn and S using an isostatic approach. I was also directly estimated from Fsn as can be obtained from laser altimetry. The Root-mean-square difference (RMSD) between observed and calculated I reduces, and the correlation between Fsn and I increases substantially, when 1) using values averaged over the survey lines (~50m) instead of single drill hole measurements (~1m), and 2) treating positive and negative sea ice freeboard (Fi) separately. For small Fi, however, S approximates Fsn pointing towards an isostatic balance also between S and I. Our linear regression analysis between the in situ measurements suggests a direct conversion of Fsn into I using a region-specific set of equations. RMSD values are similar to those obtained employing isostatic balance models and treating positive and negative Fi separately. However, more data would have been needed to obtain significant differences between most of the various models suggested. Still our new approach gives a viable alternative for Antarctic I retrieval from altimetric measurements of Fsn alone. Correlation between in situ observations of Fsn and S is high. RMSD between observed and calculated S is small. This suggests estimation of S from altimetric Fsn measurements. Such S has an estimated precision of ~5cm, and is neither affected by snow wetness or grain size, nor limited to S &lt; 50cm.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20253" xmlns="http://purl.org/rss/1.0/"><title>Longitudinal variability of size-fractionated N2 fixation and DON release rates along 24.5ºN in the subtropical North Atlantic</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20253</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Longitudinal variability of size-fractionated N2 fixation and DON release rates along 24.5ºN in the subtropical North Atlantic</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mar Benavides, Deborah A. Bronk, Nona S.R. Agawin, M. Dolores Pérez-Hernández, Alonso Hernández-Guerra, Javier Arístegui</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T02:04:56.969895-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20253</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20253</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20253</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Dinitrogen (N<sub>2</sub>) fixation and dissolved organic nitrogen (DON) release rates were measured on fractionated samples (&gt;10 µm and &lt;10 µm). Net N<sub>2</sub> fixation rates (N<sub>2</sub> assimilation into biomass) ranged from 0.01 to 0.4 nmol N L<sup>-1</sup> h<sup>-1</sup>, and DON release rates ranged from 0.001 to 0.09 nmol N L<sup>-1</sup> h<sup>-1</sup>. DON release represented ˜14% and ˜23% of &gt;10 µm and &lt;10 µm gross N<sub>2</sub> fixation (assimilation into biomass plus DON release), respectively. This implies that by overlooking DON release, N<sub>2</sub> fixation rates are underestimated. Net N<sub>2</sub> fixation rates were higher in the east and decreased significantly towards the west (r<sub>s</sub> = -0.487, p = 0.002, and r<sub>s</sub> = -0.496, p = 0.001, for the &gt;10 µm and &lt;10 µm fractions, respectively). The sum of both fractions correlated with aerosol optical depth at 550 nm (AOD 550 nm) (r<sub>s</sub> = 0.382, p = 0.017) and phosphate (PO<sub>4</sub><sup>3-</sup>) concentrations (r<sub>s</sub> = 0.453, p = 0.018), suggesting an enhancement of diazotrophy as a response to aerosol inputs and phosphorus availability. In contrast, DON release was constant among size fractions and did not correlate with any of these variables. We also compared N<sub>2</sub> fixation rates obtained using the <sup>15</sup>N<sub>2</sub> dissolved and bubble methods. The first gave average rates 50% higher than the latter, which supports the finding that previously published N<sub>2</sub> fixation rates are likely underestimated. We suggest that by combining N<sub>2</sub> fixation and DON release measurements using dissolved <sup>15</sup>N<sub>2</sub> global N<sub>2</sub> fixation rates could increase enough to balance oceanic fixed nitrogen budget disequilibria.</p></div>
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Dinitrogen (N2) fixation and dissolved organic nitrogen (DON) release rates were measured on fractionated samples (&gt;10 µm and &lt;10 µm). Net N2 fixation rates (N2 assimilation into biomass) ranged from 0.01 to 0.4 nmol N L-1 h-1, and DON release rates ranged from 0.001 to 0.09 nmol N L-1 h-1. DON release represented ˜14% and ˜23% of &gt;10 µm and &lt;10 µm gross N2 fixation (assimilation into biomass plus DON release), respectively. This implies that by overlooking DON release, N2 fixation rates are underestimated. Net N2 fixation rates were higher in the east and decreased significantly towards the west (rs = -0.487, p = 0.002, and rs = -0.496, p = 0.001, for the &gt;10 µm and &lt;10 µm fractions, respectively). The sum of both fractions correlated with aerosol optical depth at 550 nm (AOD 550 nm) (rs = 0.382, p = 0.017) and phosphate (PO43-) concentrations (rs = 0.453, p = 0.018), suggesting an enhancement of diazotrophy as a response to aerosol inputs and phosphorus availability. In contrast, DON release was constant among size fractions and did not correlate with any of these variables. We also compared N2 fixation rates obtained using the 15N2 dissolved and bubble methods. The first gave average rates 50% higher than the latter, which supports the finding that previously published N2 fixation rates are likely underestimated. We suggest that by combining N2 fixation and DON release measurements using dissolved 15N2 global N2 fixation rates could increase enough to balance oceanic fixed nitrogen budget disequilibria.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20251" xmlns="http://purl.org/rss/1.0/"><title>Enhancing the comprehension of mixed layer depth control on the mediterranean phytoplankton phenology</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20251</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Enhancing the comprehension of mixed layer depth control on the mediterranean phytoplankton phenology</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Héloïse Lavigne, Fabrizio D'Ortenzio, Christophe Migon, Hervé Claustre, Pierre Testor, Maurizio Ribera d'Alcalà, Rosario Lavezza, Loïc Houpert, Louis Prieur</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T01:50:41.595027-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20251</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20251</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20251</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Phytoplankton phenology is primarily affected by physical forcing. However, its quantification is far from being completely understood. Among the physical forcing factors, the Mixed Layer Depth (MLD) is considered to have the strongest impact on phytoplankton dynamics, and consequently, on their phenology. The role of MLD variations in shaping the phytoplankton phenology was explored in the Mediterranean Sea, a basin displaying contrasting phenological regimes. A database of MLD estimations was merged with ocean color chlorophyll concentrations ([Chl]<sub>SAT</sub>) to generate concomitant annual MLD and [Chl]<sub>SAT</sub> cycles. Several indices were calculated to quantitatively analyze these cycles. The relevance of indices summarizing the temporal difference between main characteristics of MLD and [Chl]<sub>SAT</sub> cycles was emphasized. As previously observed, two dominant phenological regimes co-exist in the Mediterranean Sea. The first is marked by a typical spring bloom, as in temperate regions. The second displays a low seasonality and an absence of an intense [Chl]<sub>SAT</sub> peak as in subtropical areas. The MLD is shown to play a key role in determining the dominant phenological regime in a given area. Results also show that regions having low seasonality display concomitant MLD and [Chl]<sub>SAT</sub> maxima, whereas [Chl]<sub>SAT</sub> peaks are generally observed 30 days after MLD peaks in regions with strongest seasonality. Over the whole basin, [Chl]<sub>SAT</sub> increase starts one month after the initiation of MLD deepening. Finally, after examining the impact of MLD on light and nutrient availability for phytoplankton, mechanisms were proposed to explain the time-lags between MLD and [Chl]<sub>SAT</sub> increase and MLD and [Chl]<sub>SAT</sub> maxima.</p></div>
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Phytoplankton phenology is primarily affected by physical forcing. However, its quantification is far from being completely understood. Among the physical forcing factors, the Mixed Layer Depth (MLD) is considered to have the strongest impact on phytoplankton dynamics, and consequently, on their phenology. The role of MLD variations in shaping the phytoplankton phenology was explored in the Mediterranean Sea, a basin displaying contrasting phenological regimes. A database of MLD estimations was merged with ocean color chlorophyll concentrations ([Chl]SAT) to generate concomitant annual MLD and [Chl]SAT cycles. Several indices were calculated to quantitatively analyze these cycles. The relevance of indices summarizing the temporal difference between main characteristics of MLD and [Chl]SAT cycles was emphasized. As previously observed, two dominant phenological regimes co-exist in the Mediterranean Sea. The first is marked by a typical spring bloom, as in temperate regions. The second displays a low seasonality and an absence of an intense [Chl]SAT peak as in subtropical areas. The MLD is shown to play a key role in determining the dominant phenological regime in a given area. Results also show that regions having low seasonality display concomitant MLD and [Chl]SAT maxima, whereas [Chl]SAT peaks are generally observed 30 days after MLD peaks in regions with strongest seasonality. Over the whole basin, [Chl]SAT increase starts one month after the initiation of MLD deepening. Finally, after examining the impact of MLD on light and nutrient availability for phytoplankton, mechanisms were proposed to explain the time-lags between MLD and [Chl]SAT increase and MLD and [Chl]SAT maxima.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20246" xmlns="http://purl.org/rss/1.0/"><title>How much net surface heat flux should go into the Western Pacific Warm Pool?</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20246</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">How much net surface heat flux should go into the Western Pacific Warm Pool?</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Xiangzhou Song, Lisan Yu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-29T02:11:03.068063-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20246</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20246</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20246</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The western tropical Pacific warm pool, with the surface area bounded by the 28°C isotherm, receives heat from the atmosphere through the year. However, the exact amount of net surface heat flux into this area remains to be determined. A survey of nine heat flux climatologies (including three latest atmospheric reanalyses, three early reanalyses, and three analyzed products) shows that the estimates are clustered into two groups, with a mean of 18 Wm<sup>-2</sup> for the five-member low net heat flux group (ERA-Interim, CORE.2, NCEP 1 and 2 and ERA-40) and of 49 Wm<sup>-2</sup> for the four-member high net heat flux group (CFSR, OAFlux+ISCCP, NOCSv2.0 and MERRA). This study used a pool-area based heat budget analysis together with in situ air-sea and subsurface measurements to examine the physical consistency of the nine flux climatologies and to ascribe the statistical uncertainty of each product.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The heat budget analysis indicates that the annual mean net surface heat flux should be 28±10 Wm<sup>-2</sup>. The observed eddy coefficient along the 28°C isotherm is 1.5 cm<sup>2</sup>s<sup>-1</sup> based on the TAO/TRION buoys and the historical records. The ocean cannot dissipate the excessive high heat fluxes, while the low fluxes cannot balance the estimated diffusive heat flux across the isotherm. Both the one-point direct comparison and pool integrated eddy diffusive heat flux analysis demonstrate that, the high net heat flux climatologies have high bias; on the other hand, the low fluxes have low bias. These biases and uncertainties are given and documented in this paper.</p></div>
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The western tropical Pacific warm pool, with the surface area bounded by the 28°C isotherm, receives heat from the atmosphere through the year. However, the exact amount of net surface heat flux into this area remains to be determined. A survey of nine heat flux climatologies (including three latest atmospheric reanalyses, three early reanalyses, and three analyzed products) shows that the estimates are clustered into two groups, with a mean of 18 Wm-2 for the five-member low net heat flux group (ERA-Interim, CORE.2, NCEP 1 and 2 and ERA-40) and of 49 Wm-2 for the four-member high net heat flux group (CFSR, OAFlux+ISCCP, NOCSv2.0 and MERRA). This study used a pool-area based heat budget analysis together with in situ air-sea and subsurface measurements to examine the physical consistency of the nine flux climatologies and to ascribe the statistical uncertainty of each product.
The heat budget analysis indicates that the annual mean net surface heat flux should be 28±10 Wm-2. The observed eddy coefficient along the 28°C isotherm is 1.5 cm2s-1 based on the TAO/TRION buoys and the historical records. The ocean cannot dissipate the excessive high heat fluxes, while the low fluxes cannot balance the estimated diffusive heat flux across the isotherm. Both the one-point direct comparison and pool integrated eddy diffusive heat flux analysis demonstrate that, the high net heat flux climatologies have high bias; on the other hand, the low fluxes have low bias. These biases and uncertainties are given and documented in this paper.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20248" xmlns="http://purl.org/rss/1.0/"><title>Implications from the comparisons between two- and three-dimensional model simulations of the Hurricane Ike storm surge</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20248</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Implications from the comparisons between two- and three-dimensional model simulations of the Hurricane Ike storm surge</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Lianyuan Zheng, Robert H. Weisberg, Yong Huang, Rick A. Luettich, Joannes J. Westerink, Patrick Corbitt Kerr, Aaron Donahue, Gary Crane, Linda Akli</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-29T02:10:37.613351-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20248</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20248</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20248</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>We apply the Finite Volume Coastal Ocean Model to simulate the Hurricane Ike storm surge using two-dimensional (2D) and three-dimensional (3D) formulations. The high resolution, unstructured grid extends over the Gulf of Mexico with open boundaries in the Straits of Florida and the Yucatan Channel. With the same wind and pressure forcing, the bottom drag coefficients for the baseline 2D and 3D simulations are determined by spatially varying Manning coefficients and constant bottom roughness, respectively. The baseline 2D model simulates both the forerunner and the surge, whereas the baseline 3D model simulates the surge, but underestimates the forerunner. Increasing the minimum Manning coefficient reduces the 2D forerunner and the surge. Manning coefficient and bottom roughness parameterizations produce different bottom drag coefficients. Using the same bottom drag coefficient, the 2D simulation yields a smaller surge than in 3D. This is investigated for scenarios of either constant or variable bottom roughness where the bottom roughness is determined through Manning coefficient transformation. These sensitivity studies indicate that storm surges, simulated either in 2D or 3D, depend critically upon the parameterizations and the parameter values used for specifying bottom stress (and similar may be said of surface stress). Given suitable calibration, 2D and 3D models may adequately simulate storm surge. However, it is unclear that a calibration for a given storm and location may apply generally. Hence additional experimental guidance is required on the parameterizations and the parameter values used for both the surface and bottom stresses under severe wind conditions.</p></div>
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We apply the Finite Volume Coastal Ocean Model to simulate the Hurricane Ike storm surge using two-dimensional (2D) and three-dimensional (3D) formulations. The high resolution, unstructured grid extends over the Gulf of Mexico with open boundaries in the Straits of Florida and the Yucatan Channel. With the same wind and pressure forcing, the bottom drag coefficients for the baseline 2D and 3D simulations are determined by spatially varying Manning coefficients and constant bottom roughness, respectively. The baseline 2D model simulates both the forerunner and the surge, whereas the baseline 3D model simulates the surge, but underestimates the forerunner. Increasing the minimum Manning coefficient reduces the 2D forerunner and the surge. Manning coefficient and bottom roughness parameterizations produce different bottom drag coefficients. Using the same bottom drag coefficient, the 2D simulation yields a smaller surge than in 3D. This is investigated for scenarios of either constant or variable bottom roughness where the bottom roughness is determined through Manning coefficient transformation. These sensitivity studies indicate that storm surges, simulated either in 2D or 3D, depend critically upon the parameterizations and the parameter values used for specifying bottom stress (and similar may be said of surface stress). Given suitable calibration, 2D and 3D models may adequately simulate storm surge. However, it is unclear that a calibration for a given storm and location may apply generally. Hence additional experimental guidance is required on the parameterizations and the parameter values used for both the surface and bottom stresses under severe wind conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20239" xmlns="http://purl.org/rss/1.0/"><title>State estimates and forecasts of the loop current in the Gulf of Mexico using the MITgcm and its adjoint</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20239</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">State estimates and forecasts of the loop current in the Gulf of Mexico using the MITgcm and its adjoint</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ganesh Gopalakrishnan, Bruce D. Cornuelle, Ibrahim Hoteit, Daniel L. Rudnick, W. Brechner Owens</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-23T03:10:50.756332-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20239</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20239</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20239</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>An ocean state estimate has been developed for the Gulf of Mexico (GoM) using the MIT general circulation model (MITgcm) and its adjoint. The estimate has been tested by forecasting Loop Current (LC) evolution and eddy shedding in the GoM. The adjoint (or four-dimensional variational (4D-VAR)) method was used to match the model evolution to observations by adjusting model temperature and salinity initial conditions, open boundary conditions, and atmospheric forcing fields. The model was fit to satellite-derived along-track sea surface height (SSH), separated into temporal mean and anomalies, and gridded sea surface temperature (SST) for two month periods. The optimized state at the end of the assimilation period was used to initialize the forecast for two months. Forecasts explore practical LC predictability and provide a cross-validation test of the state estimate by comparing it to independent future observations. The model forecast was tested for several Loop Current Eddy (LCE) separation events, including Eddy Franklin (Eddy-F) in May 2010 during the Deepwater Horizon (DwH) oil spill disaster in the GoM. The forecast used monthly climatological open boundary conditions, atmospheric forcing, and run-off fluxes. The model performance was evaluated by computing model-observation root-mean-square-difference (<em>rmsd</em>) during both the hindcast and forecast periods. The <em>rmsd</em> metrics for the forecast generally outperformed persistence (keeping the initial state fixed) and reference (forecast initialized using assimilated HYCOM 1/12° global analysis) model simulations during LCE separation events for a period of 1 ~ 2 months.</p></div>
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An ocean state estimate has been developed for the Gulf of Mexico (GoM) using the MIT general circulation model (MITgcm) and its adjoint. The estimate has been tested by forecasting Loop Current (LC) evolution and eddy shedding in the GoM. The adjoint (or four-dimensional variational (4D-VAR)) method was used to match the model evolution to observations by adjusting model temperature and salinity initial conditions, open boundary conditions, and atmospheric forcing fields. The model was fit to satellite-derived along-track sea surface height (SSH), separated into temporal mean and anomalies, and gridded sea surface temperature (SST) for two month periods. The optimized state at the end of the assimilation period was used to initialize the forecast for two months. Forecasts explore practical LC predictability and provide a cross-validation test of the state estimate by comparing it to independent future observations. The model forecast was tested for several Loop Current Eddy (LCE) separation events, including Eddy Franklin (Eddy-F) in May 2010 during the Deepwater Horizon (DwH) oil spill disaster in the GoM. The forecast used monthly climatological open boundary conditions, atmospheric forcing, and run-off fluxes. The model performance was evaluated by computing model-observation root-mean-square-difference (rmsd) during both the hindcast and forecast periods. The rmsd metrics for the forecast generally outperformed persistence (keeping the initial state fixed) and reference (forecast initialized using assimilated HYCOM 1/12° global analysis) model simulations during LCE separation events for a period of 1 ~ 2 months.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20245" xmlns="http://purl.org/rss/1.0/"><title>Observed intraseasonal thermocline variability in the Bay of Bengal</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20245</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Observed intraseasonal thermocline variability in the Bay of Bengal</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. S Girishkumar, M. Ravichandran, W. Han</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T08:27:54.954356-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20245</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20245</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20245</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The time series of temperature data obtained from moored buoys deployed at 8°N, 12°N and 15°N along 90°E in the Bay of Bengal (BoB) shows a persistent intraseasonal variability on 30-120 day time scale in three distinct periods 30-70 day, near 90-day and near 120-day in the thermocline region. The standard deviation of moored buoy temperature data shows that half of the variability in the thermocline region is contributed from the 30-120 day variability. The relative contribution of local Ekman pumping velocity and remote wind forcing from equatorial Indian Ocean (EIO) to the intraseasonal thermocline variability in the BoB is examined using satellite derived Sea surface height anomaly (SSHA), wind and depths of 23° isotherm (D23, proxy for thermocline depth) derived from moored buoys temperature data. The analysis shows that large amplitude intraseasonal oscillations of thermocline - particularly the near 90-day and 120-day variability - could not be explained by local Ekman pumping velocity alone. The SSHA, D23 and wind fields reveal that the first and second baroclinic mode Kelvin and Rossby waves, which are generated remotely by winds from the EIO and eastern BoB, can significantly influence the thermocline variability in the BoB. The near 90-day and 120-day thermocline variability is driven primarily by the variability of equatorial zonal wind stress. While the 30-70 day thermocline variability is affected most by interior Ekman pumping over the Bay, it also appears to be influenced by zonal wind stress in the EIO and alongshore wind stress in the eastern BoB.</p></div>
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The time series of temperature data obtained from moored buoys deployed at 8°N, 12°N and 15°N along 90°E in the Bay of Bengal (BoB) shows a persistent intraseasonal variability on 30-120 day time scale in three distinct periods 30-70 day, near 90-day and near 120-day in the thermocline region. The standard deviation of moored buoy temperature data shows that half of the variability in the thermocline region is contributed from the 30-120 day variability. The relative contribution of local Ekman pumping velocity and remote wind forcing from equatorial Indian Ocean (EIO) to the intraseasonal thermocline variability in the BoB is examined using satellite derived Sea surface height anomaly (SSHA), wind and depths of 23° isotherm (D23, proxy for thermocline depth) derived from moored buoys temperature data. The analysis shows that large amplitude intraseasonal oscillations of thermocline - particularly the near 90-day and 120-day variability - could not be explained by local Ekman pumping velocity alone. The SSHA, D23 and wind fields reveal that the first and second baroclinic mode Kelvin and Rossby waves, which are generated remotely by winds from the EIO and eastern BoB, can significantly influence the thermocline variability in the BoB. The near 90-day and 120-day thermocline variability is driven primarily by the variability of equatorial zonal wind stress. While the 30-70 day thermocline variability is affected most by interior Ekman pumping over the Bay, it also appears to be influenced by zonal wind stress in the EIO and alongshore wind stress in the eastern BoB.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20243" xmlns="http://purl.org/rss/1.0/"><title>Integrating satellite observations and modern climate measurements with the recent sedimentary record: An example from Southeast Alaska</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20243</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Integrating satellite observations and modern climate measurements with the recent sedimentary record: An example from Southeast Alaska</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jason A. Addison, Bruce P. Finney, John M. Jaeger, Joseph S. Stoner, Richard D. Norris, Alexandra Hangsterfer</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T08:21:50.273811-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20243</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20243</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20243</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Assessments of climate change over time scales that exceed the last 100 years require robust integration of high-quality instrument records with high-resolution paleoclimate proxy data. In this study, we show that the recent biogenic sediments accumulating in two temperate ice-free fjords in Southeast Alaska preserve evidence of North Pacific Ocean climate variability as recorded by both instrument networks and satellite observations. Multicore samples EW0408-32MC and -43MC were investigated with <sup>137</sup>Cs and excess <sup>210</sup>Pb geochronometry, 3D computerized tomography, high-resolution scanning XRF geochemistry, and organic stable isotope analyses. EW0408-32MC (57.162°N, 135.357°W, 146 m depth) is a moderately-bioturbated continuous record that spans AD ~1930 - 2004. EW0408-43MC (56.965°N, 135.268°W, 91 m depth) is composed of laminated diatom oozes, a turbidite, and a hypopycnal plume (river flood) deposit. A discontinuous event-based varve chronology indicates 43MC spans AD ~1940 - 1981. Decadal-scale fluctuations in sedimentary Br/Cl ratios accurately reflect changes in marine organic matter accumulation that display the same temporal pattern as that of the Pacific Decadal Oscillation. An estimated Sitka summer productivity parameter calibrated using SeaWiFS satellite observations support these relationships. The correlation of North Pacific climate regime states, primary productivity, and sediment geochemistry indicate the accumulation of biogenic sediment in Southeast Alaska temperate fjords can be used as a sensitive recorder of past productivity variability, and by inference, past climate conditions in the high-latitude Gulf of Alaska.</p></div>
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Assessments of climate change over time scales that exceed the last 100 years require robust integration of high-quality instrument records with high-resolution paleoclimate proxy data. In this study, we show that the recent biogenic sediments accumulating in two temperate ice-free fjords in Southeast Alaska preserve evidence of North Pacific Ocean climate variability as recorded by both instrument networks and satellite observations. Multicore samples EW0408-32MC and -43MC were investigated with 137Cs and excess 210Pb geochronometry, 3D computerized tomography, high-resolution scanning XRF geochemistry, and organic stable isotope analyses. EW0408-32MC (57.162°N, 135.357°W, 146 m depth) is a moderately-bioturbated continuous record that spans AD ~1930 - 2004. EW0408-43MC (56.965°N, 135.268°W, 91 m depth) is composed of laminated diatom oozes, a turbidite, and a hypopycnal plume (river flood) deposit. A discontinuous event-based varve chronology indicates 43MC spans AD ~1940 - 1981. Decadal-scale fluctuations in sedimentary Br/Cl ratios accurately reflect changes in marine organic matter accumulation that display the same temporal pattern as that of the Pacific Decadal Oscillation. An estimated Sitka summer productivity parameter calibrated using SeaWiFS satellite observations support these relationships. The correlation of North Pacific climate regime states, primary productivity, and sediment geochemistry indicate the accumulation of biogenic sediment in Southeast Alaska temperate fjords can be used as a sensitive recorder of past productivity variability, and by inference, past climate conditions in the high-latitude Gulf of Alaska.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20242" xmlns="http://purl.org/rss/1.0/"><title>On the factors influencing the development of sporadic upwelling in the Leeuwin Current system</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20242</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">On the factors influencing the development of sporadic upwelling in the Leeuwin Current system</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Vincent Rossi, Ming Feng, Charitha Pattiaratchi, Moninya Roughan, Anya M. Waite</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T08:16:55.678218-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20242</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20242</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20242</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>While there is no persistent upwelling along the West-Australian (WA) coastline, sporadic upwelling events have been documented primarily in summer. By analysing comparatively the variability of both Ekman and geostrophic cross-shore transports over a seasonal cycle, we show that the situation is more contrasted. Based on a composite index computed from satellite data over a 15 year period, calibrated with well documented events, we investigate the factors influencing the development of sporadic upwelling in the region. Overall, the occurrence of transient upwelling events lasting 3 to 10 days varies largely in space and time. Shelf regions at 31.5 and 34°S are favoured with up to 12 upwelling days per month during the austral spring/summer. Although being generally favoured from September to April, sporadic upwelling events can also occur at any time of the year at certain locations north of 30°S. On average over 1995-2010, the Ningaloo region (22.5°S) cumulates the highest number of upwelling (~140 days per year) and is characterized by longer events. The intensity of intermittent upwelling is influenced by the upwelling-favourable winds, the characteristics of the Leeuwin Current (e.g. onshore geostrophic flow, mesoscale eddies and meanders, stratification and nitracline) and the local topography. This suggests that short-living nutrient enrichment of variable magnitude may occur at any time of the year at many locations along the WA coast.</p></div>
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While there is no persistent upwelling along the West-Australian (WA) coastline, sporadic upwelling events have been documented primarily in summer. By analysing comparatively the variability of both Ekman and geostrophic cross-shore transports over a seasonal cycle, we show that the situation is more contrasted. Based on a composite index computed from satellite data over a 15 year period, calibrated with well documented events, we investigate the factors influencing the development of sporadic upwelling in the region. Overall, the occurrence of transient upwelling events lasting 3 to 10 days varies largely in space and time. Shelf regions at 31.5 and 34°S are favoured with up to 12 upwelling days per month during the austral spring/summer. Although being generally favoured from September to April, sporadic upwelling events can also occur at any time of the year at certain locations north of 30°S. On average over 1995-2010, the Ningaloo region (22.5°S) cumulates the highest number of upwelling (~140 days per year) and is characterized by longer events. The intensity of intermittent upwelling is influenced by the upwelling-favourable winds, the characteristics of the Leeuwin Current (e.g. onshore geostrophic flow, mesoscale eddies and meanders, stratification and nitracline) and the local topography. This suggests that short-living nutrient enrichment of variable magnitude may occur at any time of the year at many locations along the WA coast.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20244" xmlns="http://purl.org/rss/1.0/"><title>Co-limitation by light, nitrate and iron in the Beaufort sea in late summer</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20244</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Co-limitation by light, nitrate and iron in the Beaufort sea in late summer</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rebecca L. Taylor, David M. Semeniuk, Christopher D. Payne, Jie Zhou, Jean-Éric Tremblay, Jay T. Cullen, Maria T. Maldonado</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T08:06:58.534042-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20244</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20244</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20244</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>As part of the GEOTRACES International Polar Year program, in September 2009 we performed a grow-out experiment to investigate the potential for nitrate, light, and iron (Fe) limitation of Beaufort Sea phytoplankton. Nutrients, phytoplankton biomass/composition, and Fe and C uptake rates were measured regularly. Nitrate additions enhanced phytoplankton growth, demonstrating that the late summer phytoplankton community was N limited. In the treatments with additions of nitrate but not Fe, total chlorophyll <em>a</em> doubled with each increase in light level, indicating the community was also light limited. In nitrate enriched treatments, co-limitation of primary production by Fe and light was observed at light levels ≤ 10 % surface irradiance (I<sub>o</sub>), which corresponded to depths ≥ 33 m. The higher Fe demand associated with low irradiance was supported by 10 to 100-fold higher Fe:C assimilation ratios. Furthermore, the Fe:C assimilation ratios of phytoplankton with an Fe addition (1 nmol L<sup>-1</sup>) were ~ 2-fold higher than those with no Fe added at 1 %I<sub>o</sub>, indicating severe Fe deficiency at <em>in situ</em> Fe (0.154 nmol L<sup>-1</sup>) and low light. The average light intensity experienced by phytoplankton in the 1 %I<sub>o</sub> treatments corresponded to the light intensity at ~ 73 m, which is well below the 44 m euphotic depth at this station in late summer, but coincides with the depth where the subsurface chlorophyll maximum is often found in this region (~70 m). These results suggest that, in addition to nitrate and light, Fe availability may control primary productivity in the Beaufort Sea, and seasonal changes in light, nitrate, and Fe availability may differentially control Arctic phytoplankton growth.</p></div>
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As part of the GEOTRACES International Polar Year program, in September 2009 we performed a grow-out experiment to investigate the potential for nitrate, light, and iron (Fe) limitation of Beaufort Sea phytoplankton. Nutrients, phytoplankton biomass/composition, and Fe and C uptake rates were measured regularly. Nitrate additions enhanced phytoplankton growth, demonstrating that the late summer phytoplankton community was N limited. In the treatments with additions of nitrate but not Fe, total chlorophyll a doubled with each increase in light level, indicating the community was also light limited. In nitrate enriched treatments, co-limitation of primary production by Fe and light was observed at light levels ≤ 10 % surface irradiance (Io), which corresponded to depths ≥ 33 m. The higher Fe demand associated with low irradiance was supported by 10 to 100-fold higher Fe:C assimilation ratios. Furthermore, the Fe:C assimilation ratios of phytoplankton with an Fe addition (1 nmol L-1) were ~ 2-fold higher than those with no Fe added at 1 %Io, indicating severe Fe deficiency at in situ Fe (0.154 nmol L-1) and low light. The average light intensity experienced by phytoplankton in the 1 %Io treatments corresponded to the light intensity at ~ 73 m, which is well below the 44 m euphotic depth at this station in late summer, but coincides with the depth where the subsurface chlorophyll maximum is often found in this region (~70 m). These results suggest that, in addition to nitrate and light, Fe availability may control primary productivity in the Beaufort Sea, and seasonal changes in light, nitrate, and Fe availability may differentially control Arctic phytoplankton growth.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20240" xmlns="http://purl.org/rss/1.0/"><title>Adjoint sensitivity studies of loop current and Eddy Shedding in the Gulf of Mexico</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20240</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Adjoint sensitivity studies of loop current and Eddy Shedding in the Gulf of Mexico</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ganesh Gopalakrishnan, Bruce D. Cornuelle, Ibrahim Hoteit</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T08:01:35.526989-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20240</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20240</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20240</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Adjoint model sensitivity analyses were applied for the Loop Current (LC) and its eddy shedding in the Gulf of Mexico (GoM) using the MIT general circulation model (MITgcm). The circulation in the GoM is mainly driven by the energetic LC and subsequent LC eddy separation. In order to understand which ocean regions and features control the evolution of the LC, including anti-cyclonic warm-core eddy shedding in the GoM, forward and adjoint sensitivities with respect to previous model state and atmospheric forcing were computed using the MITgcm and its adjoint. Since the validity of the adjoint model sensitivities depends on the capability of the forward model to simulate the real LC system and the eddy shedding processes, a five year (2004-2008) forward model simulation was performed for the GoM using realistic atmospheric forcing, initial, and boundary conditions. This forward model simulation was compared to satellite measurements of sea-surface height (SSH) and sea-surface temperature (SST), and observed transport variability. Despite realistic mean state, standard deviations, and LC eddy shedding period, the simulated LC extension shows less variability and more regularity than the observations. However, the model is suitable for studying the LC system and can be utilized for examining the ocean influences leading to a simple, and hopefully generic LC eddy separation in the GoM. The adjoint sensitivities of the LC show influences from the Yucatan Channel (YC) flow and Loop Current Frontal Eddy (LCFE) on both LC extension and eddy separation, as suggested by earlier work. Some of the processes that control LC extension after eddy separation differ from those controlling eddy shedding, but include YC through-flow. The sensitivity remains stable for more than 30 days and moves generally upstream, entering the Caribbean Sea. The sensitivities of the LC for SST generally remain closer to the surface and move at speeds consistent with advection by the high-speed core of the current, while sensitivities to SSH generally extend to deeper layers and propagate more slowly. The adjoint sensitivity to relative vorticity deduced from the sensitivities to velocity fields suggests that advection of cyclonic (positive) relative vorticity anomalies from the YC or the LCFEs accelerate the LC eddy separation. Forward model perturbation experiments were performed to complement and check the adjoint sensitivity analysis as well as sampling the predictability and non-linearity of the LC evolution. The model and its adjoint can be used in four-dimensional variational assimilation (4D-VAR) to produce dynamically consistent ocean state estimates for analysis and forecasts of the circulation of the GoM [<em>gopalakrishnan et al</em>., 2012-2]</p></div>
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Adjoint model sensitivity analyses were applied for the Loop Current (LC) and its eddy shedding in the Gulf of Mexico (GoM) using the MIT general circulation model (MITgcm). The circulation in the GoM is mainly driven by the energetic LC and subsequent LC eddy separation. In order to understand which ocean regions and features control the evolution of the LC, including anti-cyclonic warm-core eddy shedding in the GoM, forward and adjoint sensitivities with respect to previous model state and atmospheric forcing were computed using the MITgcm and its adjoint. Since the validity of the adjoint model sensitivities depends on the capability of the forward model to simulate the real LC system and the eddy shedding processes, a five year (2004-2008) forward model simulation was performed for the GoM using realistic atmospheric forcing, initial, and boundary conditions. This forward model simulation was compared to satellite measurements of sea-surface height (SSH) and sea-surface temperature (SST), and observed transport variability. Despite realistic mean state, standard deviations, and LC eddy shedding period, the simulated LC extension shows less variability and more regularity than the observations. However, the model is suitable for studying the LC system and can be utilized for examining the ocean influences leading to a simple, and hopefully generic LC eddy separation in the GoM. The adjoint sensitivities of the LC show influences from the Yucatan Channel (YC) flow and Loop Current Frontal Eddy (LCFE) on both LC extension and eddy separation, as suggested by earlier work. Some of the processes that control LC extension after eddy separation differ from those controlling eddy shedding, but include YC through-flow. The sensitivity remains stable for more than 30 days and moves generally upstream, entering the Caribbean Sea. The sensitivities of the LC for SST generally remain closer to the surface and move at speeds consistent with advection by the high-speed core of the current, while sensitivities to SSH generally extend to deeper layers and propagate more slowly. The adjoint sensitivity to relative vorticity deduced from the sensitivities to velocity fields suggests that advection of cyclonic (positive) relative vorticity anomalies from the YC or the LCFEs accelerate the LC eddy separation. Forward model perturbation experiments were performed to complement and check the adjoint sensitivity analysis as well as sampling the predictability and non-linearity of the LC evolution. The model and its adjoint can be used in four-dimensional variational assimilation (4D-VAR) to produce dynamically consistent ocean state estimates for analysis and forecasts of the circulation of the GoM [gopalakrishnan et al., 2012-2]
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20241" xmlns="http://purl.org/rss/1.0/"><title>Predicting wave-induced ripple equilibrium geometry</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20241</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Predicting wave-induced ripple equilibrium geometry</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Timothy Robert Nelson, George Voulgaris, Peter Traykovski</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T07:53:05.844415-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20241</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20241</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20241</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>A comprehensive database of existing (since 1954) field and laboratory measurements of ripple geometry is compiled and combined with newly collected field data to examine the performance of ripple equilibrium predictors. Re-analysis of this enlarged ripple geometry data set reveals that ripples formed from monochromatic waves scale differently than ripples formed from random waves for many existing ripple predictors. Our analysis indicates that ripple wavelengths from the two data sets collapse into a single scaling when the semi-orbital excursion and sediment grain diameter are used as normalizing factors. Ripple steepness remains relatively constant for both regular and irregular wave conditions and it only slightly increases for shorter ripple wavelengths. These findings allowed for the development of a new equilibrium ripple predictor suitable for application in a wide range of wave and sediment conditions.</p></div>
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A comprehensive database of existing (since 1954) field and laboratory measurements of ripple geometry is compiled and combined with newly collected field data to examine the performance of ripple equilibrium predictors. Re-analysis of this enlarged ripple geometry data set reveals that ripples formed from monochromatic waves scale differently than ripples formed from random waves for many existing ripple predictors. Our analysis indicates that ripple wavelengths from the two data sets collapse into a single scaling when the semi-orbital excursion and sediment grain diameter are used as normalizing factors. Ripple steepness remains relatively constant for both regular and irregular wave conditions and it only slightly increases for shorter ripple wavelengths. These findings allowed for the development of a new equilibrium ripple predictor suitable for application in a wide range of wave and sediment conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20236" xmlns="http://purl.org/rss/1.0/"><title>Tidally induced increases in melting of Amundsen Sea Ice Shelves</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20236</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Tidally induced increases in melting of Amundsen Sea Ice Shelves</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Robin Robertson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-17T11:17:41.180881-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20236</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20236</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20236</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Tidal effects on the circulation under the ice shelves and ice shelf melting in the Amundsen Sea were investigated using a numerical model, through comparison of simulations with and without tides. In the Amundsen Sea, tidal impacts were dependant on the location of the ice shelf front with respect to the M<sub>2</sub> effective critical latitude. The critical latitude is the latitude where the tidal frequency equals the inertial frequency. The effective critical latitude is where the tidal frequency equals the inertial frequency adjusted by relative vorticity, such as that associated with a wind-driven gyre. For ice shelves located equatorward of the M<sub>2</sub> effective critical latitude, tides increased both mixing in front of and under the ice shelf and flow into the ice shelf cavities by as much as 50%, despite weak tides compared with the mean flows. Tides also increased melting for these ice shelves by 1-3.5 m yr<sup>-1</sup>, a 50% increase for Dotson Ice Shelf and 25% for Pine Island Ice Shelf. These enhancements were not a result of tidal residual flows, but instead originated from resonant effects, increases in the baroclinity of the velocities, and higher mixing, all of which are associated with critical latitude effects on internal tides. For ice shelves located poleward of the effective critical latitude, tides very slightly retarded flow into the cavity and slightly reduced melting.</p></div>
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Tidal effects on the circulation under the ice shelves and ice shelf melting in the Amundsen Sea were investigated using a numerical model, through comparison of simulations with and without tides. In the Amundsen Sea, tidal impacts were dependant on the location of the ice shelf front with respect to the M2 effective critical latitude. The critical latitude is the latitude where the tidal frequency equals the inertial frequency. The effective critical latitude is where the tidal frequency equals the inertial frequency adjusted by relative vorticity, such as that associated with a wind-driven gyre. For ice shelves located equatorward of the M2 effective critical latitude, tides increased both mixing in front of and under the ice shelf and flow into the ice shelf cavities by as much as 50%, despite weak tides compared with the mean flows. Tides also increased melting for these ice shelves by 1-3.5 m yr-1, a 50% increase for Dotson Ice Shelf and 25% for Pine Island Ice Shelf. These enhancements were not a result of tidal residual flows, but instead originated from resonant effects, increases in the baroclinity of the velocities, and higher mixing, all of which are associated with critical latitude effects on internal tides. For ice shelves located poleward of the effective critical latitude, tides very slightly retarded flow into the cavity and slightly reduced melting.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20235" xmlns="http://purl.org/rss/1.0/"><title>Observations of near-inertial surface currents off Oregon: Decorrelation time and length scales</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20235</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Observations of near-inertial surface currents off Oregon: Decorrelation time and length scales</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sung Yong Kim, P. Michael Kosro</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-17T11:02:35.212662-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20235</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20235</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20235</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>High-resolution (km in space and hourly in time) surface currents observed by an array of high-frequency radars off Oregon are analyzed to quantify the decorrelation time and length scales of their near-inertial motions. The near-inertial surface currents are dominantly clockwise with amplitudes of 9 to 12 cm s<sup>-1</sup>. However, they appear asymmetric and elliptical as a result of counter-clockwise inertial motions with magnitudes in a range of 2 to 5 cm s<sup>-1</sup>. The decorrelation time and length scales are computed from the decay slope of the near-inertial peak and the spatial coherence in the near-inertial frequency band, respectively. Decorrelation time scales of clockwise near-inertial motions increase from 2 days nearshore (within 30 km from the coast) to 6 days offshore, and their length scales increase from 30 km to 90 km seaward possibly due to coastal inhibition. The local spatial coherence has an exponentially decaying structure for both clockwise and counter-clockwise rotations, and their phases propagate northwestward (offshore) for clockwise and northeastward (onshore) for counter-clockwise rotations.</p></div>
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High-resolution (km in space and hourly in time) surface currents observed by an array of high-frequency radars off Oregon are analyzed to quantify the decorrelation time and length scales of their near-inertial motions. The near-inertial surface currents are dominantly clockwise with amplitudes of 9 to 12 cm s-1. However, they appear asymmetric and elliptical as a result of counter-clockwise inertial motions with magnitudes in a range of 2 to 5 cm s-1. The decorrelation time and length scales are computed from the decay slope of the near-inertial peak and the spatial coherence in the near-inertial frequency band, respectively. Decorrelation time scales of clockwise near-inertial motions increase from 2 days nearshore (within 30 km from the coast) to 6 days offshore, and their length scales increase from 30 km to 90 km seaward possibly due to coastal inhibition. The local spatial coherence has an exponentially decaying structure for both clockwise and counter-clockwise rotations, and their phases propagate northwestward (offshore) for clockwise and northeastward (onshore) for counter-clockwise rotations.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20232" xmlns="http://purl.org/rss/1.0/"><title>Physical and biogeochemical properties in landfast sea ice (Barrow, Alaska): Insights on brine and gas dynamics across seasons</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20232</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Physical and biogeochemical properties in landfast sea ice (Barrow, Alaska): Insights on brine and gas dynamics across seasons</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jiayun Zhou, Bruno Delille, Hajo Eicken, Martin Vancoppenolle, Frédéric Brabant, Gauthier Carnat, Nicolas-Xavier Geilfus, Tim Papakyriakou, Bernard Heinesch, Jean-Louis Tison</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-17T10:55:31.719046-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20232</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20232</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20232</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The impacts of the seasonal evolution of sea-ice physical properties on ice-ocean biogeochemical exchanges were investigated in landfast ice at Barrow (Alaska) from January through June 2009. Three stages of brine dynamics across the annual cycle have been identified based on brine salinity, brine volume fraction and porous medium Rayleigh number (Ra). These are sea-ice bottom-layer convection, full-depth convection and brine stratification. We further discuss the impact of brine dynamics on biogeochemical compounds in sea ice: stable isotopes of water (δD, δ<sup>18</sup>O), nutrients (NO<sub>3</sub><sup>-</sup>, PO<sub>4</sub><sup>3-</sup>, NH<sub>4</sub><sup>+</sup>), micro-algae (chlorophyll-a) and inert gas (argon). In general, full-depth convection events favour exchanges between sea ice and seawater, while brine stratification limits these exchanges. However, argon responds differently to brine dynamics than the other biogeochemical compounds analysed in this study. This contrast is attributed to the impact of bubble nucleation on inert gas transport compared to the other biogeochemical compounds. We present a scenario for argon bubble formation and evolution in sea ice and suggest that a brine volume fraction approaching 7.5 % to 10 % is required for inert gas bubbles to escape from sea ice to the atmosphere.</p></div>
]]></content:encoded><description>

The impacts of the seasonal evolution of sea-ice physical properties on ice-ocean biogeochemical exchanges were investigated in landfast ice at Barrow (Alaska) from January through June 2009. Three stages of brine dynamics across the annual cycle have been identified based on brine salinity, brine volume fraction and porous medium Rayleigh number (Ra). These are sea-ice bottom-layer convection, full-depth convection and brine stratification. We further discuss the impact of brine dynamics on biogeochemical compounds in sea ice: stable isotopes of water (δD, δ18O), nutrients (NO3-, PO43-, NH4+), micro-algae (chlorophyll-a) and inert gas (argon). In general, full-depth convection events favour exchanges between sea ice and seawater, while brine stratification limits these exchanges. However, argon responds differently to brine dynamics than the other biogeochemical compounds analysed in this study. This contrast is attributed to the impact of bubble nucleation on inert gas transport compared to the other biogeochemical compounds. We present a scenario for argon bubble formation and evolution in sea ice and suggest that a brine volume fraction approaching 7.5 % to 10 % is required for inert gas bubbles to escape from sea ice to the atmosphere.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20233" xmlns="http://purl.org/rss/1.0/"><title>Projected future wave climate in the NW Mediterranean Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20233</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Projected future wave climate in the NW Mediterranean Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Casas-Prat, J. P. Sierra</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-13T09:28:37.445268-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20233</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20233</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20233</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Projected future regional wave climate scenarios at a high temporal-spatial scale were obtained for the NW Mediterranean Sea, using 5 combinations of regional-global circulation models. Changes in wave variables were analyzed and related to the variations of the forcing wind projections, while also evaluating the evolution of the presence of the different types of sea states. To assess the significance of the changes produced, a bootstrap-based method was proposed which accounts for the autocorrelation of data and correctly reproduces the extremes.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>For the mean climate, relative changes of H<sub>s</sub> up to ±10% were obtained, whereas they were around ±20% for the extreme climate. In mean terms, variations of H<sub>s</sub> are similar to those associated with wind speed but are enhanced/attenuated, respectively, when fetch conditions are favorable/unfavorable. In general, most notable alterations are not in the H<sub>s</sub> magnitude but rather in its direction. In this regard, during the winter season, it is interesting to note that the signiﬁcant deviations between the results derived from the two global circulation models are larger than those between regional models. ECHAM5 simulated an enhanced W wind flow which is translated into more frequent W-NW waves, whereas the HadCM3Q3 global model gives rise to the E component, which contributes to a higher intensity and number of storms coming from such a direction and directly affects the wind-sea/swell distribution of coastal stretches that face E, like the Catalan coast. Different patterns of change were obtained during the summer, when a common rise of NE-E waves was found.</p></div>
]]></content:encoded><description>

Projected future regional wave climate scenarios at a high temporal-spatial scale were obtained for the NW Mediterranean Sea, using 5 combinations of regional-global circulation models. Changes in wave variables were analyzed and related to the variations of the forcing wind projections, while also evaluating the evolution of the presence of the different types of sea states. To assess the significance of the changes produced, a bootstrap-based method was proposed which accounts for the autocorrelation of data and correctly reproduces the extremes.
For the mean climate, relative changes of Hs up to ±10% were obtained, whereas they were around ±20% for the extreme climate. In mean terms, variations of Hs are similar to those associated with wind speed but are enhanced/attenuated, respectively, when fetch conditions are favorable/unfavorable. In general, most notable alterations are not in the Hs magnitude but rather in its direction. In this regard, during the winter season, it is interesting to note that the signiﬁcant deviations between the results derived from the two global circulation models are larger than those between regional models. ECHAM5 simulated an enhanced W wind flow which is translated into more frequent W-NW waves, whereas the HadCM3Q3 global model gives rise to the E component, which contributes to a higher intensity and number of storms coming from such a direction and directly affects the wind-sea/swell distribution of coastal stretches that face E, like the Catalan coast. Different patterns of change were obtained during the summer, when a common rise of NE-E waves was found.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20231" xmlns="http://purl.org/rss/1.0/"><title>Creation and tidal advection of a cold salinity front in Storfjorden. Part 1: Polynya dynamics</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20231</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Creation and tidal advection of a cold salinity front in Storfjorden. Part 1: Polynya dynamics</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ragnheid Skogseth, Miles G. McPhee, Frank Nilsen, Lars H. Smedsrud</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T05:30:20.138256-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20231</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20231</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20231</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Hydrographical measurements from the Storfjorden polynya document the presence of an abrupt front in near-freezing water dividing saline (dense) water recently created by a polynya event, from less saline water originating further south. This event occurred days before the survey with estimated heat flux ~400 W m<sup>-2</sup> over the polynya indicated by satellite images. Brine-enriched shelf water (BSW) is observed downslope toward deeper parts of Storfjorden, and BSW from earlier polynya events overflows the sill. Current measurements from a nearby sound, Freemansundet, document tidal currents exceeding 80 cm s<sup>-1</sup> that displaced the front back and forth beneath the measurement site on fast ice ~400 m from the polynya edge. Front displacement of ~12 km is documented and mainly due to the M<sub>2</sub> component superimposed on a mean residual current of 0.28 m s<sup>-1</sup> into the sound induced by the southerly wind during the measuring period. Complex topography imposes baroclinic tidal currents with strong vertical shear in the fast-ice covered sound, and with significant cross channel flow. Supercooling events indicated in the hydrographical time series, and most likely enhanced frazil ice production, are associated with double-diffusive turbulent mixing when the salinity front passes the measurement site. In this way, these measurements indicate a novel ice production process along the edge of tidally induced latent heat polynyas where salinity fronts are generated. Turbulence increases (decreases) during flood (ebb) due to the destabilization (stabilization) of the water column when the salinity front passes the measurement site. Double-diffusive turbulent mixing related to tidal advection of salinity front below fast ice is pursued in a companion paper: <em>McPhee et al.</em> [2013].</p></div>
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Hydrographical measurements from the Storfjorden polynya document the presence of an abrupt front in near-freezing water dividing saline (dense) water recently created by a polynya event, from less saline water originating further south. This event occurred days before the survey with estimated heat flux ~400 W m-2 over the polynya indicated by satellite images. Brine-enriched shelf water (BSW) is observed downslope toward deeper parts of Storfjorden, and BSW from earlier polynya events overflows the sill. Current measurements from a nearby sound, Freemansundet, document tidal currents exceeding 80 cm s-1 that displaced the front back and forth beneath the measurement site on fast ice ~400 m from the polynya edge. Front displacement of ~12 km is documented and mainly due to the M2 component superimposed on a mean residual current of 0.28 m s-1 into the sound induced by the southerly wind during the measuring period. Complex topography imposes baroclinic tidal currents with strong vertical shear in the fast-ice covered sound, and with significant cross channel flow. Supercooling events indicated in the hydrographical time series, and most likely enhanced frazil ice production, are associated with double-diffusive turbulent mixing when the salinity front passes the measurement site. In this way, these measurements indicate a novel ice production process along the edge of tidally induced latent heat polynyas where salinity fronts are generated. Turbulence increases (decreases) during flood (ebb) due to the destabilization (stabilization) of the water column when the salinity front passes the measurement site. Double-diffusive turbulent mixing related to tidal advection of salinity front below fast ice is pursued in a companion paper: McPhee et al. [2013].
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20230" xmlns="http://purl.org/rss/1.0/"><title>Remote impacts of the 18.6-year period modulation of localized tidal mixing in the North Pacific</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20230</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Remote impacts of the 18.6-year period modulation of localized tidal mixing in the North Pacific</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">S. Osafune, I. Yasuda</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T01:56:46.306707-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20230</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20230</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20230</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The impact of the 18.6-year period modulation of the localized strong tidal mixing on the annual mean sea surface temperature (SST) in the open North Pacific Ocean is analyzed in a numerical experiment using an ocean general circulation model. Oscillatory SST anomalies induced in this model move eastward along the boundary between the subarctic and the subtropical gyres from the western boundary to the central Pacific in about 10 years, with a speed slower than that of the surface currents. Anomalous currents in the upper 300 m play an important role in inducing the SST anomalies. These anomalous currents are coupled to subsurface density anomalies, and could be related to eastward-moving, low-mode (second or higher), baroclinic long Rossby waves. These results suggest that the 18.6-year modulation of localized strong tidal mixing can influence large-scale SST and/or heat flux, and thus climate, as a result of remote impacts associated with changes in the mid-depth density structure, induced locally where mixing is strong, that move horizontally into the open ocean.</p></div>
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The impact of the 18.6-year period modulation of the localized strong tidal mixing on the annual mean sea surface temperature (SST) in the open North Pacific Ocean is analyzed in a numerical experiment using an ocean general circulation model. Oscillatory SST anomalies induced in this model move eastward along the boundary between the subarctic and the subtropical gyres from the western boundary to the central Pacific in about 10 years, with a speed slower than that of the surface currents. Anomalous currents in the upper 300 m play an important role in inducing the SST anomalies. These anomalous currents are coupled to subsurface density anomalies, and could be related to eastward-moving, low-mode (second or higher), baroclinic long Rossby waves. These results suggest that the 18.6-year modulation of localized strong tidal mixing can influence large-scale SST and/or heat flux, and thus climate, as a result of remote impacts associated with changes in the mid-depth density structure, induced locally where mixing is strong, that move horizontally into the open ocean.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20220" xmlns="http://purl.org/rss/1.0/"><title>Evaluating the use of high-frequency radar coastal currents to correct satellite altimetry</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20220</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Evaluating the use of high-frequency radar coastal currents to correct satellite altimetry</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. J. Roesler, W. J. Emery, S.Y. Kim</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-07T21:00:34.266799-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20220</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20220</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20220</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Coastal altimeter waveforms may differ from the ones in the open ocean, either from rapid changes in the sea state or the presence of land within the satellite altimeter footprint. The optimal retracking method for an individual track may turn out to be a combination of several retrackers, and may depend on the sea state. The coastal High-Frequency Radar (HFR) ocean surface currents, hourly interpolated with a resolution up to 2 km and an offshore range up to 150 km, are evaluated to validate the altimeter Sea Surface Height (SSH) measurements. A method to derive HFR SSH mapped, with a varying spatial scale optimal interpolation, from the HFR velocities has been implemented. Evaluated, mainly, in the regions further than 25 km off the U.S. West coast, the HFR SSH shows good agreement with Jason-1-2 altimetry products over the years 2008 and 2009. Three Jason-2 PISTACH retrackers and one generic open ocean retracker have been analyzed using the traditional 1-Hz sampling rate. Near shore an experimental reprocessing of the 20-Hz range measurements is also tested to check for a gain in along-track spatial resolution. Referencing to the HFR SSH indicate the need to have several retrackers available, even over the continental shelf, with Ice3 fitting better during Bloom events and MLE-4 (or Red3) for high sea states. These studies demonstrate the value of HFR as a potential tool to correct coastal altimeter SSH, refine their spatial resolution and provide some insight into the altimeter behavior as a function of ocean conditions.</p></div>
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Coastal altimeter waveforms may differ from the ones in the open ocean, either from rapid changes in the sea state or the presence of land within the satellite altimeter footprint. The optimal retracking method for an individual track may turn out to be a combination of several retrackers, and may depend on the sea state. The coastal High-Frequency Radar (HFR) ocean surface currents, hourly interpolated with a resolution up to 2 km and an offshore range up to 150 km, are evaluated to validate the altimeter Sea Surface Height (SSH) measurements. A method to derive HFR SSH mapped, with a varying spatial scale optimal interpolation, from the HFR velocities has been implemented. Evaluated, mainly, in the regions further than 25 km off the U.S. West coast, the HFR SSH shows good agreement with Jason-1-2 altimetry products over the years 2008 and 2009. Three Jason-2 PISTACH retrackers and one generic open ocean retracker have been analyzed using the traditional 1-Hz sampling rate. Near shore an experimental reprocessing of the 20-Hz range measurements is also tested to check for a gain in along-track spatial resolution. Referencing to the HFR SSH indicate the need to have several retrackers available, even over the continental shelf, with Ice3 fitting better during Bloom events and MLE-4 (or Red3) for high sea states. These studies demonstrate the value of HFR as a potential tool to correct coastal altimeter SSH, refine their spatial resolution and provide some insight into the altimeter behavior as a function of ocean conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20224" xmlns="http://purl.org/rss/1.0/"><title>Examining the global record of interannual variability in stratification and marine productivity in the low-and mid-latitude ocean</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20224</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Examining the global record of interannual variability in stratification and marine productivity in the low-and mid-latitude ocean</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Apurva C. Dave, M. Susan Lozier</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-06T10:35:56.066365-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20224</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20224</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20224</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Strengthened stratification of the upper ocean, associated with anthropogenic or climate-driven warming, is generally expected to inhibit marine primary productivity in light-replete, nutrient-limited environments - essentially, in the low and middle latitude ocean - based on the supposition that increased water column stability will inhibit vertical mixing and consequently the upward entrainment of deep nutrients into the euphotic zone. Herein, we examine the local stratification control of productivity on interannual time scales over the global subtropical and tropical ocean by directly comparing in situ measures of stratification (from hydrographic profile data) with contemporaneous values of ocean chlorophyll (from satellite data). In the subtropical ocean we find no evidence of a strong local correlative relationship between these properties over the observational record, a result that challenges the widely held view that stratification variability is a primary driver of interannual variability in nutrient supply and productivity in these waters. A strong negative relationship is observed, however, in the tropical Pacific, suggesting that previously reported correlations between globally-averaged stratification and productivity variability are driven by strong associations in this region. An examination of the long-term changes in our profile data also reveals trends of decreasing stratification scattered across the low- and mid-latitude ocean, driven by faster rates of warming in the subsurface relative to the surface. This observation seemingly undercuts a fundamental assumption of the paradigm of local stratification control, namely that increases in upper ocean heat content necessarily produce strengthened stratification.</p></div>
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Strengthened stratification of the upper ocean, associated with anthropogenic or climate-driven warming, is generally expected to inhibit marine primary productivity in light-replete, nutrient-limited environments - essentially, in the low and middle latitude ocean - based on the supposition that increased water column stability will inhibit vertical mixing and consequently the upward entrainment of deep nutrients into the euphotic zone. Herein, we examine the local stratification control of productivity on interannual time scales over the global subtropical and tropical ocean by directly comparing in situ measures of stratification (from hydrographic profile data) with contemporaneous values of ocean chlorophyll (from satellite data). In the subtropical ocean we find no evidence of a strong local correlative relationship between these properties over the observational record, a result that challenges the widely held view that stratification variability is a primary driver of interannual variability in nutrient supply and productivity in these waters. A strong negative relationship is observed, however, in the tropical Pacific, suggesting that previously reported correlations between globally-averaged stratification and productivity variability are driven by strong associations in this region. An examination of the long-term changes in our profile data also reveals trends of decreasing stratification scattered across the low- and mid-latitude ocean, driven by faster rates of warming in the subsurface relative to the surface. This observation seemingly undercuts a fundamental assumption of the paradigm of local stratification control, namely that increases in upper ocean heat content necessarily produce strengthened stratification.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20218" xmlns="http://purl.org/rss/1.0/"><title>Correction to “Physical modeling of tsunamis generated by three-dimensional deformable granular landslides"</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20218</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Correction to “Physical modeling of tsunamis generated by three-dimensional deformable granular landslides"</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Fahad Mohammed, Hermann M. Fritz</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-05T22:25:49.704235-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20218</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20218</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20218</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Correction</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20216" xmlns="http://purl.org/rss/1.0/"><title>Modeling the temperature-nitrate relationship in the coastal upwelling domain of the California Current</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20216</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Modeling the temperature-nitrate relationship in the coastal upwelling domain of the California Current</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Daniel M. Palacios, Elliott L. Hazen, Isaac D. Schroeder, Steven J. Bograd</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-03T23:58:26.400381-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20216</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20216</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20216</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Given the importance of nitrate in sustaining high primary production and fishery yields in eastern boundary current ecosystems, it is desirable to know the amounts of this nutrient reaching the euphotic zone through the upwelling process. Because such measurements are not routinely available, we developed predictive models of water-column (0-200 m) nitrate based on temperature for a region of the California Current System (CCS; 30-47°N) within 50 km from the coast. Prediction was done using generalized additive models (GAMs) based on a compilation of 37607 observations collected over the period 1959-2004 and validated with a separate set of 6430 observations for the period 2005-2011. A temperature-only model had relatively high explanatory power (explained deviance, <em>D<sup>2</sup></em> = 71.6%) but contained important depth, latitudinal and seasonal biases. A model incorporating salinity in addition to temperature (<em>D<sup>2</sup></em> = 91.2%) corrected for the latitudinal and depth biases but not the seasonal bias. The best model included oxygen, temperature and salinity (<em>D<sup>2</sup></em> = 96.6%) and adequately predicted nitrate temporal behavior at two widely separated locations (44°39.1′N and 32°54.6′N) with slight or no bias (RMSE = 2.39 and 0.40 µM, respectively). For situations when only temperature is available, a model including depth, month and latitude as proxy covariates corrects some of the biases, but it had lower predictive skill (RMSE = 2.50 μM and 5.22 μM, respectively). The results of this study have applications for the proxy derivation of nitrate availability for primary producers (phytoplankton, macroalgae) in upwelling regions, and for biogeochemical and ecosystem modeling studies.</p></div>
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Given the importance of nitrate in sustaining high primary production and fishery yields in eastern boundary current ecosystems, it is desirable to know the amounts of this nutrient reaching the euphotic zone through the upwelling process. Because such measurements are not routinely available, we developed predictive models of water-column (0-200 m) nitrate based on temperature for a region of the California Current System (CCS; 30-47°N) within 50 km from the coast. Prediction was done using generalized additive models (GAMs) based on a compilation of 37607 observations collected over the period 1959-2004 and validated with a separate set of 6430 observations for the period 2005-2011. A temperature-only model had relatively high explanatory power (explained deviance, D2 = 71.6%) but contained important depth, latitudinal and seasonal biases. A model incorporating salinity in addition to temperature (D2 = 91.2%) corrected for the latitudinal and depth biases but not the seasonal bias. The best model included oxygen, temperature and salinity (D2 = 96.6%) and adequately predicted nitrate temporal behavior at two widely separated locations (44°39.1′N and 32°54.6′N) with slight or no bias (RMSE = 2.39 and 0.40 µM, respectively). For situations when only temperature is available, a model including depth, month and latitude as proxy covariates corrects some of the biases, but it had lower predictive skill (RMSE = 2.50 μM and 5.22 μM, respectively). The results of this study have applications for the proxy derivation of nitrate availability for primary producers (phytoplankton, macroalgae) in upwelling regions, and for biogeochemical and ecosystem modeling studies.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20204" xmlns="http://purl.org/rss/1.0/"><title>Satellite observations of turbidity in the Dead Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20204</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Satellite observations of turbidity in the Dead Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Nehorai R, Lensky IM, Hochman L, Gertman I, Brenner S, Muskin A, Lensky NG</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-03T01:53:37.182581-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20204</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20204</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20204</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>A methodology to attain daily variability of turbidity in the Dead Sea by means of remote sensing was developed. 250 m/pixel MODIS surface reflectance data were used to characterize the seasonal cycle of turbidity and plume spreading generated by flood events in the lake. Fifteen minutes interval images from Meteosat Second Generation (MSG) 1.6 km/pixel High Resolution Visible (HRV) channel were used to monitor daily variations of turbidity. The HRV reflectance was normalized throughout the day to correct for the changing geometry and then calibrated against available MODIS surface reflectance. Finally, hourly averaged reflectance maps are presented for summer and winter. The results show that turbidity is concentrated along the silty shores of the lake and the southern embayments, with a gradual decrease of turbidity values from the shoreline towards the center of the lake. This pattern is most pronounced following the nighttime hours of intense winds. A few hours after winds calm the concentric turbidity pattern fades. In situ and remote sensing observations show a clear relation between wind intensity, wave amplitude and water turbidity. In summer and winter similar concentric turbidity patterns are observed but with a much narrower structure in winter. A simple Lagrangain trajectory model suggests that the combined effects of horizontal transport and vertical mixing of suspended particles leads to more effective mixing in winter. The dynamics of suspended matter contributions from winter desert floods are also presented in terms of hourly turbidity maps showing the spreading of the plumes and their decay.</p></div>
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A methodology to attain daily variability of turbidity in the Dead Sea by means of remote sensing was developed. 250 m/pixel MODIS surface reflectance data were used to characterize the seasonal cycle of turbidity and plume spreading generated by flood events in the lake. Fifteen minutes interval images from Meteosat Second Generation (MSG) 1.6 km/pixel High Resolution Visible (HRV) channel were used to monitor daily variations of turbidity. The HRV reflectance was normalized throughout the day to correct for the changing geometry and then calibrated against available MODIS surface reflectance. Finally, hourly averaged reflectance maps are presented for summer and winter. The results show that turbidity is concentrated along the silty shores of the lake and the southern embayments, with a gradual decrease of turbidity values from the shoreline towards the center of the lake. This pattern is most pronounced following the nighttime hours of intense winds. A few hours after winds calm the concentric turbidity pattern fades. In situ and remote sensing observations show a clear relation between wind intensity, wave amplitude and water turbidity. In summer and winter similar concentric turbidity patterns are observed but with a much narrower structure in winter. A simple Lagrangain trajectory model suggests that the combined effects of horizontal transport and vertical mixing of suspended particles leads to more effective mixing in winter. The dynamics of suspended matter contributions from winter desert floods are also presented in terms of hourly turbidity maps showing the spreading of the plumes and their decay.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20205" xmlns="http://purl.org/rss/1.0/"><title>AVHRR, MODIS, and VIIRS radiometric stability and consistency in SST bands</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20205</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">AVHRR, MODIS, and VIIRS radiometric stability and consistency in SST bands</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">XingMing Liang, Alexander Ignatov</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T06:57:46.839693-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20205</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20205</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20205</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">ABSTRACT</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Monitoring of IR Clear-Sky Radiances over Oceans for SST (MICROS; <!--TODO: clickthrough URL--><a href="http://www.star.nesdis.noaa.gov/sod/sst/micros" title="Link to external resource: http://www.star.nesdis.noaa.gov/sod/sst/micros">www.star.nesdis.noaa.gov/sod/sst/micros</a>) is NESDIS near-real time web-based radiance monitoring system. It analyzes <span class="underlined ">M</span>odel (Community Radiative Transfer Model, CRTM) minus <span class="underlined ">O</span>bservation (M-O) biases in brightness temperatures (BT) in three bands centered at 3.7 (IR37), 11 (IR11), and 12µm (IR12), for several AVHRR (NOAA-16, -17, -18, -19, Metop-A, -B), V<em>IIRS (Suomi National Polar Partnership, S-NPP),</em> and MODIS (Terra, Aqua) sensors. Double-differences (DD) are employed to check BTs for radiometric stability and consistency. All sensors are stable, with the exception of two AVHRRs, onboard NOAA-16 and to a lesser extent NOAA-18, and generally consistent. VIIRS onboard S-NPP, launched in October 2011, is well in-family, especially after its calibration was fine-tuned on 7 March 2012. MODIS M-O biases were initially out-of-family by up to -0.6 K, due to incorrect CRTM transmittance coefficients. Following MICROS feedback, CRTM Team updated coefficients and brought MODIS back in-family. Terra and Aqua BTs are very consistent in IR11 and IR12 but show cross-platform bias of 0.3 K in IR37, likely attributed to MODIS characterization. Work with MODIS Characterization Support Team is underway to resolve this. Initial analyses of AVHRR onboard Metop-B launched in September 2012 suggest that its BTs are offset from Metop-A by up to ~0.3 K. Overall, MICROS DDs are well suited to evaluate the sensors stability, but dedicated effort is needed to ensure consistent radiative transfer modeling (RTM) calculations for various sensors before DDs can be used in Global Space-based Inter-Calibration System (GSICS) quantitative applications.</p></div>
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Monitoring of IR Clear-Sky Radiances over Oceans for SST (MICROS; www.star.nesdis.noaa.gov/sod/sst/micros) is NESDIS near-real time web-based radiance monitoring system. It analyzes Model (Community Radiative Transfer Model, CRTM) minus Observation (M-O) biases in brightness temperatures (BT) in three bands centered at 3.7 (IR37), 11 (IR11), and 12µm (IR12), for several AVHRR (NOAA-16, -17, -18, -19, Metop-A, -B), VIIRS (Suomi National Polar Partnership, S-NPP), and MODIS (Terra, Aqua) sensors. Double-differences (DD) are employed to check BTs for radiometric stability and consistency. All sensors are stable, with the exception of two AVHRRs, onboard NOAA-16 and to a lesser extent NOAA-18, and generally consistent. VIIRS onboard S-NPP, launched in October 2011, is well in-family, especially after its calibration was fine-tuned on 7 March 2012. MODIS M-O biases were initially out-of-family by up to -0.6 K, due to incorrect CRTM transmittance coefficients. Following MICROS feedback, CRTM Team updated coefficients and brought MODIS back in-family. Terra and Aqua BTs are very consistent in IR11 and IR12 but show cross-platform bias of 0.3 K in IR37, likely attributed to MODIS characterization. Work with MODIS Characterization Support Team is underway to resolve this. Initial analyses of AVHRR onboard Metop-B launched in September 2012 suggest that its BTs are offset from Metop-A by up to ~0.3 K. Overall, MICROS DDs are well suited to evaluate the sensors stability, but dedicated effort is needed to ensure consistent radiative transfer modeling (RTM) calculations for various sensors before DDs can be used in Global Space-based Inter-Calibration System (GSICS) quantitative applications.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20200" xmlns="http://purl.org/rss/1.0/"><title>Clarifying the link between surface salinity and freshwater fluxes on monthly to inter-annual timescales</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20200</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Clarifying the link between surface salinity and freshwater fluxes on monthly to inter-annual timescales</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Nadya T. Vinogradova, Rui M. Ponte</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T03:23:39.757005-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20200</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20200</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20200</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>Freshwater fluxes (<em>F</em>) between the ocean and the atmosphere and land, comprised of evaporation, precipitation and terrestrial runoff, are an essential component of the Earth's climate system. However, direct observations of <em>F</em> and its components are sparse and available estimates have substantial uncertainties. In this study we investigate if measurements of sea surface salinity (<em>S</em>) can provide an alternative indirect method for estimating <em>F</em>. We examine the relationship between <em>S</em>, <em>F</em> and oceanic fluxes from surface advection and mixing processes, on time scales from months to years, using a consistent estimate of the ocean/atmosphere state obtained from model/data synthesis produced by the ECCO consortium. ECCO salinity averaged over the mixed layer is used as an estimate of <em>S</em>. Budget analysis shows that variability in <em>s</em> tendencies can be attributed to both <em>F</em> and oceanic fluxes, demonstrating the importance of the ocean's role in evolution of <em>s</em>, for both local and global mean fields. Regression analysis of the 13-year long ECCO fields shows that there are only a few regions (e.g., subtropical gyres) where <em>s</em> can be used as a proxy for <em>F</em> using linear models, and only at monthly to annual time scales. Results are similar over a range of spatial scales from ~100 to 2000 km. Findings are discussed in the context of the general sensitivities of <em>S</em> to atmospheric and oceanic processes and the potential of satellite salinity measurements to constrain estimates of <em>F</em></p></div>
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Freshwater fluxes (F) between the ocean and the atmosphere and land, comprised of evaporation, precipitation and terrestrial runoff, are an essential component of the Earth's climate system. However, direct observations of F and its components are sparse and available estimates have substantial uncertainties. In this study we investigate if measurements of sea surface salinity (S) can provide an alternative indirect method for estimating F. We examine the relationship between S, F and oceanic fluxes from surface advection and mixing processes, on time scales from months to years, using a consistent estimate of the ocean/atmosphere state obtained from model/data synthesis produced by the ECCO consortium. ECCO salinity averaged over the mixed layer is used as an estimate of S. Budget analysis shows that variability in s tendencies can be attributed to both F and oceanic fluxes, demonstrating the importance of the ocean's role in evolution of s, for both local and global mean fields. Regression analysis of the 13-year long ECCO fields shows that there are only a few regions (e.g., subtropical gyres) where s can be used as a proxy for F using linear models, and only at monthly to annual time scales. Results are similar over a range of spatial scales from ~100 to 2000 km. Findings are discussed in the context of the general sensitivities of S to atmospheric and oceanic processes and the potential of satellite salinity measurements to constrain estimates of F
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20238" xmlns="http://purl.org/rss/1.0/"><title>Estimating the volume and salt transports during a major inflow event in the Baltic Sea with the reanalysis of the hydrography based on 3DVAR</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20238</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Estimating the volume and salt transports during a major inflow event in the Baltic Sea with the reanalysis of the hydrography based on 3DVAR</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Weiwei Fu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T10:35:34.729531-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20238</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20238</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20238</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Volume and salt transports are estimated from three dimensional variational analysis (3DVAR) reanalysis in the Baltic Sea. With the assimilation of temperature and salinity profiles, we find that 3DVAR assimilation causes larger volume and salt transports into the Baltic Sea than directly estimated in the Skagerrak for the 2003 major inflow. In addition, the daily transport obtained as the derivatives of total salt and volume reveals pronounced difference from what is directly estimated. The reason is found to be related to the unbalanced part in the reanalysis obtained from weak constraint 3DVAR. The reanalysis of hydrography is further used to estimate the transport in the Danish strait. For the 2003 major inflow, the total net volume/salt transports across the Darss Sill and Drogden Sill are comparable to observations and other model studies. However, the effect of the 3DVAR assimilation amounts to a volume decrease of 7 km<sup>3</sup> and a salt increase of 0.23 Gt in the Arkona region. The reason is related to the barotropic flow through the Danish strait that was supposed to be enhanced in the reanalysis. It suggests that the solution of 3DVAR is statistically optimal but not physically balanced. In coastal regions, reanalysis data must be used with special care when transport is estimated. Meanwhile, misfit of the transports acquired in different ways helps to identify problems in the application of 3DVAR and the model quality.</p></div>
]]></content:encoded><description>Volume and salt transports are estimated from three dimensional variational analysis (3DVAR) reanalysis in the Baltic Sea. With the assimilation of temperature and salinity profiles, we find that 3DVAR assimilation causes larger volume and salt transports into the Baltic Sea than directly estimated in the Skagerrak for the 2003 major inflow. In addition, the daily transport obtained as the derivatives of total salt and volume reveals pronounced difference from what is directly estimated. The reason is found to be related to the unbalanced part in the reanalysis obtained from weak constraint 3DVAR. The reanalysis of hydrography is further used to estimate the transport in the Danish strait. For the 2003 major inflow, the total net volume/salt transports across the Darss Sill and Drogden Sill are comparable to observations and other model studies. However, the effect of the 3DVAR assimilation amounts to a volume decrease of 7 km3 and a salt increase of 0.23 Gt in the Arkona region. The reason is related to the barotropic flow through the Danish strait that was supposed to be enhanced in the reanalysis. It suggests that the solution of 3DVAR is statistically optimal but not physically balanced. In coastal regions, reanalysis data must be used with special care when transport is estimated. Meanwhile, misfit of the transports acquired in different ways helps to identify problems in the application of 3DVAR and the model quality.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20186" xmlns="http://purl.org/rss/1.0/"><title>Variability of the Atlantic off-equatorial eastward currents during 1993–2010 using a synthetic method</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20186</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Variability of the Atlantic off-equatorial eastward currents during 1993–2010 using a synthetic method</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Marlos Goes, Gustavo Goni, Verena Hormann, Renellys C. Perez</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T10:30:19.856925-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20186</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20186</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20186</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We have developed, validated, and applied a synthetic method to monitor the off-equatorial eastward currents in the central tropical Atlantic. This method combines high-density expendable bathythermograph (XBT) temperature data along the AX08 transect with altimetric sea level anomalies (SLAs) to estimate dynamic height fields from which the mean properties of the North Equatorial Countercurrent (NECC), the North Equatorial Undercurrent (NEUC) and the South Equatorial Undercurrent (SEUC), and their variability can be estimated on seasonal to interannual timescales. On seasonal to interannual timescales, the synthetic method is well suited for reconstructions of the NECC variability, reproduces the variability of the NEUC with considerable skill, and less efficiently describes variations of the SEUC, which is located in a region of low SLA variability. A positive correlation is found between interannual variations of the NECC transport and two indices based on an interhemispheric sea surface temperature (SST) gradient and southeasterly wind stress in the central tropical Atlantic. The NEUC is correlated on interannual timescales with SSTs and meridional wind stress in the Gulf of Guinea and zonal equatorial wind stress. This study shows that both altimetry and XBT data can be effectively combined for near-real-time inference of the dynamic and thermodynamic properties of the tropical Atlantic current system.</p></div>
]]></content:encoded><description>We have developed, validated, and applied a synthetic method to monitor the off-equatorial eastward currents in the central tropical Atlantic. This method combines high-density expendable bathythermograph (XBT) temperature data along the AX08 transect with altimetric sea level anomalies (SLAs) to estimate dynamic height fields from which the mean properties of the North Equatorial Countercurrent (NECC), the North Equatorial Undercurrent (NEUC) and the South Equatorial Undercurrent (SEUC), and their variability can be estimated on seasonal to interannual timescales. On seasonal to interannual timescales, the synthetic method is well suited for reconstructions of the NECC variability, reproduces the variability of the NEUC with considerable skill, and less efficiently describes variations of the SEUC, which is located in a region of low SLA variability. A positive correlation is found between interannual variations of the NECC transport and two indices based on an interhemispheric sea surface temperature (SST) gradient and southeasterly wind stress in the central tropical Atlantic. The NEUC is correlated on interannual timescales with SSTs and meridional wind stress in the Gulf of Guinea and zonal equatorial wind stress. This study shows that both altimetry and XBT data can be effectively combined for near-real-time inference of the dynamic and thermodynamic properties of the tropical Atlantic current system.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20195" xmlns="http://purl.org/rss/1.0/"><title>Barotropic and deep-referenced baroclinic SSH variability derived from Pressure Inverted Echo Sounders (PIES) south of Africa</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20195</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Barotropic and deep-referenced baroclinic SSH variability derived from Pressure Inverted Echo Sounders (PIES) south of Africa</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Behnisch, A. Macrander, O. Boebel, J.-O. Wolff, J. Schröter</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T08:55:52.63828-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20195</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20195</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20195</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The objective of this paper is to evaluate the baroclinic and barotropic components of sea surface height (SSH) anomalies in the Southern Ocean and investigates the causes for the weak correlation between hydrographically derived and satellite measured SSH anomalies. To this end, data obtained by six Pressure Inverted Echo Sounders (PIES) deployed south of Africa were used to derive baroclinic and barotropic SSH anomalies. Our results show that the barotropic component accounts for 30%–60% of the variability between the jets of the Antarctic Circumpolar Current (ACC). In contrast, the jets associated with the major ACC fronts are predominantly baroclinic. The deep baroclinic component is important in the ACC and accounts for the major part of the baroclinic variability. The comparison with along-track satellite altimetry (Jason 1/2) shows correlations coefficients of 0.24–0.92, with low values in regions of high-barotropic variability. The comparison with gridded Aviso satellite altimetry generally shows higher correlation coefficients (0.33–0.92) and lower root mean square (RMS) errors compared to the along-track product. In conclusion the barotropic SSH anomaly plays a major role in this region and has to be accounted for when assimilating SSH into ocean models. Due to their high-baroclinic component, the correct representation of the time and space varying ACC fronts seems to be crucial for the right SSH anomaly partitioning used for assimilation purposes. Gridded products, namely Aviso, seems to be more suitable compared to along-track products (Jason 1/2) in representing the variability of SSH anomalies.</p></div>
]]></content:encoded><description>The objective of this paper is to evaluate the baroclinic and barotropic components of sea surface height (SSH) anomalies in the Southern Ocean and investigates the causes for the weak correlation between hydrographically derived and satellite measured SSH anomalies. To this end, data obtained by six Pressure Inverted Echo Sounders (PIES) deployed south of Africa were used to derive baroclinic and barotropic SSH anomalies. Our results show that the barotropic component accounts for 30%–60% of the variability between the jets of the Antarctic Circumpolar Current (ACC). In contrast, the jets associated with the major ACC fronts are predominantly baroclinic. The deep baroclinic component is important in the ACC and accounts for the major part of the baroclinic variability. The comparison with along-track satellite altimetry (Jason 1/2) shows correlations coefficients of 0.24–0.92, with low values in regions of high-barotropic variability. The comparison with gridded Aviso satellite altimetry generally shows higher correlation coefficients (0.33–0.92) and lower root mean square (RMS) errors compared to the along-track product. In conclusion the barotropic SSH anomaly plays a major role in this region and has to be accounted for when assimilating SSH into ocean models. Due to their high-baroclinic component, the correct representation of the time and space varying ACC fronts seems to be crucial for the right SSH anomaly partitioning used for assimilation purposes. Gridded products, namely Aviso, seems to be more suitable compared to along-track products (Jason 1/2) in representing the variability of SSH anomalies.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20222" xmlns="http://purl.org/rss/1.0/"><title>Analysis of the potential and limitations of microwave radiometry for the retrieval of sea surface temperature: Definition of MICROWAT, a new mission concept</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20222</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Analysis of the potential and limitations of microwave radiometry for the retrieval of sea surface temperature: Definition of MICROWAT, a new mission concept</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. Prigent, F. Aires, F. Bernardo, J.-C. Orlhac, J.-M. Goutoule, H. Roquet, C. Donlon</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T08:43:53.442928-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20222</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20222</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20222</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The sensitivity of passive microwave observations to the sea surface temperature (SST) is carefully analyzed, with the objective of designing an optimized satellite instrument, MICROwave Wind And Temperature (MICROWAT), dedicated to an “all-weather” estimation of the SST at high spatial resolution (15 km). Our study stresses the importance of low-frequency observations around 6 GHz for accurate SST retrieval. Compared to the 11 GHz channel, the 6 GHz channel provides more sensitivity to the low SSTs and offers lower instrument noise, thanks to possibly broader channel bandwidths. However, it requires much larger antenna size for a given spatial resolution. Two instrument concepts have been suggested, one using a classic real aperture antenna and the other using synthetic interferometric antennas. This first analysis shows that 2-D interferometric systems would be very complex and would not satisfy the user requirements in terms of SST accuracy. A 1-D interferometric system could be proposed, but its development requires additional investigation. A dedicated conical scanner onboard a microsatellite with a 6 m antenna and channels at 6.9 and 18.7 GHz (both with V and H polarizations) can provide an SST accuracy of 0.3 K with a 15 km spatial resolution, with today's technology.</p></div>
]]></content:encoded><description>The sensitivity of passive microwave observations to the sea surface temperature (SST) is carefully analyzed, with the objective of designing an optimized satellite instrument, MICROwave Wind And Temperature (MICROWAT), dedicated to an “all-weather” estimation of the SST at high spatial resolution (15 km). Our study stresses the importance of low-frequency observations around 6 GHz for accurate SST retrieval. Compared to the 11 GHz channel, the 6 GHz channel provides more sensitivity to the low SSTs and offers lower instrument noise, thanks to possibly broader channel bandwidths. However, it requires much larger antenna size for a given spatial resolution. Two instrument concepts have been suggested, one using a classic real aperture antenna and the other using synthetic interferometric antennas. This first analysis shows that 2-D interferometric systems would be very complex and would not satisfy the user requirements in terms of SST accuracy. A 1-D interferometric system could be proposed, but its development requires additional investigation. A dedicated conical scanner onboard a microsatellite with a 6 m antenna and channels at 6.9 and 18.7 GHz (both with V and H polarizations) can provide an SST accuracy of 0.3 K with a 15 km spatial resolution, with today's technology.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20225" xmlns="http://purl.org/rss/1.0/"><title>Hydrodynamics of spur and groove formations on a coral reef</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20225</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Hydrodynamics of spur and groove formations on a coral reef</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Justin S. Rogers, Stephen G. Monismith, Falk Feddersen, Curt D. Storlazzi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T08:40:09.531914-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20225</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20225</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20225</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Spur and groove (SAG) formations are found on the fore reefs of many coral reefs worldwide. Although these formations are primarily present in wave-dominated environments, their effect on wave-driven hydrodynamics is not well understood. A two-dimensional, depth-averaged, phase-resolving nonlinear Boussinesq model (<em>funwaveC</em>) was used to model hydrodynamics on a simplified SAG system. The modeling results show that the SAG formations together with shoaling waves induce a nearshore Lagrangian circulation pattern of counter-rotating circulation cells. The mechanism driving the modeled flow is an alongshore imbalance between the pressure gradient (PG) and nonlinear wave (NLW) terms in the momentum balance. Variations in model parameters suggest the strongest factors affecting circulation include spur-normal waves, increased wave height, weak alongshore currents, increased spur height, and decreased bottom drag. The modeled circulation is consistent with a simple scaling analysis based on the dynamical balance of NLW, PG, and bottom stress terms. Model results indicate that the SAG formations efficiently drive circulation cells when the alongshore SAG wavelength allows for the effects of diffraction to create alongshore differences in wave height without changing the mean wave angle.</p></div>
]]></content:encoded><description>Spur and groove (SAG) formations are found on the fore reefs of many coral reefs worldwide. Although these formations are primarily present in wave-dominated environments, their effect on wave-driven hydrodynamics is not well understood. A two-dimensional, depth-averaged, phase-resolving nonlinear Boussinesq model (funwaveC) was used to model hydrodynamics on a simplified SAG system. The modeling results show that the SAG formations together with shoaling waves induce a nearshore Lagrangian circulation pattern of counter-rotating circulation cells. The mechanism driving the modeled flow is an alongshore imbalance between the pressure gradient (PG) and nonlinear wave (NLW) terms in the momentum balance. Variations in model parameters suggest the strongest factors affecting circulation include spur-normal waves, increased wave height, weak alongshore currents, increased spur height, and decreased bottom drag. The modeled circulation is consistent with a simple scaling analysis based on the dynamical balance of NLW, PG, and bottom stress terms. Model results indicate that the SAG formations efficiently drive circulation cells when the alongshore SAG wavelength allows for the effects of diffraction to create alongshore differences in wave height without changing the mean wave angle.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20237" xmlns="http://purl.org/rss/1.0/"><title>Seasonal variability of light absorption properties and water optical constituents in Hudson Bay, Canada</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20237</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seasonal variability of light absorption properties and water optical constituents in Hudson Bay, Canada</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Hongyan Xi, Pierre Larouche, Shilin Tang, Christine Michel</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-19T08:14:12.350601-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20237</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20237</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20237</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Previous studies have shown that the properties of optically significant water constituents (phytoplankton, suspended matter, and colored dissolved organic matter (CDOM)) in Hudson Bay are different from other Arctic regions. A new bio-optical data set collected in summer 2010 shows that this region also presents seasonal variability of the light absorption coefficients by the different constituents, with a higher relative proportion of CDOM absorption in summer than in the fall as a result of decreased phytoplankton absorption in summer. The slope of the exponential function describing nonalgal particles and CDOM spectral absorption shows little variability between fall and summer. Seasonal variability of light absorption coefficients and water optical constituents is more pronounced near the coast, while less variability is observed in the central part of the bay. Very low summertime chlorophyll-specific absorption coefficients by phytoplankton, among the lowest reported in the literature, are attributed to the high proportion of large size phytoplankton (microphytoplankton) and important packaging effect. There is also a smaller contribution of accessory pigments to total pigments in the summer than in the fall, resulting in a lower blue-to-red phytoplankton absorption ratio. These results emphasize that it is necessary to take into account the seasonal variability of light absorption properties in bio-optical models for further remote sensing applications in Hudson Bay.</p></div>
]]></content:encoded><description>Previous studies have shown that the properties of optically significant water constituents (phytoplankton, suspended matter, and colored dissolved organic matter (CDOM)) in Hudson Bay are different from other Arctic regions. A new bio-optical data set collected in summer 2010 shows that this region also presents seasonal variability of the light absorption coefficients by the different constituents, with a higher relative proportion of CDOM absorption in summer than in the fall as a result of decreased phytoplankton absorption in summer. The slope of the exponential function describing nonalgal particles and CDOM spectral absorption shows little variability between fall and summer. Seasonal variability of light absorption coefficients and water optical constituents is more pronounced near the coast, while less variability is observed in the central part of the bay. Very low summertime chlorophyll-specific absorption coefficients by phytoplankton, among the lowest reported in the literature, are attributed to the high proportion of large size phytoplankton (microphytoplankton) and important packaging effect. There is also a smaller contribution of accessory pigments to total pigments in the summer than in the fall, resulting in a lower blue-to-red phytoplankton absorption ratio. These results emphasize that it is necessary to take into account the seasonal variability of light absorption properties in bio-optical models for further remote sensing applications in Hudson Bay.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20234" xmlns="http://purl.org/rss/1.0/"><title>Multiscale variability in the Balearic Sea: An altimetric perspective</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20234</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Multiscale variability in the Balearic Sea: An altimetric perspective</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Evan Mason, Ananda Pascual</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-17T08:26:38.608305-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20234</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20234</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20234</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The present-day availability of an 18 year record of 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20234/asset/equation/jgrc20234-math-0001.gif?v=1&amp;t=hi5l2oba&amp;s=3f1ee30eb7dddee66e6457c7538d2ce8e8a07eeb" class="inlineGraphic"/> merged Mediterranean Sea sea level anomaly (SLA) data enables a contemporary description of long-term mesoscale activity in the Balearic Sea. SLA data from satellite altimetry are used to study the variability of sea level and surface geostrophic circulation at different spatial and temporal scales within this complex and relatively understudied region in the western Mediterranean (WMED). We find that the mean Northern Current along the Iberian slope is strongest in autumn, although higher variability in winter leads to stronger peaks in kinetic energy. The Balearic Current, which flows along the northern slopes of the Balearic islands, also has its maximum expression in autumn. Across the two Balearic channels (Ibiza and Mallorca), key locations that partly regulate meridional exchange in the WMED, observed seasonal variability in geostrophic velocity anomalies conforms rather well to prior descriptions, suggesting cautious confidence in the use of the Mediterranean merged altimeter product in nearshore regions. Circulation through the channels is maximum in winter. The channel data support the hypothesis that the channel circulation may be hindered by the intermittent presence of the Western Intermediate Water mass, which sometimes forms in winter in the Gulf of Lions. This is the first time that an analysis of variability in the Balearic channels has been performed using altimetric data.</p></div>
]]></content:encoded><description>The present-day availability of an 18 year record of 
1/8° merged Mediterranean Sea sea level anomaly (SLA) data enables a contemporary description of long-term mesoscale activity in the Balearic Sea. SLA data from satellite altimetry are used to study the variability of sea level and surface geostrophic circulation at different spatial and temporal scales within this complex and relatively understudied region in the western Mediterranean (WMED). We find that the mean Northern Current along the Iberian slope is strongest in autumn, although higher variability in winter leads to stronger peaks in kinetic energy. The Balearic Current, which flows along the northern slopes of the Balearic islands, also has its maximum expression in autumn. Across the two Balearic channels (Ibiza and Mallorca), key locations that partly regulate meridional exchange in the WMED, observed seasonal variability in geostrophic velocity anomalies conforms rather well to prior descriptions, suggesting cautious confidence in the use of the Mediterranean merged altimeter product in nearshore regions. Circulation through the channels is maximum in winter. The channel data support the hypothesis that the channel circulation may be hindered by the intermittent presence of the Western Intermediate Water mass, which sometimes forms in winter in the Gulf of Lions. This is the first time that an analysis of variability in the Balearic channels has been performed using altimetric data.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20201" xmlns="http://purl.org/rss/1.0/"><title>Estimation of relative phycoerythrin concentrations from hyperspectral underwater radiance measurements––A statistical approach</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20201</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Estimation of relative phycoerythrin concentrations from hyperspectral underwater radiance measurements––A statistical approach</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Bettina B. Taylor, Marc H. Taylor, Tilman Dinter, Astrid Bracher</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-14T14:53:13.655219-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20201</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20201</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20201</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Phycobiliproteins are a family of water-soluble pigment proteins that play an important role as accessory or antenna pigments and absorb in the green part of the light spectrum poorly used by chlorophyll <em>a</em>. The phycoerythrins (PEs) are one of four types of phycobiliproteins that are generally distinguished based on their absorption properties. As PEs are water soluble, they are generally not captured with conventional pigment analysis. Here we present a statistical model based on in situ measurements of three transatlantic cruises which allows us to derive relative PE concentration from standardized hyperspectral underwater radiance measurements (<em>L<sub>u</sub></em>). The model relies on Empirical Orthogonal Function (EOF) analysis of <em>L<sub>u</sub></em> spectra and, subsequently, a Generalized Linear Model with measured PE concentrations as the response variable and EOF loadings as predictor variables. The method is used to predict relative PE concentrations throughout the water column and to calculate integrated PE estimates based on those profiles.</p></div>
]]></content:encoded><description>Phycobiliproteins are a family of water-soluble pigment proteins that play an important role as accessory or antenna pigments and absorb in the green part of the light spectrum poorly used by chlorophyll a. The phycoerythrins (PEs) are one of four types of phycobiliproteins that are generally distinguished based on their absorption properties. As PEs are water soluble, they are generally not captured with conventional pigment analysis. Here we present a statistical model based on in situ measurements of three transatlantic cruises which allows us to derive relative PE concentration from standardized hyperspectral underwater radiance measurements (Lu). The model relies on Empirical Orthogonal Function (EOF) analysis of Lu spectra and, subsequently, a Generalized Linear Model with measured PE concentrations as the response variable and EOF loadings as predictor variables. The method is used to predict relative PE concentrations throughout the water column and to calculate integrated PE estimates based on those profiles.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20206" xmlns="http://purl.org/rss/1.0/"><title>A model for partitioning the light absorption coefficient of suspended marine particles into phytoplankton and nonalgal components</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20206</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A model for partitioning the light absorption coefficient of suspended marine particles into phytoplankton and nonalgal components</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Guangming Zheng, Dariusz Stramski</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-14T14:51:40.496275-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20206</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20206</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20206</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We developed a model for partitioning the spectral absorption coefficient of suspended marine particles, <em>a<sub>p</sub></em>(<em>λ</em>), into phytoplankton, <em>a</em><sub><em>ph</em></sub>(<em>λ</em>), and nonalgal, <em>a<sub>d</sub></em>(<em>λ</em>), components based on the stacked-constraints approach. The key aspect of our model is the use of a set of inequality constraints that account for large variability in the <em>a</em><sub><em>ph</em></sub>(<em>λ</em>) and <em>a<sub>d</sub></em>(<em>λ</em>) coefficients within the world's oceans. The bounds of inequality constraints were determined from the analysis of a comprehensive set of 505 field determinations of absorption coefficients in various oceanic environments. The feasible solutions of the model are found by simultaneously satisfying all inequality constraints. The optimal solutions represented by the median values of feasible solutions for <em>a</em><sub><em>ph</em></sub>(<em>λ</em>) and <em>a<sub>d</sub></em>(<em>λ</em>) generally agree well with field measurements and are superior in terms of error statistics compared with previous partitioning models. For example, on the basis of comparisons of optimal model solutions with field determinations of absorption coefficients, the systematic error calculated as the median ratio of model-derived to measured values for both <em>a</em><sub><em>ph</em></sub>(443) and <em>a<sub>d</sub></em>(443) is within ±1% for our model. The random error represented by the mean absolute percent difference for <em>a</em><sub><em>ph</em></sub>(443) and <em>a<sub>d</sub></em>(443) is &lt;5% and &lt;20%, respectively. This study suggests that our model has the potential for successful applications with input data of <em>a<sub>p</sub></em>(<em>λ</em>) which can be collected from various oceanographic platforms.</p></div>
]]></content:encoded><description>We developed a model for partitioning the spectral absorption coefficient of suspended marine particles, ap(λ), into phytoplankton, aph(λ), and nonalgal, ad(λ), components based on the stacked-constraints approach. The key aspect of our model is the use of a set of inequality constraints that account for large variability in the aph(λ) and ad(λ) coefficients within the world's oceans. The bounds of inequality constraints were determined from the analysis of a comprehensive set of 505 field determinations of absorption coefficients in various oceanic environments. The feasible solutions of the model are found by simultaneously satisfying all inequality constraints. The optimal solutions represented by the median values of feasible solutions for aph(λ) and ad(λ) generally agree well with field measurements and are superior in terms of error statistics compared with previous partitioning models. For example, on the basis of comparisons of optimal model solutions with field determinations of absorption coefficients, the systematic error calculated as the median ratio of model-derived to measured values for both aph(443) and ad(443) is within ±1% for our model. The random error represented by the mean absolute percent difference for aph(443) and ad(443) is &lt;5% and &lt;20%, respectively. This study suggests that our model has the potential for successful applications with input data of ap(λ) which can be collected from various oceanographic platforms.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20210" xmlns="http://purl.org/rss/1.0/"><title>Global ocean surface velocities from drifters: Mean, variance, El Niño–Southern Oscillation response, and seasonal cycle</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20210</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Global ocean surface velocities from drifters: Mean, variance, El Niño–Southern Oscillation response, and seasonal cycle</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rick Lumpkin, Gregory C. Johnson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-14T14:41:42.393236-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20210</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20210</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20210</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Global near-surface currents are calculated from satellite-tracked drogued drifter velocities on a 0.5° × 0.5° latitude-longitude grid using a new methodology. Data used at each grid point lie within a centered bin of set area with a shape defined by the variance ellipse of current fluctuations within that bin. The time-mean current, its annual harmonic, semiannual harmonic, correlation with the Southern Oscillation Index (SOI), spatial gradients, and residuals are estimated along with formal error bars for each component. The time-mean field resolves the major surface current systems of the world. The magnitude of the variance reveals enhanced eddy kinetic energy in the western boundary current systems, in equatorial regions, and along the Antarctic Circumpolar Current, as well as three large “eddy deserts,” two in the Pacific and one in the Atlantic. The SOI component is largest in the western and central tropical Pacific, but can also be seen in the Indian Ocean. Seasonal variations reveal details such as the gyre-scale shifts in the convergence centers of the subtropical gyres, and the seasonal evolution of tropical currents and eddies in the western tropical Pacific Ocean. The results of this study are available as a monthly climatology.</p></div>
]]></content:encoded><description>Global near-surface currents are calculated from satellite-tracked drogued drifter velocities on a 0.5° × 0.5° latitude-longitude grid using a new methodology. Data used at each grid point lie within a centered bin of set area with a shape defined by the variance ellipse of current fluctuations within that bin. The time-mean current, its annual harmonic, semiannual harmonic, correlation with the Southern Oscillation Index (SOI), spatial gradients, and residuals are estimated along with formal error bars for each component. The time-mean field resolves the major surface current systems of the world. The magnitude of the variance reveals enhanced eddy kinetic energy in the western boundary current systems, in equatorial regions, and along the Antarctic Circumpolar Current, as well as three large “eddy deserts,” two in the Pacific and one in the Atlantic. The SOI component is largest in the western and central tropical Pacific, but can also be seen in the Indian Ocean. Seasonal variations reveal details such as the gyre-scale shifts in the convergence centers of the subtropical gyres, and the seasonal evolution of tropical currents and eddies in the western tropical Pacific Ocean. The results of this study are available as a monthly climatology.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20202" xmlns="http://purl.org/rss/1.0/"><title>Climate change projection of the Tasman Sea from an Eddy-resolving Ocean Model</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20202</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Climate change projection of the Tasman Sea from an Eddy-resolving Ocean Model</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. J. Matear, M. A. Chamberlain, C. Sun, M. Feng</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-14T14:38:59.496445-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20202</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20202</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20202</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The ocean's western boundary current regions display the greatest rate of twentieth century warming and global climate models project that the accelerated rate of warming will continue with climate change. All existing global climate change projections come from simulations that do not fully resolve either these boundary currents or their eddies. Using an Ocean Eddy-resolving Model (OEM) that captures the dynamics of the East Australian Current (EAC) and its eddies we show the response of the Tasman Sea to climate change differs from what is projected with a coarse resolution Global Climate Model (GCM). With climate change, the OEM projects increased EAC transport with increased eddy activity and an approximately 1° southward latitudinal shift in the point where the EAC separates from the shelf and flows eastward. The OEM increased eddy activity in the Tasman Sea with climate change increases the nutrient supply to the upper ocean and causes an increase in the phytoplankton concentrations and primary productivity by 10% in the oligotrophic waters of the Tasman Sea. The increase in primary productivity is absent in the GCM climate change projection, which projects the region will have a decrease in primary productivity with climate change. Applying the OEM climate change projection for the Tasman Sea to other western boundary current regions suggests the projected intensification of all western boundary currents with climate change should increase eddy activity and provide an important nutrient supply mechanism to counter the increased stratification projected with global warming.</p></div>
]]></content:encoded><description>The ocean's western boundary current regions display the greatest rate of twentieth century warming and global climate models project that the accelerated rate of warming will continue with climate change. All existing global climate change projections come from simulations that do not fully resolve either these boundary currents or their eddies. Using an Ocean Eddy-resolving Model (OEM) that captures the dynamics of the East Australian Current (EAC) and its eddies we show the response of the Tasman Sea to climate change differs from what is projected with a coarse resolution Global Climate Model (GCM). With climate change, the OEM projects increased EAC transport with increased eddy activity and an approximately 1° southward latitudinal shift in the point where the EAC separates from the shelf and flows eastward. The OEM increased eddy activity in the Tasman Sea with climate change increases the nutrient supply to the upper ocean and causes an increase in the phytoplankton concentrations and primary productivity by 10% in the oligotrophic waters of the Tasman Sea. The increase in primary productivity is absent in the GCM climate change projection, which projects the region will have a decrease in primary productivity with climate change. Applying the OEM climate change projection for the Tasman Sea to other western boundary current regions suggests the projected intensification of all western boundary currents with climate change should increase eddy activity and provide an important nutrient supply mechanism to counter the increased stratification projected with global warming.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20223" xmlns="http://purl.org/rss/1.0/"><title>An assessment of the skill of real-time models of Mid-Atlantic Bight continental shelf circulation</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20223</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">An assessment of the skill of real-time models of Mid-Atlantic Bight continental shelf circulation</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">John L. Wilkin, Elias J. Hunter</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-13T15:11:41.995437-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20223</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20223</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20223</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Prescribing open boundary conditions for regional coastal ocean models encounters the challenge of imposing information on sea level, velocity and tracers that characterize the unrepresented far field ocean. Deriving such information from a larger domain model without communicating information from the “nested” model back to the exterior model is “downscaling”. We evaluate whether real-time models presently in operation for the Mid-Atlantic Bight (MAB) can deliver useful predictions of subtidal frequency currents and subsurface temperature and salinity for this downscaling purpose. The MAB is a broad continental shelf region where several models run in real time and there is a dense observational data set available for skill assessment. We examine seven real-time models that cover the MAB: three global models, and four regional models. A regional climatology is included as an eighth model. Skill metrics with respect to model bias, centered root mean square error and cross correlation are computed for temperature and salinity profile data from 16 autonomous underwater glider vehicle missions and four hydrographic voyages in 2010–2011. Two years of hourly HF-radar surface current observations that span the shelf are used to evaluate modeled mean surface currents and daily time scale variability in speed and direction. Skill metrics, with uncertainty estimates, are reported for inner and outer shelf subregions, and for stratified and unstratified seasons. A group of models is identified that offers useful skill for the purposes of providing open boundary data to inner shelf and estuary models for real-time applications.</p></div>
]]></content:encoded><description>Prescribing open boundary conditions for regional coastal ocean models encounters the challenge of imposing information on sea level, velocity and tracers that characterize the unrepresented far field ocean. Deriving such information from a larger domain model without communicating information from the “nested” model back to the exterior model is “downscaling”. We evaluate whether real-time models presently in operation for the Mid-Atlantic Bight (MAB) can deliver useful predictions of subtidal frequency currents and subsurface temperature and salinity for this downscaling purpose. The MAB is a broad continental shelf region where several models run in real time and there is a dense observational data set available for skill assessment. We examine seven real-time models that cover the MAB: three global models, and four regional models. A regional climatology is included as an eighth model. Skill metrics with respect to model bias, centered root mean square error and cross correlation are computed for temperature and salinity profile data from 16 autonomous underwater glider vehicle missions and four hydrographic voyages in 2010–2011. Two years of hourly HF-radar surface current observations that span the shelf are used to evaluate modeled mean surface currents and daily time scale variability in speed and direction. Skill metrics, with uncertainty estimates, are reported for inner and outer shelf subregions, and for stratified and unstratified seasons. A group of models is identified that offers useful skill for the purposes of providing open boundary data to inner shelf and estuary models for real-time applications.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20212" xmlns="http://purl.org/rss/1.0/"><title>Oceanographic observations at the shelf break of the Amundsen Sea, Antarctica</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20212</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Oceanographic observations at the shelf break of the Amundsen Sea, Antarctica</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Dziga P. Walker, Adrian Jenkins, Karen M. Assmann, Deborah R. Shoosmith, Mark A. Brandon</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-13T09:08:42.7727-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20212</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20212</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20212</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The glaciers draining into the Amundsen Sea Embayment are rapidly losing mass, making a significant contribution to current sea level rise. Studies of Pine Island Glacier (PIG) in this region indicate that the mass loss is associated with rapid melting of its floating ice shelf driven by warm Circumpolar Deep Water (CDW) that is able to penetrate all the way to its grounding line, and that recent intensification of the mass loss is associated with higher melt rates and stronger subice-shelf circulation. CDW is sourced from within the Antarctic Circumpolar Current (ACC) situated well north of the glacial ice fronts. To be able to access the Amundsen Sea glaciers, CDW must first cross the continental shelf break where the deep ocean meets the shallower waters of the continental shelf. Here, we present data that shows how CDW moves along the continental slope and across the shelf break into the Amundsen Sea. On-shelf flow of CDW is enhanced where a subsea trough bisects the shelf edge. A previously unreported undercurrent is observed flowing eastward along the shelf edge and when this current encounters the trough mouth it circulates southward into the trough and toward the glaciers. Upwelling associated with this trough circulation appears to allow Lower CDW onto the shelf that would otherwise be blocked by the topography. These observations concur with the results of a theoretical modeling study of circulation in a similar topographic setting and also with the results of a regional ocean/ice modeling study of the Amundsen Sea specifically.</p></div>
]]></content:encoded><description>The glaciers draining into the Amundsen Sea Embayment are rapidly losing mass, making a significant contribution to current sea level rise. Studies of Pine Island Glacier (PIG) in this region indicate that the mass loss is associated with rapid melting of its floating ice shelf driven by warm Circumpolar Deep Water (CDW) that is able to penetrate all the way to its grounding line, and that recent intensification of the mass loss is associated with higher melt rates and stronger subice-shelf circulation. CDW is sourced from within the Antarctic Circumpolar Current (ACC) situated well north of the glacial ice fronts. To be able to access the Amundsen Sea glaciers, CDW must first cross the continental shelf break where the deep ocean meets the shallower waters of the continental shelf. Here, we present data that shows how CDW moves along the continental slope and across the shelf break into the Amundsen Sea. On-shelf flow of CDW is enhanced where a subsea trough bisects the shelf edge. A previously unreported undercurrent is observed flowing eastward along the shelf edge and when this current encounters the trough mouth it circulates southward into the trough and toward the glaciers. Upwelling associated with this trough circulation appears to allow Lower CDW onto the shelf that would otherwise be blocked by the topography. These observations concur with the results of a theoretical modeling study of circulation in a similar topographic setting and also with the results of a regional ocean/ice modeling study of the Amundsen Sea specifically.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20229" xmlns="http://purl.org/rss/1.0/"><title>Sea-level trends and interannual variability in the Caribbean Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20229</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea-level trends and interannual variability in the Caribbean Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. Ricardo Torres, Michael N. Tsimplis</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-13T09:02:32.471397-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20229</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20229</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20229</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Sea-level trends and their forcing have been investigated in the Caribbean Sea using altimetry and tide gauge time series from 19 stations. The basin average sea-level rise is 1.7 ± 1.3 mm yr<sup>−1</sup> for the period 1993–2010. Significant spatial variability of the trends is found. The steric variability above 800 m combined with the global isostatic adjustment explains the observed trends for the altimetry period in most of the basin. Wind forcing changes causes the trends in the southern part of the basin, modulating the sea level through changes in the ocean circulation. The longest time series (102 years) of Cristobal shows a trend of 1.9 ± 0.1 mm yr<sup>−1</sup> insignificantly different from the global mean sea-level rise for the twentieth century. By contrast Cartagena, a world heritage site, has a large trend (5.3 ± 0.3 mm yr<sup>−1</sup>) significantly affected by local vertical land movements. Stations dominated by the steric contribution have smaller trends (∼1.3 ± 0.2 mm yr<sup>−1</sup>). Sea-level trends at tide gauges are not affected by atmospheric pressure changes or by the open ocean steric contribution at most stations. Decadal variability in the sea-level trends can partly be explained by steric and wind variability. The decadal variability in the trends is not spatially coherent. Interannual sea-level variability accounts for one third of the total sea-level variability and can be partly explained by the influence of El Niño-Southern Oscillation at different time and spatial scales. No correlation with the North Atlantic Oscillation is found.</p></div>
]]></content:encoded><description>Sea-level trends and their forcing have been investigated in the Caribbean Sea using altimetry and tide gauge time series from 19 stations. The basin average sea-level rise is 1.7 ± 1.3 mm yr−1 for the period 1993–2010. Significant spatial variability of the trends is found. The steric variability above 800 m combined with the global isostatic adjustment explains the observed trends for the altimetry period in most of the basin. Wind forcing changes causes the trends in the southern part of the basin, modulating the sea level through changes in the ocean circulation. The longest time series (102 years) of Cristobal shows a trend of 1.9 ± 0.1 mm yr−1 insignificantly different from the global mean sea-level rise for the twentieth century. By contrast Cartagena, a world heritage site, has a large trend (5.3 ± 0.3 mm yr−1) significantly affected by local vertical land movements. Stations dominated by the steric contribution have smaller trends (∼1.3 ± 0.2 mm yr−1). Sea-level trends at tide gauges are not affected by atmospheric pressure changes or by the open ocean steric contribution at most stations. Decadal variability in the sea-level trends can partly be explained by steric and wind variability. The decadal variability in the trends is not spatially coherent. Interannual sea-level variability accounts for one third of the total sea-level variability and can be partly explained by the influence of El Niño-Southern Oscillation at different time and spatial scales. No correlation with the North Atlantic Oscillation is found.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20227" xmlns="http://purl.org/rss/1.0/"><title>The source of the Canary current in fall 2009</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20227</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The source of the Canary current in fall 2009</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Dolores Pérez-Hernández, Alonso Hernández-Guerra, Eugenio Fraile-Nuez, Isis Comas-Rodríguez, Verónica M. Benítez-Barrios, J. Francisco Domínguez-Yanes, Pedro Vélez-Belchí, Demetrio Armas</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-11T15:41:41.76099-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20227</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20227</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20227</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The source of the Canary Current has been inferred from an inverse box model applied to the hydrographic data of a survey carried out in 2009 in the northeast subtropical gyre (29–37°N, 9–24°W). The Portugal Current is observed between 13.5 and 14.8°W at 37°N carrying 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0001.gif?v=1&amp;t=hi5l2oc8&amp;s=2ccf5347288b182cd4fa31c64cdab5561cb6bdfe" class="inlineGraphic"/> Sv southward. This current presumably merges with the eastward transport of the Azores Current System and partly contributes to the Mediterranean inflow and partly to the northward recirculation of the Azores Current through the Gulf of Cadiz. The Azores Current System is located in the meridional range 33.50–36.25°N at 24.50°W. This System transports eastward 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0002.gif?v=1&amp;t=hi5l2oc8&amp;s=1269541be196b673552faef58ada3b271c928980" class="inlineGraphic"/> Sv in the thermocline layers and 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0003.gif?v=1&amp;t=hi5l2oc8&amp;s=8bbb761f0042a339f32dbad31d63b35d5c413089" class="inlineGraphic"/> Sv at intermediate layers. The Azores Current intermediate water mass has the highest portion of Sub-Arctic intermediate water (SAIW) in the region, while the Azores Countercurrent intermediate waters mass is mainly Mediterranean water. The Canary Current extends from 22.25° to 18.50°W at 29°N, the westernmost position ever observed. This current transports southward 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0004.gif?v=1&amp;t=hi5l2oc9&amp;s=7b72f18288d89d3c92309554bc5c6582d8f2a844" class="inlineGraphic"/> Sv in the thermocline layers and 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0005.gif?v=1&amp;t=hi5l2oc9&amp;s=1d3c672323e9952715dd909d869f01b51d245bb0" class="inlineGraphic"/> Sv in the intermediate layers. This intermediate flow shows a relative maximum of oxygen and a relative minimum in nutrient concentration, indicating the presence of SAIW. The study concludes that, at least in fall 2009, the Canary Current extends to the intermediate waters (
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20227/asset/equation/jgrc20227-math-0006.gif?v=1&amp;t=hi5l2oca&amp;s=278ce5e9f0c2dd71192ab0589e88fef9df84fe52" class="inlineGraphic"/> approximately 1600 dbar) and that Azores Current feeds the Canary Current at surface and intermediate layers.</p></div>
]]></content:encoded><description>The source of the Canary Current has been inferred from an inverse box model applied to the hydrographic data of a survey carried out in 2009 in the northeast subtropical gyre (29–37°N, 9–24°W). The Portugal Current is observed between 13.5 and 14.8°W at 37°N carrying 
1.8±0.4 Sv southward. This current presumably merges with the eastward transport of the Azores Current System and partly contributes to the Mediterranean inflow and partly to the northward recirculation of the Azores Current through the Gulf of Cadiz. The Azores Current System is located in the meridional range 33.50–36.25°N at 24.50°W. This System transports eastward 
7.2±0.5 Sv in the thermocline layers and 
1.1±0.8 Sv at intermediate layers. The Azores Current intermediate water mass has the highest portion of Sub-Arctic intermediate water (SAIW) in the region, while the Azores Countercurrent intermediate waters mass is mainly Mediterranean water. The Canary Current extends from 22.25° to 18.50°W at 29°N, the westernmost position ever observed. This current transports southward 
−6.2±0.6 Sv in the thermocline layers and 
−2.0±0.8 Sv in the intermediate layers. This intermediate flow shows a relative maximum of oxygen and a relative minimum in nutrient concentration, indicating the presence of SAIW. The study concludes that, at least in fall 2009, the Canary Current extends to the intermediate waters (
γn≤27.9220 approximately 1600 dbar) and that Azores Current feeds the Canary Current at surface and intermediate layers.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20228" xmlns="http://purl.org/rss/1.0/"><title>Arctic-scale assessment of satellite passive microwave-derived snow depth on sea ice using Operation IceBridge airborne data</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20228</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Arctic-scale assessment of satellite passive microwave-derived snow depth on sea ice using Operation IceBridge airborne data</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ludovic Brucker, Thorsten Markus</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-11T15:35:24.39498-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20228</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20228</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20228</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Snow depth on sea ice (SD) is a key geophysical variable, knowledge of which is critical for calculating the energy and mass balance budgets. Moreover, accurate knowledge of the SD distribution is important to retrieve sea-ice thicknesses from altimetry data. So far, only space-based microwave radiometers (e.g., Advanced Microwave Scanning Radiometer for Earth Observing System; AMSR-E) provide operational SD on seasonal sea-ice retrievals. A thorough assessment of these retrievals is needed on a large scale and on a variety of sea-ice types. Our study presents such an assessment on Arctic sea ice using NASA's airborne Operation IceBridge (OIB) SDs, retrieved from radar measurements. Between 2009 and 2011, ∼610 12.5 km satellite grid cells were covered by seasonal sea ice where both satellite SD retrievals and OIB data were available. Using all the available data, the difference between the AMSR-E product and the averaged OIB snow-radar-derived SD is 0.00±0.07 m. Satellite-derived SD was accurate in the Beaufort Sea and the Canadian Archipelago but underestimated (∼0.07 m) in the Nares Strait. The RMSE between the two products ranges between 0.03 and 0.15 m. The RMSE is less than 0.06 m over a shallow snow cover (&lt;0.20 m), in areas where satellite-retrieved ice concentrations are higher than 90%, surface smooth, and ice thicker than ∼0.5 m. Locally the AMSR-E algorithm can significantly underestimate SD. Several regions where the retrievals were less accurate (error &gt;0.10 m) have been identified and related to the presence of either low ice concentration or significant fraction of multiyear ice within the grid cell that has not been flagged.</p></div>
]]></content:encoded><description>Snow depth on sea ice (SD) is a key geophysical variable, knowledge of which is critical for calculating the energy and mass balance budgets. Moreover, accurate knowledge of the SD distribution is important to retrieve sea-ice thicknesses from altimetry data. So far, only space-based microwave radiometers (e.g., Advanced Microwave Scanning Radiometer for Earth Observing System; AMSR-E) provide operational SD on seasonal sea-ice retrievals. A thorough assessment of these retrievals is needed on a large scale and on a variety of sea-ice types. Our study presents such an assessment on Arctic sea ice using NASA's airborne Operation IceBridge (OIB) SDs, retrieved from radar measurements. Between 2009 and 2011, ∼610 12.5 km satellite grid cells were covered by seasonal sea ice where both satellite SD retrievals and OIB data were available. Using all the available data, the difference between the AMSR-E product and the averaged OIB snow-radar-derived SD is 0.00±0.07 m. Satellite-derived SD was accurate in the Beaufort Sea and the Canadian Archipelago but underestimated (∼0.07 m) in the Nares Strait. The RMSE between the two products ranges between 0.03 and 0.15 m. The RMSE is less than 0.06 m over a shallow snow cover (&lt;0.20 m), in areas where satellite-retrieved ice concentrations are higher than 90%, surface smooth, and ice thicker than ∼0.5 m. Locally the AMSR-E algorithm can significantly underestimate SD. Several regions where the retrievals were less accurate (error &gt;0.10 m) have been identified and related to the presence of either low ice concentration or significant fraction of multiyear ice within the grid cell that has not been flagged.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20196" xmlns="http://purl.org/rss/1.0/"><title>Dynamical responses of the west Pacific North Equatorial Countercurrent (NECC) system to El Niño events</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20196</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Dynamical responses of the west Pacific North Equatorial Countercurrent (NECC) system to El Niño events</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jun Zhao, Yuanlong Li, Fan Wang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-11T15:15:24.768299-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20196</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20196</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20196</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Analysis of data sets based on satellite measurements during 1992–2011 reveals pronounced interannual-to-decadal variations of the west Pacific North Equatorial Countercurrent (NECC) system, involving the intensity (INT), position (<em>Y</em><sub>CM</sub>), and path length (<em>L</em><sub>CM</sub>) of the surface NECC jet, together with the associated recirculation gyres and mesoscale eddies. During the 1997–1998 and 2009–2010 El Niño events, the NECC jet showed increased INT before, and decreased INT, northerly position, and lengthened path after the mature phase. During the 1993–1995 and 2002–2005 central Pacific warming events, it also showed increased INT but no evident changes in <em>Y</em><sub>CM</sub> and <em>L</em><sub>CM</sub>. The varied responses caused the different natures of individual El Niño events. In 1998 and 2010, reflected upwelling Kelvin waves south of the NECC jet, together with the downwelling Rossby waves north of it induced by the following strong La Niña events, weakened the NECC jet through geostrophy and shifted it northward. This process was however absent during the 1993–1995 and 2002–2005 events. Intensified NECC jet during warm conditions gives rise to anomalously active mesoscale eddies, which also contribute to the unstable states of the NECC system in 1998 and 2010. Hindcast with a linear Rossby wave model reveals a slow change of the western Pacific NECC system during the past 50 years. Since 1990s, low-frequency variance of the NECC system has been dominated by quasi-decadal signals and more closely associated with wind forcing in the western Pacific Ocean, which corresponds to the slow changes of the El Niño/Southern Oscillation (ENSO)-related wind forcing pattern.</p></div>
]]></content:encoded><description>Analysis of data sets based on satellite measurements during 1992–2011 reveals pronounced interannual-to-decadal variations of the west Pacific North Equatorial Countercurrent (NECC) system, involving the intensity (INT), position (YCM), and path length (LCM) of the surface NECC jet, together with the associated recirculation gyres and mesoscale eddies. During the 1997–1998 and 2009–2010 El Niño events, the NECC jet showed increased INT before, and decreased INT, northerly position, and lengthened path after the mature phase. During the 1993–1995 and 2002–2005 central Pacific warming events, it also showed increased INT but no evident changes in YCM and LCM. The varied responses caused the different natures of individual El Niño events. In 1998 and 2010, reflected upwelling Kelvin waves south of the NECC jet, together with the downwelling Rossby waves north of it induced by the following strong La Niña events, weakened the NECC jet through geostrophy and shifted it northward. This process was however absent during the 1993–1995 and 2002–2005 events. Intensified NECC jet during warm conditions gives rise to anomalously active mesoscale eddies, which also contribute to the unstable states of the NECC system in 1998 and 2010. Hindcast with a linear Rossby wave model reveals a slow change of the western Pacific NECC system during the past 50 years. Since 1990s, low-frequency variance of the NECC system has been dominated by quasi-decadal signals and more closely associated with wind forcing in the western Pacific Ocean, which corresponds to the slow changes of the El Niño/Southern Oscillation (ENSO)-related wind forcing pattern.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20215" xmlns="http://purl.org/rss/1.0/"><title>Development of a variational data assimilation system for the diurnal cycle of sea surface temperature</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20215</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Development of a variational data assimilation system for the diurnal cycle of sea surface temperature</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J. While, M. Martin</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-11T08:51:24.57586-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20215</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20215</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20215</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A variational data assimilation system based on an incremental 4D-Var approach is proposed for use with a zero-dimensional model of the diurnal cycle of sea surface temperature (SST). Traditional 4D-Var, which seeks to find the initial state of a system, is not appropriate for diurnal SST which is a wind and heat flux driven system that has only a limited memory of its prior state. Instead the proposed assimilation system corrects both the initial SST and the heat and wind fluxes applied throughout the day. The assimilation system is tested using ensembles in a set of idealized twin experiments. In these tests controlling parameters are varied around reasonable “default” values with the quality of the analyses assessed against a known “truth”. Within our tests data assimilation is shown to improve diurnal SST under most circumstances. Analyzed heat fluxes are also sometimes improved, although the improvement is much less than that observed for diurnal SST. The system was not found to improve the wind stress. The only circumstances where diurnal SST was not found to be improved by the assimilation were where either observational errors were large (greater than 0.5 K in our tests), or biases in the observations were too big (less than −0.3 K or greater than 0.2 K). The non-Gaussian behavior of the wind stress was found to have an impact on the assimilation in low-wind conditions and under these conditions the best analyses were obtained by artificially inflating the observation error.</p></div>
]]></content:encoded><description>A variational data assimilation system based on an incremental 4D-Var approach is proposed for use with a zero-dimensional model of the diurnal cycle of sea surface temperature (SST). Traditional 4D-Var, which seeks to find the initial state of a system, is not appropriate for diurnal SST which is a wind and heat flux driven system that has only a limited memory of its prior state. Instead the proposed assimilation system corrects both the initial SST and the heat and wind fluxes applied throughout the day. The assimilation system is tested using ensembles in a set of idealized twin experiments. In these tests controlling parameters are varied around reasonable “default” values with the quality of the analyses assessed against a known “truth”. Within our tests data assimilation is shown to improve diurnal SST under most circumstances. Analyzed heat fluxes are also sometimes improved, although the improvement is much less than that observed for diurnal SST. The system was not found to improve the wind stress. The only circumstances where diurnal SST was not found to be improved by the assimilation were where either observational errors were large (greater than 0.5 K in our tests), or biases in the observations were too big (less than −0.3 K or greater than 0.2 K). The non-Gaussian behavior of the wind stress was found to have an impact on the assimilation in low-wind conditions and under these conditions the best analyses were obtained by artificially inflating the observation error.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20221" xmlns="http://purl.org/rss/1.0/"><title>Sea level rise and tidal power plants in the Gulf of Maine</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20221</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea level rise and tidal power plants in the Gulf of Maine</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Holly E. Pelling, J. A. Mattias Green</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-11T08:34:09.276873-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20221</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20221</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20221</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The response of the Bay of Fundy and Gulf of Maine to large-scale tidal power plants and future sea-level rise is investigated using an established numerical tidal model. Free stream tidal turbines were simulated within the Bay of Fundy by implementing an additional bed friction term, <em>K<sub>t</sub></em>. The present-day maximum tidal power output was determined to be 7.1 GW, and required <em>K<sub>t</sub></em> = 0.03. Extraction at this level would lead to large changes in the tidal amplitudes across the Gulf of Maine. With future SLR implemented, the energy available for extraction increases with 0.5–1 GW per m SLR. SLR simulations without tidal power extraction revealed that the response of the semidiurnal tides to SLR is highly dependent on how changes in sea level are implemented in the model. When extensive flood defenses are assumed at the present-day coast line, the response to SLR is far larger than when land is allowed to (permanently) flood. For example, within the Bay of Fundy itself, the M<sub>2</sub> amplitude increases with nearly 0.12 m per m SLR without flooding, but it changes with only 0.03 m per m SLR with flooding. We suggest that this is due to the flooding of land cells changing the resonant properties of the basin.</p></div>
]]></content:encoded><description>The response of the Bay of Fundy and Gulf of Maine to large-scale tidal power plants and future sea-level rise is investigated using an established numerical tidal model. Free stream tidal turbines were simulated within the Bay of Fundy by implementing an additional bed friction term, Kt. The present-day maximum tidal power output was determined to be 7.1 GW, and required Kt = 0.03. Extraction at this level would lead to large changes in the tidal amplitudes across the Gulf of Maine. With future SLR implemented, the energy available for extraction increases with 0.5–1 GW per m SLR. SLR simulations without tidal power extraction revealed that the response of the semidiurnal tides to SLR is highly dependent on how changes in sea level are implemented in the model. When extensive flood defenses are assumed at the present-day coast line, the response to SLR is far larger than when land is allowed to (permanently) flood. For example, within the Bay of Fundy itself, the M2 amplitude increases with nearly 0.12 m per m SLR without flooding, but it changes with only 0.03 m per m SLR with flooding. We suggest that this is due to the flooding of land cells changing the resonant properties of the basin.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20226" xmlns="http://purl.org/rss/1.0/"><title>Entrainment-driven modulation of Southern Ocean mixed layer properties and sea ice variability in CMIP5 models</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20226</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Entrainment-driven modulation of Southern Ocean mixed layer properties and sea ice variability in CMIP5 models</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sally E. Close, Hugues Goosse</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-10T16:41:30.728211-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20226</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20226</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20226</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The evolution of the upper Southern Ocean hydrographic structure in response to the representative concentration pathways 4.5 (RCP 4.5) forcing scenario is analyzed using model data drawn from the coupled model intercomparison project phase 5 (CMIP5) archive. A robust freshening trend is evident, associated with an increase in stratification and decoupling of the upper ocean as the mixed layer gains buoyancy at a faster rate than the underlying ocean. The magnitudes of the individual terms of the salinity and heat budgets are evaluated. Convection-driven entrainment from the thermocline into the mixed layer is found to play a significant role in modulating the mixed layer salinity, whilst the heat budget of the mixed layer is dominated by a primary balance between atmospheric warming and the entrainment-modulated supply of oceanic heat from below the mixed layer. The relationship between oceanic heat storage below the mixed layer, ice thickness and atmospheric temperature is investigated, and a very disparate response noted amongst the models considered here. Based on this analysis, we hypothesize that the balance between the entrainment-modulated supply of oceanic heat from below the mixed layer and the heat supplied by the atmosphere may play an important role in determining the simulated sea ice variability.</p></div>
]]></content:encoded><description>The evolution of the upper Southern Ocean hydrographic structure in response to the representative concentration pathways 4.5 (RCP 4.5) forcing scenario is analyzed using model data drawn from the coupled model intercomparison project phase 5 (CMIP5) archive. A robust freshening trend is evident, associated with an increase in stratification and decoupling of the upper ocean as the mixed layer gains buoyancy at a faster rate than the underlying ocean. The magnitudes of the individual terms of the salinity and heat budgets are evaluated. Convection-driven entrainment from the thermocline into the mixed layer is found to play a significant role in modulating the mixed layer salinity, whilst the heat budget of the mixed layer is dominated by a primary balance between atmospheric warming and the entrainment-modulated supply of oceanic heat from below the mixed layer. The relationship between oceanic heat storage below the mixed layer, ice thickness and atmospheric temperature is investigated, and a very disparate response noted amongst the models considered here. Based on this analysis, we hypothesize that the balance between the entrainment-modulated supply of oceanic heat from below the mixed layer and the heat supplied by the atmosphere may play an important role in determining the simulated sea ice variability.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20208" xmlns="http://purl.org/rss/1.0/"><title>Effects of solar penetration on the annual cycle of sea surface temperature in the North Pacific</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20208</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Effects of solar penetration on the annual cycle of sea surface temperature in the North Pacific</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Xi Liang, Lixin Wu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-10T11:39:45.865501-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20208</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20208</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20208</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The effects of solar penetration on the annual cycle of extratropical North Pacific sea surface temperature (SST) are investigated based on coupled ocean-atmosphere model simulations. It is found that the solar penetration can significantly improve the seasonal cycle of the North Pacific SST in the model. In summer, the solar penetration can partly reduce the SST warm bias in the model by diluting the shortwave radiation to the seasonal thermocline, while in winter, it can reduce the model SST cold bias through the entrainment of the warm thermocline water into the mixed layer. The solar penetration forces significant changes not only in the ocean but also in the atmosphere. The changes in the atmospheric circulation are characterized by a baroclinic structure with ridge/trough in the lower/upper troposphere in summer and an equivalent barotropic trough in winter. As a result, the annual mean of the oceanic subtropical gyre is intensified. Our study echoes the potential importance of the ecosystem in modulating the coupled ocean-atmosphere interaction over the extratropical oceans.</p></div>
]]></content:encoded><description>The effects of solar penetration on the annual cycle of extratropical North Pacific sea surface temperature (SST) are investigated based on coupled ocean-atmosphere model simulations. It is found that the solar penetration can significantly improve the seasonal cycle of the North Pacific SST in the model. In summer, the solar penetration can partly reduce the SST warm bias in the model by diluting the shortwave radiation to the seasonal thermocline, while in winter, it can reduce the model SST cold bias through the entrainment of the warm thermocline water into the mixed layer. The solar penetration forces significant changes not only in the ocean but also in the atmosphere. The changes in the atmospheric circulation are characterized by a baroclinic structure with ridge/trough in the lower/upper troposphere in summer and an equivalent barotropic trough in winter. As a result, the annual mean of the oceanic subtropical gyre is intensified. Our study echoes the potential importance of the ecosystem in modulating the coupled ocean-atmosphere interaction over the extratropical oceans.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20219" xmlns="http://purl.org/rss/1.0/"><title>Instability of some equatorially trapped waves</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20219</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Instability of some equatorially trapped waves</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Adrian Constantin, Pierre Germain</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-10T11:15:46.004496-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20219</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20219</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20219</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A high-frequency asymptotics approach within the Lagrangian framework shows that some exact equatorially trapped three-dimensional waves are linearly unstable when their steepness exceeds a specific threshold.</p></div>
]]></content:encoded><description>A high-frequency asymptotics approach within the Lagrangian framework shows that some exact equatorially trapped three-dimensional waves are linearly unstable when their steepness exceeds a specific threshold.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20217" xmlns="http://purl.org/rss/1.0/"><title>Rates and mechanisms of turbulent dissipation and mixing in the Southern Ocean: Results from the Diapycnal and Isopycnal Mixing Experiment in the Southern Ocean (DIMES)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20217</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Rates and mechanisms of turbulent dissipation and mixing in the Southern Ocean: Results from the Diapycnal and Isopycnal Mixing Experiment in the Southern Ocean (DIMES)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">K. L. Sheen, J. A. Brearley, A. C. Naveira Garabato, D. A. Smeed, S. Waterman, J. R. Ledwell, M. P. Meredith, L. St. Laurent, A. M. Thurnherr, J. M. Toole, A. J. Watson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T15:46:48.351786-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20217</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20217</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20217</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The spatial distribution of turbulent dissipation rates and internal wavefield characteristics is analyzed across two contrasting regimes of the Antarctic Circumpolar Current (ACC), using microstructure and finestructure data collected as part of the Diapycnal and Isopycnal Mixing Experiment in the Southern Ocean (DIMES). Mid-depth turbulent dissipation rates are found to increase from 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20217/asset/equation/jgrc20217-math-0001.gif?v=1&amp;t=hi5l2odt&amp;s=78c00cc8a333ce77b49370e48111a16aaf9a3fd4" class="inlineGraphic"/> in the Southeast Pacific to 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20217/asset/equation/jgrc20217-math-0002.gif?v=1&amp;t=hi5l2odu&amp;s=e7cd5dac390e2a01f2707091114001ec3175a805" class="inlineGraphic"/> in the Scotia Sea, typically reaching 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20217/asset/equation/jgrc20217-math-0003.gif?v=1&amp;t=hi5l2odu&amp;s=8e330da6fbb184a00c08b12430436ac3eab200ec" class="inlineGraphic"/> within a kilometer of the seabed. Enhanced levels of turbulent mixing are associated with strong near-bottom flows, rough topography, and regions where the internal wavefield is found to have enhanced energy, a less-inertial frequency content and a dominance of upward propagating energy. These results strongly suggest that bottom-generated internal waves play a major role in determining the spatial distribution of turbulent dissipation in the ACC. The energy flux associated with the bottom internal wave generation process is calculated using wave radiation theory, and found to vary between 0.8 mW m<sup>−2</sup> in the Southeast Pacific and 14 mW m<sup>−2</sup> in the Scotia Sea. Typically, 10%–30% of this energy is found to dissipate within 1 km of the seabed. Comparison between turbulent dissipation rates inferred from finestructure parameterizations and microstructure-derived estimates suggests a significant departure from wave-wave interaction physics in the near-field of wave generation sites.</p></div>
]]></content:encoded><description>The spatial distribution of turbulent dissipation rates and internal wavefield characteristics is analyzed across two contrasting regimes of the Antarctic Circumpolar Current (ACC), using microstructure and finestructure data collected as part of the Diapycnal and Isopycnal Mixing Experiment in the Southern Ocean (DIMES). Mid-depth turbulent dissipation rates are found to increase from 
O(1×10−10Wkg −1) in the Southeast Pacific to 
O(1×10−9Wkg −1) in the Scotia Sea, typically reaching 
3×10−9Wkg −1 within a kilometer of the seabed. Enhanced levels of turbulent mixing are associated with strong near-bottom flows, rough topography, and regions where the internal wavefield is found to have enhanced energy, a less-inertial frequency content and a dominance of upward propagating energy. These results strongly suggest that bottom-generated internal waves play a major role in determining the spatial distribution of turbulent dissipation in the ACC. The energy flux associated with the bottom internal wave generation process is calculated using wave radiation theory, and found to vary between 0.8 mW m−2 in the Southeast Pacific and 14 mW m−2 in the Scotia Sea. Typically, 10%–30% of this energy is found to dissipate within 1 km of the seabed. Comparison between turbulent dissipation rates inferred from finestructure parameterizations and microstructure-derived estimates suggests a significant departure from wave-wave interaction physics in the near-field of wave generation sites.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20198" xmlns="http://purl.org/rss/1.0/"><title>Reduction of near-inertial energy through the dependence of wind stress on the ocean-surface velocity</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20198</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Reduction of near-inertial energy through the dependence of wind stress on the ocean-surface velocity</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Willi Rath, Richard J. Greatbatch, Xiaoming Zhai</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-06-04T10:38:21.848584-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20198</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20198</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20198</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A realistic primitive-equation model of the Southern Ocean at eddying spatial resolution is used to examine the effect of ocean-surface-velocity dependence of the wind stress on the strength of near-inertial oscillations. Accounting for the ocean-surface-velocity dependence of the wind stress leads to a large reduction of wind-induced near-inertial energy of approximately 40% and of wind power input into the near-inertial frequency band of approximately 20%. A large part of this reduction can be explained by the leading-order modification to the wind stress if the ocean-surface velocity is included. The strength of the reduction is shown to be modulated by the inverse of the ocean-surface-mixed-layer depth. We conclude that the effect of surface-velocity dependence of the wind stress should be taken into account when estimating the wind-power input into the near-inertial frequency band and when estimating near-inertial energy levels in the ocean due to wind forcing.</p></div>
]]></content:encoded><description>A realistic primitive-equation model of the Southern Ocean at eddying spatial resolution is used to examine the effect of ocean-surface-velocity dependence of the wind stress on the strength of near-inertial oscillations. Accounting for the ocean-surface-velocity dependence of the wind stress leads to a large reduction of wind-induced near-inertial energy of approximately 40% and of wind power input into the near-inertial frequency band of approximately 20%. A large part of this reduction can be explained by the leading-order modification to the wind stress if the ocean-surface velocity is included. The strength of the reduction is shown to be modulated by the inverse of the ocean-surface-mixed-layer depth. We conclude that the effect of surface-velocity dependence of the wind stress should be taken into account when estimating the wind-power input into the near-inertial frequency band and when estimating near-inertial energy levels in the ocean due to wind forcing.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20211" xmlns="http://purl.org/rss/1.0/"><title>Lateral diffusivity from tracer release experiments in the tropical North Atlantic thermocline</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20211</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Lateral diffusivity from tracer release experiments in the tropical North Atlantic thermocline</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Donata Banyte, Martin Visbeck, Toste Tanhua, Tim Fischer, Gerd Krahmann, Johannes Karstensen</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T22:49:18.318027-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20211</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20211</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20211</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Lateral diffusivity is computed from a tracer release experiment in the northeastern tropical Atlantic thermocline. The uncertainties of the estimates are inferred from a synthetic particle release using a high-resolution ocean circulation model. The main method employed to compute zonal and meridional components of lateral diffusivity is the growth of the second moment of a cloud of tracer. The application of an areal comparison method for estimating tracer-based diffusivity in the field experiments is also discussed. The best estimate of meridional eddy diffusivity in the Guinea Upwelling region at about 300 m depth is estimated to be 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20211/asset/equation/jgrc20211-math-0001.gif?v=1&amp;t=hi5l2oe6&amp;s=9a70df81c431f998274560728d00d6c710d5cc1e" class="inlineGraphic"/> m<sup>2</sup> s<sup>−1</sup>. The zonal component of lateral diffusivity is estimated to be 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20211/asset/equation/jgrc20211-math-0002.gif?v=1&amp;t=hi5l2oe7&amp;s=19fc9f27546351fdeda5d380e585c376c8790c49" class="inlineGraphic"/> m<sup>2</sup> s<sup>−1</sup>, while areal comparison method yields areal equivalent zonal diffusivity component of 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20211/asset/equation/jgrc20211-math-0003.gif?v=1&amp;t=hi5l2oe7&amp;s=c15475fe92634ddedbe1cdfb579106f17f022b78" class="inlineGraphic"/> m<sup>2</sup> s<sup>−1</sup>. In comparison to <em>K<sub>y</sub></em>, <em>K<sub>x</sub></em> is about twice larger, resulting from the tracer patch stretching by zonal jets. Employed conceptual jet model indicates that zonal jet velocities of about 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20211/asset/equation/jgrc20211-math-0004.gif?v=1&amp;t=hi5l2oe8&amp;s=b3b2e9fd2287f62566b3a5cef2525c90d5255aff" class="inlineGraphic"/> m s<sup>−1</sup> are required to explain the enhancement of the zonal eddy diffusivity component. Finally, different sampling strategies are tested on synthetic tracer release experiments. They indicate that the best sampling strategy is a sparse regular sampling grid covering most of the tracer patch.</p></div>
]]></content:encoded><description>Lateral diffusivity is computed from a tracer release experiment in the northeastern tropical Atlantic thermocline. The uncertainties of the estimates are inferred from a synthetic particle release using a high-resolution ocean circulation model. The main method employed to compute zonal and meridional components of lateral diffusivity is the growth of the second moment of a cloud of tracer. The application of an areal comparison method for estimating tracer-based diffusivity in the field experiments is also discussed. The best estimate of meridional eddy diffusivity in the Guinea Upwelling region at about 300 m depth is estimated to be 
Ky=500 ± 200 m2 s−1. The zonal component of lateral diffusivity is estimated to be 
Kx=1200 ± 600 m2 s−1, while areal comparison method yields areal equivalent zonal diffusivity component of 
Kxe=1000 ± 500 m2 s−1. In comparison to Ky, Kx is about twice larger, resulting from the tracer patch stretching by zonal jets. Employed conceptual jet model indicates that zonal jet velocities of about 
0.015 ± 0.005 m s−1 are required to explain the enhancement of the zonal eddy diffusivity component. Finally, different sampling strategies are tested on synthetic tracer release experiments. They indicate that the best sampling strategy is a sparse regular sampling grid covering most of the tracer patch.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20209" xmlns="http://purl.org/rss/1.0/"><title>A numerical investigation of the dynamics and structure of hyperpycnal river plumes on sloping continental shelves</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20209</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A numerical investigation of the dynamics and structure of hyperpycnal river plumes on sloping continental shelves</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Shih-Nan Chen, W. Rockwell Geyer, Tian-Jian Hsu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T15:30:54.57897-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20209</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20209</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20209</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A 3-D hydrodynamic model (Regional Ocean Modeling System) is used to investigate the dynamics and structure of hyperpycnal river plumes over sloping continental shelves. The focus is on the plume's response to varying slopes and settling velocities (<em>w<sub>s</sub></em>). The idealized model is configured to represent small mountainous river systems during a flood event. A hyperpycnal sediment concentration of 60 g/L is specified at the river mouth such that the sediment–freshwater mixture is denser than the seawater, causing the plumes to traverse the shelves as undercurrents. A realistic range of shelf slope of 0.001–0.03 is chosen. The settling velocity is varied based on river's carrying capacity. The model-derived velocity profiles and the entrainment rate compare favorably against prior laboratory experiments. Both cross-shore and alongshore momentum balances are primarily between gravitational forcing and bottom friction. But, the Coriolis deflection is significant at the plume core in the alongshore momentum budget (i.e., Ekman balance). As the slope increases and settling velocity decreases, hyperpycnal plumes transition from depositional to autosuspending regime. An estimate of critical slope governed by a dimensionless parameter 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20209/asset/equation/jgrc20209-math-0001.gif?v=1&amp;t=hi5l2oef&amp;s=03966f5829dea2443a574742a00013c2c3ae31bd" class="inlineGraphic"/> (<em>q<sub>b</sub></em> is buoyancy input) reasonably captures the regime transition. In the depositional regime, the plume's runout (cross-shore penetration) scales with advective distance: increasing slopes and discharge enhance the gravitational forcing and plume velocity, leading to an increase in runout. In contrast, increasing settling velocity shortens the vertical settling time, thereby reducing the plume's horizontal footprint. For the range of parameters considered, the runout of depositional plumes is confined within 15 km from the mouth, whereas the penetration of autosuspending plumes is essentially unlimited.</p></div>
]]></content:encoded><description>A 3-D hydrodynamic model (Regional Ocean Modeling System) is used to investigate the dynamics and structure of hyperpycnal river plumes over sloping continental shelves. The focus is on the plume's response to varying slopes and settling velocities (ws). The idealized model is configured to represent small mountainous river systems during a flood event. A hyperpycnal sediment concentration of 60 g/L is specified at the river mouth such that the sediment–freshwater mixture is denser than the seawater, causing the plumes to traverse the shelves as undercurrents. A realistic range of shelf slope of 0.001–0.03 is chosen. The settling velocity is varied based on river's carrying capacity. The model-derived velocity profiles and the entrainment rate compare favorably against prior laboratory experiments. Both cross-shore and alongshore momentum balances are primarily between gravitational forcing and bottom friction. But, the Coriolis deflection is significant at the plume core in the alongshore momentum budget (i.e., Ekman balance). As the slope increases and settling velocity decreases, hyperpycnal plumes transition from depositional to autosuspending regime. An estimate of critical slope governed by a dimensionless parameter 
ws3/qb (qb is buoyancy input) reasonably captures the regime transition. In the depositional regime, the plume's runout (cross-shore penetration) scales with advective distance: increasing slopes and discharge enhance the gravitational forcing and plume velocity, leading to an increase in runout. In contrast, increasing settling velocity shortens the vertical settling time, thereby reducing the plume's horizontal footprint. For the range of parameters considered, the runout of depositional plumes is confined within 15 km from the mouth, whereas the penetration of autosuspending plumes is essentially unlimited.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20203" xmlns="http://purl.org/rss/1.0/"><title>Numerical simulations of oceanic pCO2 variations and interactions between Typhoon Choi-wan (0914) and the ocean</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20203</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Numerical simulations of oceanic pCO2 variations and interactions between Typhoon Choi-wan (0914) and the ocean</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Akiyoshi Wada, Meghan F. Cronin, Adrienne J. Sutton, Yoshimi Kawai, Masao Ishii</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T14:42:10.057839-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20203</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20203</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20203</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> On 19 September 2009, Typhoon Choi-wan passed ∼40 km to the southeast of the Kuroshio Extension Observatory (KEO) surface mooring, located at 32.3°N, 144.5°E. We use an atmosphere-wave-ocean coupled model that incorporated an oceanic carbon equilibrium model to investigate the typhoon-induced CO<sub>2</sub> outgassing observed by the KEO mooring. KEO data are used to provide atmospheric surface boundary conditions for partial pressure of CO<sub>2</sub> (
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0004.gif?v=1&amp;t=hi5l2oem&amp;s=9e376a6ec51bd9473121e3e7ccb6c3b391c7d6ba" class="inlineGraphic"/>) and to validate the numerical results. The model simulated the observed sea-level pressure variations reasonably well, although the simulated-typhoon translation was 3 h slower than the estimated best track. The simulation resulted in lower than observed sea-surface temperature (SST), sea-surface salinity (SSS), and partial pressure of surface ocean CO<sub>2</sub> (
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0005.gif?v=1&amp;t=hi5l2oen&amp;s=8528577465b27fb0b4cc24629407b3e8b2dba6e4" class="inlineGraphic"/>). Better agreement was found with the grid point south of the buoy that corresponded roughly to the buoy location in the simulated-typhoon reference frame. In situ observations show CO<sub>2</sub> outgassing during the Choi-wan's passage. Forty percent of observed outgassing was explained by decreasing 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0006.gif?v=1&amp;t=hi5l2oeo&amp;s=051e76df3ca0db491585e80273b318f3eea0141b" class="inlineGraphic"/> (∼20 µatm), and thus, the remainder (∼30 µatm) must be explained by increasing 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0007.gif?v=1&amp;t=hi5l2oeo&amp;s=b320b39235e1e8f8b1656b7cb425cbb4958e72da" class="inlineGraphic"/>. The model simulated only one third of the increase in observed surface 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0008.gif?v=1&amp;t=hi5l2oeo&amp;s=6d50392dfdd4645ac7b9b1321dbe8fbc7e990a18" class="inlineGraphic"/> variation (∼9.6 µatm), suggesting that not only SST but also high salinity and dissolved inorganic carbon caused by vertical turbulent mixing and horizontal advection are important in simulating surface 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0009.gif?v=1&amp;t=hi5l2oep&amp;s=dbaa8800a2768ddb6ac1fa1ff4c76e2faf80a2a6" class="inlineGraphic"/> variation. The simulations also reveal that surface roughness length affects surface wind asymmetry during the passage and variation in SSS and 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20203/asset/equation/jgrc20203-math-0010.gif?v=1&amp;t=hi5l2oeq&amp;s=075a2060d0de57f848f131deb4fc0f74c64115aa" class="inlineGraphic"/> (∼1 µatm) after the passage.</p></div>
]]></content:encoded><description>On 19 September 2009, Typhoon Choi-wan passed ∼40 km to the southeast of the Kuroshio Extension Observatory (KEO) surface mooring, located at 32.3°N, 144.5°E. We use an atmosphere-wave-ocean coupled model that incorporated an oceanic carbon equilibrium model to investigate the typhoon-induced CO2 outgassing observed by the KEO mooring. KEO data are used to provide atmospheric surface boundary conditions for partial pressure of CO2 (
pCO2air ) and to validate the numerical results. The model simulated the observed sea-level pressure variations reasonably well, although the simulated-typhoon translation was 3 h slower than the estimated best track. The simulation resulted in lower than observed sea-surface temperature (SST), sea-surface salinity (SSS), and partial pressure of surface ocean CO2 (
pCO2sea ). Better agreement was found with the grid point south of the buoy that corresponded roughly to the buoy location in the simulated-typhoon reference frame. In situ observations show CO2 outgassing during the Choi-wan's passage. Forty percent of observed outgassing was explained by decreasing 
pCO2air  (∼20 µatm), and thus, the remainder (∼30 µatm) must be explained by increasing 
pCO2sea . The model simulated only one third of the increase in observed surface 
pCO2sea  variation (∼9.6 µatm), suggesting that not only SST but also high salinity and dissolved inorganic carbon caused by vertical turbulent mixing and horizontal advection are important in simulating surface 
pCO2sea  variation. The simulations also reveal that surface roughness length affects surface wind asymmetry during the passage and variation in SSS and 
pCO2sea  (∼1 µatm) after the passage.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20214" xmlns="http://purl.org/rss/1.0/"><title>Traditional quasi-geostrophic modes and surface quasi-geostrophic solutions in the Southwestern Atlantic</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20214</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Traditional quasi-geostrophic modes and surface quasi-geostrophic solutions in the Southwestern Atlantic</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Cesar B. Rocha, Amit Tandon, Ilson C. A. Silveira, Jose Antonio M. Lima</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T13:40:32.376248-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20214</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20214</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20214</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We investigate whether the Quasi-geostrophic (QG) modes and the Surface Quasi-geostrophic (SQG) solutions are consistent with the vertical structure of the subinertial variability off southeast Brazil. The first-order empirical orthogonal function (EOF) of current meter time series is reconstructed using different QG mode combinations; the first EOF is compared against SQG solutions. At two out of three moorings, the traditional flat-bottom barotropic (BT) and first baroclinic (BC1) mode combination fails to represent the observed sharp near-surface decay, although this combination contains up to 78% of the depth-integrated variance. A mesoscale broad-band combination of flat-bottom SQG solutions is consistent with the near-surface sharp decay, accounting for up to 85% of the first EOF variance. A higher-order QG mode combination is also consistent with the data. Similar results are obtained for a rough topography scenario, in which the velocity vanishes at the bottom. The projection of the SQG solutions onto the QG modes confirms that these two models are mutually dependent. Consequently, as far as the observed near-surface vertical structure is concerned, SQG solutions and four-QG mode combination are indistinguishable. Tentative explanations for such vertical structures are given in terms of necessary conditions for baroclinic instability. “Charney-like” instabilities, or, surface-intensified “Phillips-like” instabilities may explain the SQG-like solutions at two moorings; traditional “Phillips-like” instabilities may rationalize the BT/BC1 mode representation at the third mooring. These results point out to the presence of a richer subinertial near-surface dynamics in some regions, which should be considered for the interpretation and projection of remotely sensed surface fields to depth.</p></div>
]]></content:encoded><description>We investigate whether the Quasi-geostrophic (QG) modes and the Surface Quasi-geostrophic (SQG) solutions are consistent with the vertical structure of the subinertial variability off southeast Brazil. The first-order empirical orthogonal function (EOF) of current meter time series is reconstructed using different QG mode combinations; the first EOF is compared against SQG solutions. At two out of three moorings, the traditional flat-bottom barotropic (BT) and first baroclinic (BC1) mode combination fails to represent the observed sharp near-surface decay, although this combination contains up to 78% of the depth-integrated variance. A mesoscale broad-band combination of flat-bottom SQG solutions is consistent with the near-surface sharp decay, accounting for up to 85% of the first EOF variance. A higher-order QG mode combination is also consistent with the data. Similar results are obtained for a rough topography scenario, in which the velocity vanishes at the bottom. The projection of the SQG solutions onto the QG modes confirms that these two models are mutually dependent. Consequently, as far as the observed near-surface vertical structure is concerned, SQG solutions and four-QG mode combination are indistinguishable. Tentative explanations for such vertical structures are given in terms of necessary conditions for baroclinic instability. “Charney-like” instabilities, or, surface-intensified “Phillips-like” instabilities may explain the SQG-like solutions at two moorings; traditional “Phillips-like” instabilities may rationalize the BT/BC1 mode representation at the third mooring. These results point out to the presence of a richer subinertial near-surface dynamics in some regions, which should be considered for the interpretation and projection of remotely sensed surface fields to depth.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20207" xmlns="http://purl.org/rss/1.0/"><title>Impact of current-wave interaction on storm surge simulation: A case study for Hurricane Bob</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20207</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Impact of current-wave interaction on storm surge simulation: A case study for Hurricane Bob</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Yunfang Sun, Changsheng Chen, Robert C. Beardsley, Qichun Xu, Jianhua Qi, Huichan Lin</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T11:40:38.899356-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20207</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20207</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20207</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Hurricane Bob moved up the U.S. east coast and crossed over southern New England and the Gulf of Maine [with peak marine winds up to 54 m/s (100 mph)] on 19–20 August 1991, causing significant damage along the coast and shelf. A 3-D fully wave-current-coupled finite-volume community ocean model system was developed and applied to simulate and examine the coastal ocean responses to Hurricane Bob. Results from process study-oriented experiments showed that the impact of wave-current interaction on surge elevation varied in space and time, more significant over the shelf than inside the inner bays. While sea level change along the coast was mainly driven by the water flux controlled by barotropic dynamics and the vertically integrated highest water transports were essentially the same for cases with and without water stratification, the hurricane-induced wave-current interaction could generate strong vertical current shear in the stratified areas, leading to a strong offshore transport near the bottom and vertical turbulent mixing over the continental shelf. Stratification could also result in a significant difference of water currents around islands where the water is not vertically well mixed.</p></div>
]]></content:encoded><description>Hurricane Bob moved up the U.S. east coast and crossed over southern New England and the Gulf of Maine [with peak marine winds up to 54 m/s (100 mph)] on 19–20 August 1991, causing significant damage along the coast and shelf. A 3-D fully wave-current-coupled finite-volume community ocean model system was developed and applied to simulate and examine the coastal ocean responses to Hurricane Bob. Results from process study-oriented experiments showed that the impact of wave-current interaction on surge elevation varied in space and time, more significant over the shelf than inside the inner bays. While sea level change along the coast was mainly driven by the water flux controlled by barotropic dynamics and the vertically integrated highest water transports were essentially the same for cases with and without water stratification, the hurricane-induced wave-current interaction could generate strong vertical current shear in the stratified areas, leading to a strong offshore transport near the bottom and vertical turbulent mixing over the continental shelf. Stratification could also result in a significant difference of water currents around islands where the water is not vertically well mixed.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20213" xmlns="http://purl.org/rss/1.0/"><title>Particle filter-based data assimilation for a three-dimensional biological ocean model and satellite observations</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20213</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Particle filter-based data assimilation for a three-dimensional biological ocean model and satellite observations</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jann Paul Mattern, Michael Dowd, Katja Fennel</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T11:07:33.38795-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20213</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20213</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20213</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We assimilate satellite observations of surface chlorophyll into a three-dimensional biological ocean model in order to improve its state estimates using a particle filter referred to as sequential importance resampling (SIR). Particle Filters represent an alternative to other, more commonly used ensemble-based state estimation techniques like the ensemble Kalman filter (EnKF). Unlike the EnKF, Particle Filters do not require normality assumptions about the model error structure and are thus suitable for highly nonlinear applications. However, their application in oceanographic contexts is typically hampered by the high dimensionality of the model's state space. We apply SIR to a high-dimensional model with a small ensemble size (20) and modify the standard SIR procedure to avoid complications posed by the high dimensionality of the model state. Two extensions to the SIR include a simple smoother to deal with outliers in the observations, and state-augmentation which provides the SIR with parameter memory. Our goal is to test the feasibility of biological state estimation with SIR for realistic models. For this purpose we compare the SIR results to a model simulation with optimal parameters with respect to the same set of observations. By running replicates of our main experiments, we assess the robustness of our SIR implementation. We show that SIR is suitable for satellite data assimilation into biological models and that both extensions, the smoother and state-augmentation, are required for robust results and improved fit to the observations.</p></div>
]]></content:encoded><description>We assimilate satellite observations of surface chlorophyll into a three-dimensional biological ocean model in order to improve its state estimates using a particle filter referred to as sequential importance resampling (SIR). Particle Filters represent an alternative to other, more commonly used ensemble-based state estimation techniques like the ensemble Kalman filter (EnKF). Unlike the EnKF, Particle Filters do not require normality assumptions about the model error structure and are thus suitable for highly nonlinear applications. However, their application in oceanographic contexts is typically hampered by the high dimensionality of the model's state space. We apply SIR to a high-dimensional model with a small ensemble size (20) and modify the standard SIR procedure to avoid complications posed by the high dimensionality of the model state. Two extensions to the SIR include a simple smoother to deal with outliers in the observations, and state-augmentation which provides the SIR with parameter memory. Our goal is to test the feasibility of biological state estimation with SIR for realistic models. For this purpose we compare the SIR results to a model simulation with optimal parameters with respect to the same set of observations. By running replicates of our main experiments, we assess the robustness of our SIR implementation. We show that SIR is suitable for satellite data assimilation into biological models and that both extensions, the smoother and state-augmentation, are required for robust results and improved fit to the observations.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20193" xmlns="http://purl.org/rss/1.0/"><title>Cold core eddies and fronts of the Antarctic Circumpolar Current south of New Zealand from in situ and satellite data</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20193</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Cold core eddies and fronts of the Antarctic Circumpolar Current south of New Zealand from in situ and satellite data</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Yuri Cotroneo, Giorgio Budillon, Giannetta Fusco, Giancarlo Spezie</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T10:38:33.368662-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20193</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20193</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20193</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The meridional heat flux required to balance the heat lost by ocean to atmosphere at high latitudes must be accomplished by some mechanism other than mean advection and the heat flux by eddies crossing the Antarctic Circumpolar Current (ACC) may be a candidate. In this study, the positions of the main ACC fronts are determined based on 23 expendable bathythermographs (XBT) transects collected from 1994 to 2010 and are compared with those detected through satellite altimetry. Then, cold core anomalies in XBT sections are identified and altimetry is used to follow the spatial-temporal evolution of these cold, low sea level anomalies. Mean values of main parameters, such as speed (0.35 km/h), lifetime (79 weeks), and diameter (105 km), are estimated. Moreover, estimations of rotational speed (0.9–76.8 cm/s), ocean surface layer heat content along temperature sections and eddy available heat anomaly (mean value −9.74 × 10<sup>9</sup> Jm<sup>−2</sup>) give a wider description of the detected eddies. In our study area, the spawning of eddies is found to occur downstream of the Southeast Indian Ridge and in correspondence of the polar front (PF) with regard to the ACC frontal structure. The contribution of eddies to the global heat budget is not only linked to their ability to cross the ACC fronts but also to the capacity of keeping partially unaltered the properties of water inside them. Analysis of the relation between the translation and rotational speeds shows that a typical eddy may effectively be a significant part (0.8%) of the net meridional heat transport across the PF with a mean heat content/anomaly of −7.65 × 10<sup>19</sup> J.</p></div>
]]></content:encoded><description>The meridional heat flux required to balance the heat lost by ocean to atmosphere at high latitudes must be accomplished by some mechanism other than mean advection and the heat flux by eddies crossing the Antarctic Circumpolar Current (ACC) may be a candidate. In this study, the positions of the main ACC fronts are determined based on 23 expendable bathythermographs (XBT) transects collected from 1994 to 2010 and are compared with those detected through satellite altimetry. Then, cold core anomalies in XBT sections are identified and altimetry is used to follow the spatial-temporal evolution of these cold, low sea level anomalies. Mean values of main parameters, such as speed (0.35 km/h), lifetime (79 weeks), and diameter (105 km), are estimated. Moreover, estimations of rotational speed (0.9–76.8 cm/s), ocean surface layer heat content along temperature sections and eddy available heat anomaly (mean value −9.74 × 109 Jm−2) give a wider description of the detected eddies. In our study area, the spawning of eddies is found to occur downstream of the Southeast Indian Ridge and in correspondence of the polar front (PF) with regard to the ACC frontal structure. The contribution of eddies to the global heat budget is not only linked to their ability to cross the ACC fronts but also to the capacity of keeping partially unaltered the properties of water inside them. Analysis of the relation between the translation and rotational speeds shows that a typical eddy may effectively be a significant part (0.8%) of the net meridional heat transport across the PF with a mean heat content/anomaly of −7.65 × 1019 J.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20133" xmlns="http://purl.org/rss/1.0/"><title>Simulated heat flux and sea ice production at coastal polynyas in the southwestern Weddell Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20133</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Simulated heat flux and sea ice production at coastal polynyas in the southwestern Weddell Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">V. Haid, R. Timmermann</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-30T08:53:06.999527-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20133</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20133</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20133</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20133-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Coastal polynyas are areas in an ice-covered ocean where the ice cover is exported, mostly by off-shore winds. The resulting reduction of sea ice enables an enhanced ocean-atmosphere heat transfer. Once the water temperatures are at the freezing point, further heat loss induces sea ice production. The heat exchange and ice production in coastal polynyas in the southwestern Weddell Sea is addressed using the Finite-Element Sea-ice Ocean Model, a primitive-equation, hydrostatic ocean circulation model coupled with a dynamic-thermodynamic sea-ice model, which allows to quantify the amount of heat associated with cooling of the water column. Three important polynya regions are identified: at Brunt Ice Shelf, at Ronne Ice Shelf and along the southern part of the Antarctic Peninsula. Multiyear winter means (May–September 1990–2009) give an upward heat flux to the atmosphere of 311 W/m<sup>2</sup> in the Brunt polynyas, 511 W/m<sup>2</sup> in Ronne Polynya and 364 W/m<sup>2</sup> in the Antarctic Peninsula polynyas, whereof 57 W/m<sup>2</sup>, 49 W/m<sup>2</sup> and 48 W/m<sup>2</sup>, respectively, are supplied as oceanic heat flux from deeper layers. The mean winter sea ice production is 7.2 cm/d in the Brunt polynyas corresponding to an ice volume of 1.3 ×10<sup>10</sup> m<sup>3</sup>/winter, 13.2 cm/d at Ronne polynya (4.4 ×10<sup>10</sup> m<sup>3</sup>/winter), and 9.2 cm/d in the Antarctic Peninsula polynyas (2.1 ×10<sup>10</sup> m<sup>3</sup>/winter). The heat flux to the atmosphere inside polynyas is 7 to 9 times higher than the heat flux in the adjacent area; polynya ice production per unit area exceeds adjacent values by a factor of 9 to 14.</p></div>]]></content:encoded><description>Coastal polynyas are areas in an ice-covered ocean where the ice cover is exported, mostly by off-shore winds. The resulting reduction of sea ice enables an enhanced ocean-atmosphere heat transfer. Once the water temperatures are at the freezing point, further heat loss induces sea ice production. The heat exchange and ice production in coastal polynyas in the southwestern Weddell Sea is addressed using the Finite-Element Sea-ice Ocean Model, a primitive-equation, hydrostatic ocean circulation model coupled with a dynamic-thermodynamic sea-ice model, which allows to quantify the amount of heat associated with cooling of the water column. Three important polynya regions are identified: at Brunt Ice Shelf, at Ronne Ice Shelf and along the southern part of the Antarctic Peninsula. Multiyear winter means (May–September 1990–2009) give an upward heat flux to the atmosphere of 311 W/m2 in the Brunt polynyas, 511 W/m2 in Ronne Polynya and 364 W/m2 in the Antarctic Peninsula polynyas, whereof 57 W/m2, 49 W/m2 and 48 W/m2, respectively, are supplied as oceanic heat flux from deeper layers. The mean winter sea ice production is 7.2 cm/d in the Brunt polynyas corresponding to an ice volume of 1.3 ×1010 m3/winter, 13.2 cm/d at Ronne polynya (4.4 ×1010 m3/winter), and 9.2 cm/d in the Antarctic Peninsula polynyas (2.1 ×1010 m3/winter). The heat flux to the atmosphere inside polynyas is 7 to 9 times higher than the heat flux in the adjacent area; polynya ice production per unit area exceeds adjacent values by a factor of 9 to 14.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20189" xmlns="http://purl.org/rss/1.0/"><title>Role of asymmetric tidal mixing in the subtidal dynamics of narrow estuaries</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20189</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Role of asymmetric tidal mixing in the subtidal dynamics of narrow estuaries</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Peng Cheng, Huib E. Swart, Arnoldo Valle-Levinson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-29T08:44:17.185368-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20189</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20189</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20189</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The role of asymmetric tidal mixing (ATM) in subtidal estuarine dynamics is investigated using a series of generic numerical experiments that simulate narrow estuaries under different stratification and external forcing conditions. The focus is on quantifying the characteristics of ATM-induced flow and its contributions to stratification and salt transport. The flow induced by ATM has a two-layer vertical structure in periodically stratified estuaries, similar to that of the density-driven flow. It has a three-layer vertical structure in the central regime of weakly stratified estuaries, and a reverse two-layer structure in highly stratified estuaries. The changes in vertical distribution of ATM-induced flows result from the influence of stratification on the covariance of eddy viscosity and vertical shear. Such covariance represents the driving force of ATM-induced flow in the tidally averaged momentum equation. Compared to density-driven flow, ATM-induced flow dominates in periodically stratified estuaries with strong tides, has the same order of magnitude in weakly stratified estuaries with moderate tides, and is less important in highly stratified estuaries with weak tides. In contrast to density-driven flow that always increases estuarine stratification and transports salt landward, the ATM-induced flow exhibits different behaviors because of its varying vertical structure. In estuaries with strong tides, ATM-induced flow tends to enhance stratification and to transport salt landward, similar to density-driven flow. In estuaries with weak tides, ATM-induced flow tends to reduce stratification and to transport salt seaward.</p></div>
]]></content:encoded><description>The role of asymmetric tidal mixing (ATM) in subtidal estuarine dynamics is investigated using a series of generic numerical experiments that simulate narrow estuaries under different stratification and external forcing conditions. The focus is on quantifying the characteristics of ATM-induced flow and its contributions to stratification and salt transport. The flow induced by ATM has a two-layer vertical structure in periodically stratified estuaries, similar to that of the density-driven flow. It has a three-layer vertical structure in the central regime of weakly stratified estuaries, and a reverse two-layer structure in highly stratified estuaries. The changes in vertical distribution of ATM-induced flows result from the influence of stratification on the covariance of eddy viscosity and vertical shear. Such covariance represents the driving force of ATM-induced flow in the tidally averaged momentum equation. Compared to density-driven flow, ATM-induced flow dominates in periodically stratified estuaries with strong tides, has the same order of magnitude in weakly stratified estuaries with moderate tides, and is less important in highly stratified estuaries with weak tides. In contrast to density-driven flow that always increases estuarine stratification and transports salt landward, the ATM-induced flow exhibits different behaviors because of its varying vertical structure. In estuaries with strong tides, ATM-induced flow tends to enhance stratification and to transport salt landward, similar to density-driven flow. In estuaries with weak tides, ATM-induced flow tends to reduce stratification and to transport salt seaward.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20184" xmlns="http://purl.org/rss/1.0/"><title>Temporal changes and impacts of submarine fresh groundwater discharge to the coastal environment: A decadal case study in Toyama Bay, Japan</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20184</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Temporal changes and impacts of submarine fresh groundwater discharge to the coastal environment: A decadal case study in Toyama Bay, Japan</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mariko Hatta, Jing Zhang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-28T11:20:55.220743-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20184</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20184</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20184</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Recent dramatic changes of freshwater systems in high latitudes will allow Submarine Fresh Groundwater Discharge (SFGD) to play a more important role in the coastal environment; especially in that SFGD will directly effect heat flux. Toyama Bay, along the central western Japan coast, is a suitable and representative case study area to estimate SFGD flux using hydrographic properties since multiple high-flow rate SFGD sites exist there. Salinities averaged over the water column (depth range 10–100 m) measured during research cruises in June 2003 and May 2005 show lower levels in the eastern than the western area in this bay. Together with monthly hydrographic properties over a 10 year period (1987–1998), the low-salinity water mass in the eastern area exists consistently but distinctly and varies systematically, as does nutrient flux, affected by SFGD more than riverine input. SFGD fluxes in June 2003 (1 × 10<sup>8</sup> m<sup>3</sup> month<sup>−1</sup>) and May 2005 (&lt;1 × 10<sup>8</sup> m<sup>3</sup> month<sup>−1</sup>) were estimated using a box model, which is divided into a shallow box (0–40 m) and a deeper box (40–100 m). The monthly flux ratio between the SFGD and the river inputs is 13% in June, comparable to higher values reported in other global studies. Our results demonstrate that the box model analysis, based on hydrographic observations in coastal areas, is an efficient approach that can be used to estimate SFGD fluxes between the land and ocean.</p></div>
]]></content:encoded><description>Recent dramatic changes of freshwater systems in high latitudes will allow Submarine Fresh Groundwater Discharge (SFGD) to play a more important role in the coastal environment; especially in that SFGD will directly effect heat flux. Toyama Bay, along the central western Japan coast, is a suitable and representative case study area to estimate SFGD flux using hydrographic properties since multiple high-flow rate SFGD sites exist there. Salinities averaged over the water column (depth range 10–100 m) measured during research cruises in June 2003 and May 2005 show lower levels in the eastern than the western area in this bay. Together with monthly hydrographic properties over a 10 year period (1987–1998), the low-salinity water mass in the eastern area exists consistently but distinctly and varies systematically, as does nutrient flux, affected by SFGD more than riverine input. SFGD fluxes in June 2003 (1 × 108 m3 month−1) and May 2005 (&lt;1 × 108 m3 month−1) were estimated using a box model, which is divided into a shallow box (0–40 m) and a deeper box (40–100 m). The monthly flux ratio between the SFGD and the river inputs is 13% in June, comparable to higher values reported in other global studies. Our results demonstrate that the box model analysis, based on hydrographic observations in coastal areas, is an efficient approach that can be used to estimate SFGD fluxes between the land and ocean.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20194" xmlns="http://purl.org/rss/1.0/"><title>Changes in the onset and intensity of wind-driven upwelling and downwelling along the North American Pacific coast</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20194</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Changes in the onset and intensity of wind-driven upwelling and downwelling along the North American Pacific coast</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Brian Bylhouwer, Debby Ianson, Karen Kohfeld</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-22T16:18:39.007203-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20194</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20194</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20194</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The timing, duration, and intensity of wind-driven upwelling and downwelling along the North American Pacific coast play an integral role in coastal circulation and basinwide ecosystem composition. It has been suggested that global warming will cause changes in these winds. Here we develop a new set of objective criteria to unambiguously determine the onset, duration, and intensity of upwelling and downwelling seasons due to local wind forcing. We use these criteria to examine and better characterize temporal trends in wind-driven coastal currents over the previous 60 years and relate them to global warming and large-scale climate oscillations in the coastal ocean between northern California and Vancouver Island (37°N and 51°N). We find an exceptionally variable onset of upwelling at all locations. Some significant temporal trends are found in summer onset and upwelling intensity time series near the Juan de Fuca Strait and off the coast of Oregon. Positive phases of the Pacific Decadal Oscillation are correlated to later and shorter upwelling seasons with weaker upwelling. Warm phases of the El Niño Southern Oscillation are associated with a later onset of summer upwelling south of Oregon and with more intense downwelling throughout the study area. Our analysis identifies strong interannual to interdecadal variability, and emphasizes the importance of time series length when isolating physical temporal trends influenced by large-scale oscillatory behavior of the climate.</p></div>
]]></content:encoded><description>The timing, duration, and intensity of wind-driven upwelling and downwelling along the North American Pacific coast play an integral role in coastal circulation and basinwide ecosystem composition. It has been suggested that global warming will cause changes in these winds. Here we develop a new set of objective criteria to unambiguously determine the onset, duration, and intensity of upwelling and downwelling seasons due to local wind forcing. We use these criteria to examine and better characterize temporal trends in wind-driven coastal currents over the previous 60 years and relate them to global warming and large-scale climate oscillations in the coastal ocean between northern California and Vancouver Island (37°N and 51°N). We find an exceptionally variable onset of upwelling at all locations. Some significant temporal trends are found in summer onset and upwelling intensity time series near the Juan de Fuca Strait and off the coast of Oregon. Positive phases of the Pacific Decadal Oscillation are correlated to later and shorter upwelling seasons with weaker upwelling. Warm phases of the El Niño Southern Oscillation are associated with a later onset of summer upwelling south of Oregon and with more intense downwelling throughout the study area. Our analysis identifies strong interannual to interdecadal variability, and emphasizes the importance of time series length when isolating physical temporal trends influenced by large-scale oscillatory behavior of the climate.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20197" xmlns="http://purl.org/rss/1.0/"><title>Acoustic scattering from a suspension of flocculated sediments</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20197</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Acoustic scattering from a suspension of flocculated sediments</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Iain T. MacDonald, Christopher E. Vincent, Peter D. Thorne, Benjamin D. Moate</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-22T16:08:47.785383-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20197</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20197</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20197</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A series of controlled laboratory experiments have been conducted to investigate the backscatter of high frequency sound (3–5 MHz) from suspensions of fine sediment in its unflocculated (primary) state and at various levels of flocculation. The size and fall-velocity distributions of the flocs were determined using an optical system and a settling tube, thus allowing floc density to be determined. The measurements have conclusively demonstrated that the acoustic properties of the flocculated particles are not solely controlled by the primary particles; some aspect of the floc structure is influencing the scattering characteristics. The overall trend is for the form function (<em>K<sub>s</sub></em>) to increase as the degree of flocculation increases. This trend was also observed in the total scattering cross section (
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20197/asset/equation/jgrc20197-math-0001.gif?v=1&amp;t=hi5l2ogh&amp;s=1f2f37334d139bacef8904ce32ed74235fcb2ba3" class="inlineGraphic"/>) but this result is dependent on the assumption that viscous absorption for flocculated particles is negligible. The measured scattering properties are compared to the predicted values from two theoretical models, the elastic (ES) and fluid sphere (FS) models. While the results show that, in their current form, neither model is capable of adequately representing the scattering characteristics of a suspension of flocculated particles, the two models did provide upper (ES) and lower (FS) bounds to the measurements. In terms of the operational use of acoustics to measure the concentration of flocculated sediments, empirical relationships could be fitted to the observations but, until a better theoretical understanding of how sound interacts with flocculated particles is achieved, the fitting of such empirical relations may be somewhat premature.</p></div>
]]></content:encoded><description>A series of controlled laboratory experiments have been conducted to investigate the backscatter of high frequency sound (3–5 MHz) from suspensions of fine sediment in its unflocculated (primary) state and at various levels of flocculation. The size and fall-velocity distributions of the flocs were determined using an optical system and a settling tube, thus allowing floc density to be determined. The measurements have conclusively demonstrated that the acoustic properties of the flocculated particles are not solely controlled by the primary particles; some aspect of the floc structure is influencing the scattering characteristics. The overall trend is for the form function (Ks) to increase as the degree of flocculation increases. This trend was also observed in the total scattering cross section (
σt¯) but this result is dependent on the assumption that viscous absorption for flocculated particles is negligible. The measured scattering properties are compared to the predicted values from two theoretical models, the elastic (ES) and fluid sphere (FS) models. While the results show that, in their current form, neither model is capable of adequately representing the scattering characteristics of a suspension of flocculated particles, the two models did provide upper (ES) and lower (FS) bounds to the measurements. In terms of the operational use of acoustics to measure the concentration of flocculated sediments, empirical relationships could be fitted to the observations but, until a better theoretical understanding of how sound interacts with flocculated particles is achieved, the fitting of such empirical relations may be somewhat premature.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20199" xmlns="http://purl.org/rss/1.0/"><title>cBathy: A robust algorithm for estimating nearshore bathymetry</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20199</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">cBathy: A robust algorithm for estimating nearshore bathymetry</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Rob Holman, Nathaniel Plant, Todd Holland</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-22T14:21:42.570884-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20199</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20199</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20199</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A three-part algorithm is described and tested to provide robust bathymetry maps based solely on long time series observations of surface wave motions. The first phase consists of frequency-dependent characterization of the wave field in which dominant frequencies are estimated by Fourier transform while corresponding wave numbers are derived from spatial gradients in cross-spectral phase over analysis tiles that can be small, allowing high-spatial resolution. Coherent spatial structures at each frequency are extracted by frequency-dependent empirical orthogonal function (EOF). In phase two, depths are found that best fit weighted sets of frequency-wave number pairs. These are subsequently smoothed in time in phase 3 using a Kalman filter that fills gaps in coverage and objectively averages new estimates of variable quality with prior estimates. Objective confidence intervals are returned. Tests at Duck, NC, using 16 surveys collected over 2 years showed a bias and root-mean-square (RMS) error of 0.19 and 0.51 m, respectively but were largest near the offshore limits of analysis (roughly 500 m from the camera) and near the steep shoreline where analysis tiles mix information from waves, swash and static dry sand. Performance was excellent for small waves but degraded somewhat with increasing wave height. Sand bars and their small-scale alongshore variability were well resolved. A single ground truth survey from a dissipative, low-sloping beach (Agate Beach, OR) showed similar errors over a region that extended several kilometers from the camera and reached depths of 14 m. Vector wave number estimates can also be incorporated into data assimilation models of nearshore dynamics.</p></div>
]]></content:encoded><description>A three-part algorithm is described and tested to provide robust bathymetry maps based solely on long time series observations of surface wave motions. The first phase consists of frequency-dependent characterization of the wave field in which dominant frequencies are estimated by Fourier transform while corresponding wave numbers are derived from spatial gradients in cross-spectral phase over analysis tiles that can be small, allowing high-spatial resolution. Coherent spatial structures at each frequency are extracted by frequency-dependent empirical orthogonal function (EOF). In phase two, depths are found that best fit weighted sets of frequency-wave number pairs. These are subsequently smoothed in time in phase 3 using a Kalman filter that fills gaps in coverage and objectively averages new estimates of variable quality with prior estimates. Objective confidence intervals are returned. Tests at Duck, NC, using 16 surveys collected over 2 years showed a bias and root-mean-square (RMS) error of 0.19 and 0.51 m, respectively but were largest near the offshore limits of analysis (roughly 500 m from the camera) and near the steep shoreline where analysis tiles mix information from waves, swash and static dry sand. Performance was excellent for small waves but degraded somewhat with increasing wave height. Sand bars and their small-scale alongshore variability were well resolved. A single ground truth survey from a dissipative, low-sloping beach (Agate Beach, OR) showed similar errors over a region that extended several kilometers from the camera and reached depths of 14 m. Vector wave number estimates can also be incorporated into data assimilation models of nearshore dynamics.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20181" xmlns="http://purl.org/rss/1.0/"><title>Southern Ocean nutrient trapping and the efficiency of the biological pump</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20181</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Southern Ocean nutrient trapping and the efficiency of the biological pump</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">François W. Primeau, Mark Holzer, Timothy DeVries</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T12:57:32.862965-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20181</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20181</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20181</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We present a data-assimilated model of the ocean's phosphorus cycle that is constrained by climatological phosphate, temperature, salinity, sea-surface height, surface heat and freshwater fluxes, as well as chlorofluorocarbon-11(CFC-11) and natural Δ<sup>14</sup>C. Export production is estimated to be 5.8±2.0×10<sup>12</sup> mol P/yr of which (26±6)% originates in the Southern Ocean (SO) south of 40°S. The biological pump efficiency, defined as the proportion of the ocean's phosphate inventory that is regenerated, is (39±7)%. Dividing the SO south of 40°S into a sub-Antarctic zone (SANTZ) and an Antarctic zone (ANTZ) separated by the latitude of maximum Ekman divergence, we estimate that the SANTZ and ANTZ account, respectively, for (23±5)% and (3±1)% of global export production, (17±4)% and (3±1)% of the regenerated nutrient inventory, and (31±1)% and (43±5)% of the preformed nutrient inventory. Idealized SO nutrient depletion experiments reveal a large-scale transfer of nutrients into circumpolar and deep waters and from the preformed to the regenerated pool. In accord with the concept of the biogeochemical divide, we find that nutrient drawdown in the ANTZ is more effective than in the SANTZ for increasing the efficiency of the biological pump, while having a smaller impact on production in regions north of 40°S. Complete SO nutrient drawdown would allow the biological pump to operate at 94% efficiency by short circuiting the transport of nutrients in northward Ekman currents, leading to a trapping of nutrients in circumpolar and deep waters that would decrease production outside the SO by approximately 44% while increasing it in the SO by more than 725%.</p></div>
]]></content:encoded><description>We present a data-assimilated model of the ocean's phosphorus cycle that is constrained by climatological phosphate, temperature, salinity, sea-surface height, surface heat and freshwater fluxes, as well as chlorofluorocarbon-11(CFC-11) and natural Δ14C. Export production is estimated to be 5.8±2.0×1012 mol P/yr of which (26±6)% originates in the Southern Ocean (SO) south of 40°S. The biological pump efficiency, defined as the proportion of the ocean's phosphate inventory that is regenerated, is (39±7)%. Dividing the SO south of 40°S into a sub-Antarctic zone (SANTZ) and an Antarctic zone (ANTZ) separated by the latitude of maximum Ekman divergence, we estimate that the SANTZ and ANTZ account, respectively, for (23±5)% and (3±1)% of global export production, (17±4)% and (3±1)% of the regenerated nutrient inventory, and (31±1)% and (43±5)% of the preformed nutrient inventory. Idealized SO nutrient depletion experiments reveal a large-scale transfer of nutrients into circumpolar and deep waters and from the preformed to the regenerated pool. In accord with the concept of the biogeochemical divide, we find that nutrient drawdown in the ANTZ is more effective than in the SANTZ for increasing the efficiency of the biological pump, while having a smaller impact on production in regions north of 40°S. Complete SO nutrient drawdown would allow the biological pump to operate at 94% efficiency by short circuiting the transport of nutrients in northward Ekman currents, leading to a trapping of nutrients in circumpolar and deep waters that would decrease production outside the SO by approximately 44% while increasing it in the SO by more than 725%.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20173" xmlns="http://purl.org/rss/1.0/"><title>Annual maximum water levels from tide gauges: Contributing factors and geographic patterns</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20173</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Annual maximum water levels from tide gauges: Contributing factors and geographic patterns</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mark A. Merrifield, Ayesha S. Genz, Christopher P. Kontoes, John J. Marra</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-20T11:50:32.702534-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20173</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20173</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20173</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20173-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Hourly time series from a quasi-global set of 145 tide gauges are used to investigate annual maximum water levels at each station. High water levels are deconstructed into (1) a predicted tidal component, (2) a seasonal component, (3) a low-frequency nontidal residual that accounts for sea level variability at time scales greater than a month but less than a year, and (4) a high-frequency nontidal residual that captures variability particularly associated with storms at time scales greater than a month. The time-averaged annual maximum water level correlates significantly with, and scales as 2.5 times, the water level standard deviation at the tide gauge stations. This relationship is used to estimate time-averaged annual maximum water level on a nearly continuous global scale (excluding ice-covered polar regions) by specifying variance maps of the tides from a tide model, the seasonal and low-frequency residual components from satellite altimetry sea surface height, and the high-frequency residual component from an atmospheric reanalysis product. The variance fields are combined to estimate time-averaged annual maximum water levels that compare well with observed values at the tide gauge stations. Spatial patterns of annual maximum water levels and relative contributions from the tides and nontidal residual components are considered.</p></div>]]></content:encoded><description>Hourly time series from a quasi-global set of 145 tide gauges are used to investigate annual maximum water levels at each station. High water levels are deconstructed into (1) a predicted tidal component, (2) a seasonal component, (3) a low-frequency nontidal residual that accounts for sea level variability at time scales greater than a month but less than a year, and (4) a high-frequency nontidal residual that captures variability particularly associated with storms at time scales greater than a month. The time-averaged annual maximum water level correlates significantly with, and scales as 2.5 times, the water level standard deviation at the tide gauge stations. This relationship is used to estimate time-averaged annual maximum water level on a nearly continuous global scale (excluding ice-covered polar regions) by specifying variance maps of the tides from a tide model, the seasonal and low-frequency residual components from satellite altimetry sea surface height, and the high-frequency residual component from an atmospheric reanalysis product. The variance fields are combined to estimate time-averaged annual maximum water levels that compare well with observed values at the tide gauge stations. Spatial patterns of annual maximum water levels and relative contributions from the tides and nontidal residual components are considered.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20165" xmlns="http://purl.org/rss/1.0/"><title>Modeling how surface nitrogen fixation influences subsurface nutrient patterns in the North Atlantic</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20165</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Modeling how surface nitrogen fixation influences subsurface nutrient patterns in the North Atlantic</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Chisato Yoshikawa, Victoria J. Coles, Raleigh R. Hood, Douglas G. Capone, Naohiro Yoshida</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-20T11:25:00.604848-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20165</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20165</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20165</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20165-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We represented mechanistically the process of nitrogen (N) fixation and associated N* anomalies in the Atlantic Ocean using a three-dimensional coupled physical/biogeochemical model. Available direct measurements of N fixation rates in the Atlantic Ocean are compiled, and these, along with observed N* anomalies, constrain the model. The model N fixation rate for the whole Atlantic domain is 2.1 × 10<sup>12</sup> molN yr<sup>–1</sup>. The model-generated N* anomaly shows the observed feature of a subsurface maximum. When plotted on isopycnal surfaces, the model-generated N* anomaly bears little relation to the pattern of N fixation at the surface. However, the highest N fixation rates should be spatially related to N* distribution if particulate export is remineralized at depths in the same region where the N fixation occurred. We performed case studies varying remineralization and advection to clarify the genesis of the N* anomaly and to determine the reasons underlying differences between N* anomalies and N fixation rate patterns. These studies indicated that the difference between these two patterns was created by both horizontal advection of excess N compared to phosphorus (P) and preferential remineralization of P compared to N. N fixation and preferential P remineralization create high N* anomalies both at the surface and in subsurface waters in the tropical Atlantic, which are transported into the northwestern North Atlantic by western boundary currents and subsequently subducted. As a result, the highest N* anomalies are located not in the tropics but in the northwestern North Atlantic.</p></div>]]></content:encoded><description>
We represented mechanistically the process of nitrogen (N) fixation and associated N* anomalies in the Atlantic Ocean using a three-dimensional coupled physical/biogeochemical model. Available direct measurements of N fixation rates in the Atlantic Ocean are compiled, and these, along with observed N* anomalies, constrain the model. The model N fixation rate for the whole Atlantic domain is 2.1 × 1012 molN yr–1. The model-generated N* anomaly shows the observed feature of a subsurface maximum. When plotted on isopycnal surfaces, the model-generated N* anomaly bears little relation to the pattern of N fixation at the surface. However, the highest N fixation rates should be spatially related to N* distribution if particulate export is remineralized at depths in the same region where the N fixation occurred. We performed case studies varying remineralization and advection to clarify the genesis of the N* anomaly and to determine the reasons underlying differences between N* anomalies and N fixation rate patterns. These studies indicated that the difference between these two patterns was created by both horizontal advection of excess N compared to phosphorus (P) and preferential remineralization of P compared to N. N fixation and preferential P remineralization create high N* anomalies both at the surface and in subsurface waters in the tropical Atlantic, which are transported into the northwestern North Atlantic by western boundary currents and subsequently subducted. As a result, the highest N* anomalies are located not in the tropics but in the northwestern North Atlantic.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20142" xmlns="http://purl.org/rss/1.0/"><title>Seasonal variability of submarine melt rate and circulation in an East Greenland fjord</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20142</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seasonal variability of submarine melt rate and circulation in an East Greenland fjord</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. Sciascia, F. Straneo, C. Cenedese, P. Heimbach</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-17T09:22:01.469223-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20142</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20142</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20142</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20142-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The circulation in a glacial fjord driven by a large tidewater glacier is investigated using a nonhydrostatic ocean general circulation model with a melt rate parameterization at the vertical glacier front. The model configuration and water properties are based on data collected in Sermilik Fjord near Helheim Glacier, a major Greenland outlet glacier. The approximately two‒layer stratification of the fjord's ambient waters causes the meltwater plume at the glacier front to drive a “double cell” circulation with two distinct outflows, one at the free surface and one at the layers' interface. In summer, the discharge of surface runoff at the base of the glacier (subglacial discharge) causes the circulation to be much more vigorous and associated with a larger melt rate than in winter. The simulated “double cell” circulation is consistent, in both seasons, with observations from Sermilik Fjord. Seasonal differences are also present in the vertical structure of the melt rate, which is maximum at the base of the glacier in summer and at the layers' interface in winter. Simulated submarine melt rates are strongly sensitive to the amount of subglacial discharge, to changes in water temperature, and to the height of the layers. They are also consistent with those inferred from simplified one‒dimensional models based on the theory of buoyant plumes. Our results also indicate that to correctly represent the dynamics of the meltwater plume, care must be taken in the choice of viscosity and diffusivity values in the model.</p></div>]]></content:encoded><description>The circulation in a glacial fjord driven by a large tidewater glacier is investigated using a nonhydrostatic ocean general circulation model with a melt rate parameterization at the vertical glacier front. The model configuration and water properties are based on data collected in Sermilik Fjord near Helheim Glacier, a major Greenland outlet glacier. The approximately two‒layer stratification of the fjord's ambient waters causes the meltwater plume at the glacier front to drive a “double cell” circulation with two distinct outflows, one at the free surface and one at the layers' interface. In summer, the discharge of surface runoff at the base of the glacier (subglacial discharge) causes the circulation to be much more vigorous and associated with a larger melt rate than in winter. The simulated “double cell” circulation is consistent, in both seasons, with observations from Sermilik Fjord. Seasonal differences are also present in the vertical structure of the melt rate, which is maximum at the base of the glacier in summer and at the layers' interface in winter. Simulated submarine melt rates are strongly sensitive to the amount of subglacial discharge, to changes in water temperature, and to the height of the layers. They are also consistent with those inferred from simplified one‒dimensional models based on the theory of buoyant plumes. Our results also indicate that to correctly represent the dynamics of the meltwater plume, care must be taken in the choice of viscosity and diffusivity values in the model.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20185" xmlns="http://purl.org/rss/1.0/"><title>Dense water formation around islands</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20185</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Dense water formation around islands</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Michael A. Spall</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-17T09:01:36.922306-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20185</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20185</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20185</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Basic constraints on the dense water formation rate and circulation resulting from cooling around an island are discussed. The domain under consideration consists of an island surrounded by a shelf, a continental slope, and a stratified ocean. Atmospheric cooling over the shelf forms a dense water that penetrates down the sloping bottom into the stratified basin. Strong azimuthal flows are generated over the sloping bottom as a result of thermal wind. Thermally direct and indirect mean overturning cells are also forced over the slope as a result of bands of convergent and divergent Reynolds stresses associated with the jets. The Coriolis force associated with the net mass flux into the downwelling region over the slope is balanced by these nonlinear terms, giving rise to a fundamentally different momentum budget than arises in semienclosed marginal seas subject to cooling. A similar momentum balance is found for cases with canyons and ridges around the island provided that the terms are considered in a coordinate system that follows the topography. Both eddy fluxes and the mean overturning cells are important for the radial heat flux, although the eddy fluxes typically dominate. The properties of the dense water formed over the shelf (temperature, diapycnal mass flux) are predicted well by application of baroclinic instability theory and simple heat and mass budgets. It is shown that each of these quantities depends only on a nondimensional number derived from environmental parameters such as the shelf depth, Coriolis parameter, offshore temperature field, and atmospheric forcing.</p></div>
]]></content:encoded><description>Basic constraints on the dense water formation rate and circulation resulting from cooling around an island are discussed. The domain under consideration consists of an island surrounded by a shelf, a continental slope, and a stratified ocean. Atmospheric cooling over the shelf forms a dense water that penetrates down the sloping bottom into the stratified basin. Strong azimuthal flows are generated over the sloping bottom as a result of thermal wind. Thermally direct and indirect mean overturning cells are also forced over the slope as a result of bands of convergent and divergent Reynolds stresses associated with the jets. The Coriolis force associated with the net mass flux into the downwelling region over the slope is balanced by these nonlinear terms, giving rise to a fundamentally different momentum budget than arises in semienclosed marginal seas subject to cooling. A similar momentum balance is found for cases with canyons and ridges around the island provided that the terms are considered in a coordinate system that follows the topography. Both eddy fluxes and the mean overturning cells are important for the radial heat flux, although the eddy fluxes typically dominate. The properties of the dense water formed over the shelf (temperature, diapycnal mass flux) are predicted well by application of baroclinic instability theory and simple heat and mass budgets. It is shown that each of these quantities depends only on a nondimensional number derived from environmental parameters such as the shelf depth, Coriolis parameter, offshore temperature field, and atmospheric forcing.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20163" xmlns="http://purl.org/rss/1.0/"><title>Evaluation of model nesting performance on the Texas-Louisiana continental shelf</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20163</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Evaluation of model nesting performance on the Texas-Louisiana continental shelf</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Martinho Marta-Almeida, Robert D. Hetland, Xiaoqian Zhang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-15T14:33:32.474114-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20163</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20163</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20163</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20163-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A skill assessment of a model of the Texas-Louisiana shelf, nested in a variety of different parent models, is performed using hydrographic salinity data. The nested models show improved salinity skill compared to the same model using climatological boundary conditions, as well as general skill score improvements over the parent models in the same region. Although a variety of parent models are used and these parent models have widely different skill scores when compared with regional hydrographic data sets, the skill scores for the nested models are generally indistinguishable. This leads to the conclusion that nesting is important for improving model skill, but it does not matter which parent model is used. The model is also used to create a series of ensembles, where the local forcing is varied with identical boundary conditions and where the boundary conditions are varied by nesting within the various parent models. The variance in the ensemble spread shows that there is a significant level of unpredictable, nonlinear noise associated with instabilities along the Mississippi/Atchafalaya plume front. The noise is seasonal and is greatest during summer upwelling conditions and weaker during nonsummer downwelling.</p></div>]]></content:encoded><description>
A skill assessment of a model of the Texas-Louisiana shelf, nested in a variety of different parent models, is performed using hydrographic salinity data. The nested models show improved salinity skill compared to the same model using climatological boundary conditions, as well as general skill score improvements over the parent models in the same region. Although a variety of parent models are used and these parent models have widely different skill scores when compared with regional hydrographic data sets, the skill scores for the nested models are generally indistinguishable. This leads to the conclusion that nesting is important for improving model skill, but it does not matter which parent model is used. The model is also used to create a series of ensembles, where the local forcing is varied with identical boundary conditions and where the boundary conditions are varied by nesting within the various parent models. The variance in the ensemble spread shows that there is a significant level of unpredictable, nonlinear noise associated with instabilities along the Mississippi/Atchafalaya plume front. The noise is seasonal and is greatest during summer upwelling conditions and weaker during nonsummer downwelling.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20166" xmlns="http://purl.org/rss/1.0/"><title>Modeling Antarctic ice shelf responses to future climate changes and impacts on the ocean</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20166</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Modeling Antarctic ice shelf responses to future climate changes and impacts on the ocean</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Kazuya Kusahara, Hiroyasu Hasumi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-14T15:40:35.405814-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20166</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20166</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20166</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20166-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We investigate basal melting of all Antarctic ice shelves by a circumpolar ice shelf-sea ice-ocean coupled model and estimate the total basal melting of 770–944 Gt/yr under present-day climate conditions. We present a comparison of the basal melting with previous observational and modeling estimates for each ice shelf. Heat sources for basal melting are largely different among the ice shelves. Sensitivities of the basal melting to surface air warming and to enhanced westerly winds over the Antarctic Circumpolar Current are investigated from a series of numerical experiments. In this model the total basal melting strongly depends on the surface air warming but is hardly affected by the change of westerly winds. The magnitude of the basal melting response to the warming varies widely from one ice shelf to another. The largest response is found at ice shelves in the Bellingshausen Sea, followed by those in the Eastern Weddell Sea and the Indian sector. These increases of basal melting are caused by increases of Circumpolar Deep Water and/or Antarctic Surface Water into ice shelf cavities. By contrast, basal melting of ice shelves in the Ross and Weddell Seas is insensitive to the surface air warming, because even in the warming experiments there is high sea ice production at the front of the ice shelves that keeps the water temperature to the surface freezing point. Weakening of the thermohaline circulation driven by Antarctic dense water formation under warming climate conditions is enhanced by basal melting of ice shelves.</p></div>]]></content:encoded><description>We investigate basal melting of all Antarctic ice shelves by a circumpolar ice shelf-sea ice-ocean coupled model and estimate the total basal melting of 770–944 Gt/yr under present-day climate conditions. We present a comparison of the basal melting with previous observational and modeling estimates for each ice shelf. Heat sources for basal melting are largely different among the ice shelves. Sensitivities of the basal melting to surface air warming and to enhanced westerly winds over the Antarctic Circumpolar Current are investigated from a series of numerical experiments. In this model the total basal melting strongly depends on the surface air warming but is hardly affected by the change of westerly winds. The magnitude of the basal melting response to the warming varies widely from one ice shelf to another. The largest response is found at ice shelves in the Bellingshausen Sea, followed by those in the Eastern Weddell Sea and the Indian sector. These increases of basal melting are caused by increases of Circumpolar Deep Water and/or Antarctic Surface Water into ice shelf cavities. By contrast, basal melting of ice shelves in the Ross and Weddell Seas is insensitive to the surface air warming, because even in the warming experiments there is high sea ice production at the front of the ice shelves that keeps the water temperature to the surface freezing point. Weakening of the thermohaline circulation driven by Antarctic dense water formation under warming climate conditions is enhanced by basal melting of ice shelves.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20179" xmlns="http://purl.org/rss/1.0/"><title>Sea ice thickness estimations from ICESat Altimetry over the Bellingshausen and Amundsen Seas, 2003–2009</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20179</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea ice thickness estimations from ICESat Altimetry over the Bellingshausen and Amundsen Seas, 2003–2009</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Hongjie Xie, Ahmet Emre Tekeli, Stephen F. Ackley, Donghui Yi, H. Jay Zwally</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-10T11:05:42.418103-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20179</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20179</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20179</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20179-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Sea ice thicknesses derived from NASA's Ice, Cloud, and Land Elevation Satellite (ICESat) altimetry data are examined using two different approaches, buoyancy and empirical equations, and at two spatial scales—ICESat footprint size (70 m diameter spot) and Advanced Microwave Scanning Radiometer (AMSR-E) pixel size (12.5 km by 12.5 km) for the Bellingshausen and Amundsen Seas of west Antarctica. Ice thickness from the empirical equation shows reasonable spatial and temporal distribution of ice thickness from 2003 to 2009. Ice thickness from the buoyancy equation, however, additionally needing snow depth information derived from the AMSR-E, shows an overestimation in terms of maximum, mean (+63% to 75%), and standard deviation while underestimation in modal thickness (−20%) as compared with those from the empirical equation approach. When ICESat snow freeboard is used as the snow depth in the buoyancy equation, i.e., the zero ice freeboard assumption, the derived ice thicknesses match well with those from the empirical equation approach, within 5% overall. The AMSR-E, therefore, may underestimate snow depth and accounts for ~95% of the ice thickness overestimation as compared with the buoyancy approach. The empirical equation derived ice thickness shows a consistent asymmetrical distribution with a long tail to high values, and seasonal median values ranging from 0.8 to 1.4 m over the 2003–2009 period that are always larger than the corresponding modal values (0.6–1.1 m) and lower than the mean values (1.0–1.6 m), with standard deviation of 0.6–1.0 m. An overall increasing trend of 0.03 m/year of mean ice thickness is found from 2003 to 2009, although statistically insignificant (<em>p</em> = 0.11) at the 95% confidence level. Starting from autumn, a general picture of seasonal mean, modal, and median ice thickness increases progressively from autumn to spring and decreases from spring to the following autumn, when new thin ice dominates the ice thickness distribution. The asymmetric shape of the thickness distribution reflects the key role of ice deformation processes in the evolution of the thickness distribution. The statistical properties of the thickness distribution interannually (high range of mean thickness and standard deviation) indicate the variability of deformation processes. However, spring ice volume, the product of ice mean thickness and areal extent computed for the spring maximum, shows variability year to year but is primarily dominated by ice extent variability, with no increasing or decreasing trend over this record length. The dependence of the volume on the ice extent primarily suggests that ice thickness changes have also not covaried with the ice extent losses seen over the satellite record in this region, unlike the Arctic. These properties reflect the interactive processes of ice advection, thermodynamic growth and ice deformation that all substantially influence ice mass balance in the Bellingshausen-Amundsen Seas region.</p></div>]]></content:encoded><description>Sea ice thicknesses derived from NASA's Ice, Cloud, and Land Elevation Satellite (ICESat) altimetry data are examined using two different approaches, buoyancy and empirical equations, and at two spatial scales—ICESat footprint size (70 m diameter spot) and Advanced Microwave Scanning Radiometer (AMSR-E) pixel size (12.5 km by 12.5 km) for the Bellingshausen and Amundsen Seas of west Antarctica. Ice thickness from the empirical equation shows reasonable spatial and temporal distribution of ice thickness from 2003 to 2009. Ice thickness from the buoyancy equation, however, additionally needing snow depth information derived from the AMSR-E, shows an overestimation in terms of maximum, mean (+63% to 75%), and standard deviation while underestimation in modal thickness (−20%) as compared with those from the empirical equation approach. When ICESat snow freeboard is used as the snow depth in the buoyancy equation, i.e., the zero ice freeboard assumption, the derived ice thicknesses match well with those from the empirical equation approach, within 5% overall. The AMSR-E, therefore, may underestimate snow depth and accounts for ~95% of the ice thickness overestimation as compared with the buoyancy approach. The empirical equation derived ice thickness shows a consistent asymmetrical distribution with a long tail to high values, and seasonal median values ranging from 0.8 to 1.4 m over the 2003–2009 period that are always larger than the corresponding modal values (0.6–1.1 m) and lower than the mean values (1.0–1.6 m), with standard deviation of 0.6–1.0 m. An overall increasing trend of 0.03 m/year of mean ice thickness is found from 2003 to 2009, although statistically insignificant (p = 0.11) at the 95% confidence level. Starting from autumn, a general picture of seasonal mean, modal, and median ice thickness increases progressively from autumn to spring and decreases from spring to the following autumn, when new thin ice dominates the ice thickness distribution. The asymmetric shape of the thickness distribution reflects the key role of ice deformation processes in the evolution of the thickness distribution. The statistical properties of the thickness distribution interannually (high range of mean thickness and standard deviation) indicate the variability of deformation processes. However, spring ice volume, the product of ice mean thickness and areal extent computed for the spring maximum, shows variability year to year but is primarily dominated by ice extent variability, with no increasing or decreasing trend over this record length. The dependence of the volume on the ice extent primarily suggests that ice thickness changes have also not covaried with the ice extent losses seen over the satellite record in this region, unlike the Arctic. These properties reflect the interactive processes of ice advection, thermodynamic growth and ice deformation that all substantially influence ice mass balance in the Bellingshausen-Amundsen Seas region.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20190" xmlns="http://purl.org/rss/1.0/"><title>Quantifying the length-scale dependence of surf zone advection</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20190</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Quantifying the length-scale dependence of surf zone advection</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Greg W. Wilson, H. Tuba Özkan-Haller, Robert A. Holman</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T13:41:02.276147-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20190</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20190</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20190</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We investigate the momentum balance in the surf zone, in a setting which is weakly varying in the alongshore direction. Our focus is on the role of nonlinear advective terms. Using numerical experiments, we find that advection tends to counteract alongshore variations in momentum flux, resulting in more uniform kinematics. Additionally, advection causes a shifting of the kinematic response in the direction of flow. These effects are strongest at short alongshore length scales, and/or strong alongshore-mean velocity. The length-scale dependence is investigated using spectral analysis, where the effect of advective terms is treated as a transfer function applied to the solution to the linear (advection-free) equations of motion. The transfer function is then shown to be governed by a nondimensional parameter which quantifies the relative scales of advection and bottom stress, analogous to a Reynolds Number. Hence, this parameter can be used to quantify the length scales at which advective terms, and the resulting effects described above, are important. We also introduce an approximate functional form for the transfer function, which is valid asymptotically within a restricted range of length scales.</p></div>
]]></content:encoded><description>We investigate the momentum balance in the surf zone, in a setting which is weakly varying in the alongshore direction. Our focus is on the role of nonlinear advective terms. Using numerical experiments, we find that advection tends to counteract alongshore variations in momentum flux, resulting in more uniform kinematics. Additionally, advection causes a shifting of the kinematic response in the direction of flow. These effects are strongest at short alongshore length scales, and/or strong alongshore-mean velocity. The length-scale dependence is investigated using spectral analysis, where the effect of advective terms is treated as a transfer function applied to the solution to the linear (advection-free) equations of motion. The transfer function is then shown to be governed by a nondimensional parameter which quantifies the relative scales of advection and bottom stress, analogous to a Reynolds Number. Hence, this parameter can be used to quantify the length scales at which advective terms, and the resulting effects described above, are important. We also introduce an approximate functional form for the transfer function, which is valid asymptotically within a restricted range of length scales.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20188" xmlns="http://purl.org/rss/1.0/"><title>Toward representing wave-induced sediment suspension over sand ripples in RANS models</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20188</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Toward representing wave-induced sediment suspension over sand ripples in RANS models</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Laurent O. Amoudry, Paul S. Bell, Peter D. Thorne, Alejandro J. Souza</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T13:25:50.011553-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20188</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20188</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20188</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Parameterizations of near-bed sediment processes are commonly associated with the poor predictive skill of coastal sediment transport models. We implement a two-dimensional Reynolds-averaged Navier-Stokes model to directly assess these parameterizations by reproducing measurements obtained in large-scale wave flume experiments. A sediment transport model has been coupled to wave hydrodynamics and turbulence, and numerical experiments provide temporal and spatial variations of free surface, flow velocity, sediment concentration, and turbulence quantities. Model-data comparisons enable the direct assessment of how key suspension processes are represented and of the inherent variability of the sediment transport model. We focus on the different processes occurring above rippled beds versus dynamically flat beds. Numerical results show that increasing roughness alone is not sufficient to have good predictive capability above steep ripples. Some parameterization of the vortex entrainment process is necessary and a simple modification, which leads to constant sediment diffusivity above steep-rippled beds, is sufficient to obtain good predictions of wave-averaged suspended concentrations. Model-data comparisons for the turbulent kinetic energy are also presented and highlight the need to account for the effect of vortex entrainment on near-bed turbulence and transfer of momentum.</p></div>
]]></content:encoded><description>Parameterizations of near-bed sediment processes are commonly associated with the poor predictive skill of coastal sediment transport models. We implement a two-dimensional Reynolds-averaged Navier-Stokes model to directly assess these parameterizations by reproducing measurements obtained in large-scale wave flume experiments. A sediment transport model has been coupled to wave hydrodynamics and turbulence, and numerical experiments provide temporal and spatial variations of free surface, flow velocity, sediment concentration, and turbulence quantities. Model-data comparisons enable the direct assessment of how key suspension processes are represented and of the inherent variability of the sediment transport model. We focus on the different processes occurring above rippled beds versus dynamically flat beds. Numerical results show that increasing roughness alone is not sufficient to have good predictive capability above steep ripples. Some parameterization of the vortex entrainment process is necessary and a simple modification, which leads to constant sediment diffusivity above steep-rippled beds, is sufficient to obtain good predictions of wave-averaged suspended concentrations. Model-data comparisons for the turbulent kinetic energy are also presented and highlight the need to account for the effect of vortex entrainment on near-bed turbulence and transfer of momentum.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20187" xmlns="http://purl.org/rss/1.0/"><title>Observed near-surface flows under all tropical cyclone intensity levels using drifters in the northwestern Pacific</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20187</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Observed near-surface flows under all tropical cyclone intensity levels using drifters in the northwestern Pacific</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Yu-Chia Chang, Guan-Yu Chen, Ruo-Shan Tseng, Luca R. Centurioni, Peter C. Chu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T13:24:17.912156-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20187</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20187</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20187</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Data from drifters of the surface velocity program and tropical cyclones (TCs) of the Joint Typhoon Warning Center during 1985–2009 were analyzed to demonstrate strong currents under various storm intensities such as category-4 to −5, category-2 to −3, and tropical storm to category-1 TCs in the northwestern Pacific. Current speeds over 2.0 m s<sup>−1</sup> are observed under major TCs with the strongest mean currents to the right of the storm track. This study provides the characterization of the near-surface velocity response to all recorded TCs, and agrees roughly with Geisler's theory (1970). Our observations also verify earlier modeling results of Price (1983).</p></div>
]]></content:encoded><description>Data from drifters of the surface velocity program and tropical cyclones (TCs) of the Joint Typhoon Warning Center during 1985–2009 were analyzed to demonstrate strong currents under various storm intensities such as category-4 to −5, category-2 to −3, and tropical storm to category-1 TCs in the northwestern Pacific. Current speeds over 2.0 m s−1 are observed under major TCs with the strongest mean currents to the right of the storm track. This study provides the characterization of the near-surface velocity response to all recorded TCs, and agrees roughly with Geisler's theory (1970). Our observations also verify earlier modeling results of Price (1983).
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20192" xmlns="http://purl.org/rss/1.0/"><title>Temperature inversions and their influence on the mixed layer heat budget during the winters of 2006–2007 and 2007–2008 in the Bay of Bengal</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20192</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Temperature inversions and their influence on the mixed layer heat budget during the winters of 2006–2007 and 2007–2008 in the Bay of Bengal</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. S. Girishkumar, M. Ravichandran, M. J. McPhaden</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T13:21:54.973154-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20192</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20192</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20192</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Time series measurements of temperature, salinity and surface meteorological parameters recorded at 8°N, 90°E in the southern central Bay of Bengal (BoB) from a Research Moored Array for African-Asian-Australian Monsoon Analysis and predication (RAMA) buoy are used to document temperature inversions and their influence on the mixed layer heat budget during the winters, defined as October to March, of 2006–2007 (W67) and 2007–2008 (W78). There is a marked difference in the frequency and amplitude of temperature inversion between these two winters, with variations much stronger in W78 compared to W67. The formation of temperature inversions is favored by the existence of thick barrier layers, which are also more prominent in W78 compared to W67. Inversions occur when heating in the barrier layer below the mixed layer by penetrative shortwave radiation is greater than heating of the mixed layer by net surface heat flux and horizontal advection. Our analysis further demonstrates that intraseasonal and year-to-year variability in the frequency and magnitude of temperature inversions during winter have substantial influence on mixed layer temperature through the modulation of vertical heat flux at the base of mixed layer.</p></div>
]]></content:encoded><description>Time series measurements of temperature, salinity and surface meteorological parameters recorded at 8°N, 90°E in the southern central Bay of Bengal (BoB) from a Research Moored Array for African-Asian-Australian Monsoon Analysis and predication (RAMA) buoy are used to document temperature inversions and their influence on the mixed layer heat budget during the winters, defined as October to March, of 2006–2007 (W67) and 2007–2008 (W78). There is a marked difference in the frequency and amplitude of temperature inversion between these two winters, with variations much stronger in W78 compared to W67. The formation of temperature inversions is favored by the existence of thick barrier layers, which are also more prominent in W78 compared to W67. Inversions occur when heating in the barrier layer below the mixed layer by penetrative shortwave radiation is greater than heating of the mixed layer by net surface heat flux and horizontal advection. Our analysis further demonstrates that intraseasonal and year-to-year variability in the frequency and magnitude of temperature inversions during winter have substantial influence on mixed layer temperature through the modulation of vertical heat flux at the base of mixed layer.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20191" xmlns="http://purl.org/rss/1.0/"><title>Arctic sea ice circulation and drift speed: Decadal trends and ocean currents</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20191</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Arctic sea ice circulation and drift speed: Decadal trends and ocean currents</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. Kwok, G. Spreen, S. Pang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T13:10:31.453687-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20191</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20191</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20191</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We examine the basinwide trends in sea ice circulation and drift speed and highlight the changes between 1982 and 2009 in connection to regional winds, multiyear sea ice coverage, ice export, and the thinning of the ice cover. The polarity of the Arctic Oscillation (AO) is used as a backdrop for summarizing the variance and shifts in decadal drift patterns. The 28-year circulation fields show a net strengthening of the Beaufort Gyre and the Transpolar Drift, especially during the last decade. The imprint of the arctic dipole anomaly on the mean summer circulation is evident (2001–2009) and enhances summer ice area export at the Fram Strait. Between 2001 and 2009, the large spatially averaged trends in drift speeds (winter: +23.6%/decade, summer: +17.7%/decade) are not explained by the much smaller trends in wind speeds (winter: 1.46%/decade, summer: −3.42%/decade). Notably, positive trends in drift speed are found in regions with reduced multiyear sea ice coverage. Over 90% of the Arctic Ocean has positive trends in drift speed and negative trends in multiyear sea ice coverage. The increased responsiveness of ice drift to geostrophic wind is consistent with a thinner and weaker seasonal ice cover and suggests large-scale changes in the air-ice-ocean momentum balance. The retrieved mean ocean current field from decadal-scale average ice motion captures a steady drift from Siberia to the Fram Strait, an inflow north of the Bering Strait, and a westward drift along coastal Alaska. This mean current is comparable to geostrophic currents from satellite-derived dynamic topography.</p></div>
]]></content:encoded><description>We examine the basinwide trends in sea ice circulation and drift speed and highlight the changes between 1982 and 2009 in connection to regional winds, multiyear sea ice coverage, ice export, and the thinning of the ice cover. The polarity of the Arctic Oscillation (AO) is used as a backdrop for summarizing the variance and shifts in decadal drift patterns. The 28-year circulation fields show a net strengthening of the Beaufort Gyre and the Transpolar Drift, especially during the last decade. The imprint of the arctic dipole anomaly on the mean summer circulation is evident (2001–2009) and enhances summer ice area export at the Fram Strait. Between 2001 and 2009, the large spatially averaged trends in drift speeds (winter: +23.6%/decade, summer: +17.7%/decade) are not explained by the much smaller trends in wind speeds (winter: 1.46%/decade, summer: −3.42%/decade). Notably, positive trends in drift speed are found in regions with reduced multiyear sea ice coverage. Over 90% of the Arctic Ocean has positive trends in drift speed and negative trends in multiyear sea ice coverage. The increased responsiveness of ice drift to geostrophic wind is consistent with a thinner and weaker seasonal ice cover and suggests large-scale changes in the air-ice-ocean momentum balance. The retrieved mean ocean current field from decadal-scale average ice motion captures a steady drift from Siberia to the Fram Strait, an inflow north of the Bering Strait, and a westward drift along coastal Alaska. This mean current is comparable to geostrophic currents from satellite-derived dynamic topography.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20180" xmlns="http://purl.org/rss/1.0/"><title>Variations in the Pacific Decadal Oscillation since 1853 in a coral record from the northern South China Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20180</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Variations in the Pacific Decadal Oscillation since 1853 in a coral record from the northern South China Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Wenfeng Deng, Gangjian Wei, Luhua Xie, Ting Ke, Zhibing Wang, Ti Zeng, Ying Liu</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T10:44:32.560913-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20180</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20180</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20180</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The Pacific Decadal Oscillation (PDO) has been shown to have significant climatic and environmental impacts across the Pan-Pacific Basin; however, there are no records of PDO activity from the South China Sea (SCS), the largest marginal sea in the northwest Pacific Ocean. This study suggests that a series of geochemical profiles obtained from a modern coral in the northern SCS records annual PDO activity dating back to 1853. These geochemical data are significantly correlated with the PDO index, and their patterns of variation closely match those of the PDO index over the last century. The relationship between the PDO and coral geochemistry may be related to the influence of the PDO on rainfall on Hainan Island. Rainfall patterns influence the volume of terrestrial runoff, which, in turn, is a primary determinant of δ<sup>18</sup>O and Δδ<sup>18</sup>O values in coral; however, coral δ<sup>13</sup>C values are also influenced by the <sup>13</sup>C Suess effect. The results indicate that Sr/Ca ratios in coral are affected by a combination of sea surface temperature and terrestrial runoff.</p></div>
]]></content:encoded><description>The Pacific Decadal Oscillation (PDO) has been shown to have significant climatic and environmental impacts across the Pan-Pacific Basin; however, there are no records of PDO activity from the South China Sea (SCS), the largest marginal sea in the northwest Pacific Ocean. This study suggests that a series of geochemical profiles obtained from a modern coral in the northern SCS records annual PDO activity dating back to 1853. These geochemical data are significantly correlated with the PDO index, and their patterns of variation closely match those of the PDO index over the last century. The relationship between the PDO and coral geochemistry may be related to the influence of the PDO on rainfall on Hainan Island. Rainfall patterns influence the volume of terrestrial runoff, which, in turn, is a primary determinant of δ18O and Δδ18O values in coral; however, coral δ13C values are also influenced by the 13C Suess effect. The results indicate that Sr/Ca ratios in coral are affected by a combination of sea surface temperature and terrestrial runoff.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20156" xmlns="http://purl.org/rss/1.0/"><title>Seismic reflection imaging of shallow oceanographic structures</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20156</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seismic reflection imaging of shallow oceanographic structures</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Helen Piété, Louis Marié, Bruno Marsset, Yannick Thomas, Marc-André Gutscher</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-08T13:41:57.473939-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20156</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20156</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20156</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20156-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Multichannel seismic (MCS) reflection profiling can provide high lateral resolution images of deep ocean thermohaline fine structure. However, the shallowest layers of the water column (<em>z</em> &lt; 150 m) have remained unexplored by this technique until recently. In order to explore the feasibility of shallow seismic oceanography (SO), we reprocessed and analyzed four multichannel seismic reflection sections featuring reflectors at depths between 10 and 150 m. The influence of the acquisition parameters was quantified. Seismic data processing dedicated to SO was also investigated. Conventional seismic acquisition systems were found to be ill-suited to the imaging of shallow oceanographic structures, because of a high antenna filter effect induced by large offsets and seismic trace lengths, and sources that typically cannot provide both a high level of emission and fine vertical resolution. We considered a test case, the imagery of the seasonal thermocline on the western Brittany continental shelf. New oceanographic data acquired in this area allowed simulation of the seismic acquisition. Sea trials of a specifically designed system were performed during the ASPEX survey, conducted in early summer 2012. The seismic device featured: (i) four seismic streamers, each consisting of six traces of 1.80 m; (ii) a 1000 J SIG sparker source, providing a 400 Hz signal with a level of emission of 205 dB re 1 μPa @ 1 m. This survey captured the 15 m thick, 30 m deep seasonal thermocline in unprecedented detail, showing images of vertical displacements most probably induced by internal waves.</p></div>]]></content:encoded><description>
Multichannel seismic (MCS) reflection profiling can provide high lateral resolution images of deep ocean thermohaline fine structure. However, the shallowest layers of the water column (z &lt; 150 m) have remained unexplored by this technique until recently. In order to explore the feasibility of shallow seismic oceanography (SO), we reprocessed and analyzed four multichannel seismic reflection sections featuring reflectors at depths between 10 and 150 m. The influence of the acquisition parameters was quantified. Seismic data processing dedicated to SO was also investigated. Conventional seismic acquisition systems were found to be ill-suited to the imaging of shallow oceanographic structures, because of a high antenna filter effect induced by large offsets and seismic trace lengths, and sources that typically cannot provide both a high level of emission and fine vertical resolution. We considered a test case, the imagery of the seasonal thermocline on the western Brittany continental shelf. New oceanographic data acquired in this area allowed simulation of the seismic acquisition. Sea trials of a specifically designed system were performed during the ASPEX survey, conducted in early summer 2012. The seismic device featured: (i) four seismic streamers, each consisting of six traces of 1.80 m; (ii) a 1000 J SIG sparker source, providing a 400 Hz signal with a level of emission of 205 dB re 1 μPa @ 1 m. This survey captured the 15 m thick, 30 m deep seasonal thermocline in unprecedented detail, showing images of vertical displacements most probably induced by internal waves.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20167" xmlns="http://purl.org/rss/1.0/"><title>A comparison of methods to determine phytoplankton bloom initiation</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20167</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A comparison of methods to determine phytoplankton bloom initiation</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sarah R. Brody, M. Susan Lozier, John P. Dunne</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-08T08:25:27.816861-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20167</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20167</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20167</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Articles</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20167-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Phytoplankton bloom phenology has important consequences for marine ecosystems and fisheries. Recent studies have used remotely sensed ocean color data to calculate metrics associated with the phenological cycle, such as the phytoplankton bloom initiation date, on regional and global scales. These metrics are often linked to physical or biological forcings. Most studies choose one of several common methods for calculating bloom initiation, leading to questions about whether bloom initiation dates calculated with different methods yield comparable results. Here we compare three methods for finding the date of phytoplankton bloom initiation in the North Atlantic: a biomass-based threshold method, a rate of change method, and a cumulative biomass-based threshold method. We use these methods to examine whether the onset of positive ocean-atmosphere heat fluxes coincides with subpolar bloom initiation. In several coherent locations, we find differences in the patterns of bloom initiation created by each method and differences in the synchrony between bloom initiation and positive heat fluxes, which likely indicate various physical processes at play in the study region. We also assess the effect of missing data on the chosen methods.</p></div>]]></content:encoded><description>Phytoplankton bloom phenology has important consequences for marine ecosystems and fisheries. Recent studies have used remotely sensed ocean color data to calculate metrics associated with the phenological cycle, such as the phytoplankton bloom initiation date, on regional and global scales. These metrics are often linked to physical or biological forcings. Most studies choose one of several common methods for calculating bloom initiation, leading to questions about whether bloom initiation dates calculated with different methods yield comparable results. Here we compare three methods for finding the date of phytoplankton bloom initiation in the North Atlantic: a biomass-based threshold method, a rate of change method, and a cumulative biomass-based threshold method. We use these methods to examine whether the onset of positive ocean-atmosphere heat fluxes coincides with subpolar bloom initiation. In several coherent locations, we find differences in the patterns of bloom initiation created by each method and differences in the synchrony between bloom initiation and positive heat fluxes, which likely indicate various physical processes at play in the study region. We also assess the effect of missing data on the chosen methods.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20175" xmlns="http://purl.org/rss/1.0/"><title>Structure and surface properties of eddies in the southeast Pacific Ocean</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20175</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Structure and surface properties of eddies in the southeast Pacific Ocean</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">James Holte, Fiamma Straneo, Carlos Moffat, Robert Weller, J. Thomas Farrar</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-07T15:33:37.691265-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20175</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20175</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20175</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20175-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A number of studies have posited that coastally generated eddies could cool the southeast Pacific Ocean (SEP) by advecting cool, upwelled waters offshore. We examine this mechanism by characterizing the upper-ocean properties of mesoscale eddies in the SEP with a variety of observations and by estimating the surface-layer eddy heat flux divergence with satellite data. Cyclonic and anticyclonic eddies observed during two cruises featured deep positive salinity anomalies along the 26.5 kg m<sup>−3</sup>isopycnal, indicating that the eddies had likely trapped and transported coastal waters offshore. The cyclonic eddies observed during the cruises were characterized by shoaling isopycnals in the upper 200 m and cool near-surface temperature anomalies, whereas the upper-ocean structure of anticyclonic eddies was more variable. Using a variety of large-scale observations, including Argo float profiles, drifter records, and satellite sea surface temperature fields, we show that, relative to mean conditions, cyclonic eddies are associated with cooler surface temperatures and that anticyclonic eddies are associated with warmer surface temperatures. Within each data set, the mean eddy surface temperature anomalies are small and of approximately equal magnitude but opposite sign. Eddy statistics drawn from satellite altimetry data reveal that cyclonic and anticyclonic eddies occur with similar frequency and have similar average radii in the SEP. A satellite-based estimate of the surface-layer eddy heat flux divergence, while large in coastal regions, is small when averaged over the SEP, suggesting that eddies do not substantially contribute to cooling the surface layer of the SEP.</p></div>]]></content:encoded><description>
A number of studies have posited that coastally generated eddies could cool the southeast Pacific Ocean (SEP) by advecting cool, upwelled waters offshore. We examine this mechanism by characterizing the upper-ocean properties of mesoscale eddies in the SEP with a variety of observations and by estimating the surface-layer eddy heat flux divergence with satellite data. Cyclonic and anticyclonic eddies observed during two cruises featured deep positive salinity anomalies along the 26.5 kg m−3isopycnal, indicating that the eddies had likely trapped and transported coastal waters offshore. The cyclonic eddies observed during the cruises were characterized by shoaling isopycnals in the upper 200 m and cool near-surface temperature anomalies, whereas the upper-ocean structure of anticyclonic eddies was more variable. Using a variety of large-scale observations, including Argo float profiles, drifter records, and satellite sea surface temperature fields, we show that, relative to mean conditions, cyclonic eddies are associated with cooler surface temperatures and that anticyclonic eddies are associated with warmer surface temperatures. Within each data set, the mean eddy surface temperature anomalies are small and of approximately equal magnitude but opposite sign. Eddy statistics drawn from satellite altimetry data reveal that cyclonic and anticyclonic eddies occur with similar frequency and have similar average radii in the SEP. A satellite-based estimate of the surface-layer eddy heat flux divergence, while large in coastal regions, is small when averaged over the SEP, suggesting that eddies do not substantially contribute to cooling the surface layer of the SEP.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20183" xmlns="http://purl.org/rss/1.0/"><title>Spatial distribution of brominated very short-lived substances in the eastern Pacific</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20183</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Spatial distribution of brominated very short-lived substances in the eastern Pacific</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Yina Liu, Shari A. Yvon-Lewis, Daniel C. O. Thornton, Lisa Campbell, Thomas S. Bianchi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-07T14:53:33.686325-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20183</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20183</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20183</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Seawater concentrations and distributions of brominated very short-lived substances (BrVSLS), including bromoform (CHBr<sub>3</sub>), dibromomethane (CH<sub>2</sub>Br<sub>2</sub>), bromodichloromethane (CHBrCl<sub>2</sub>), chlorodibromomethane (CHClBr<sub>2</sub>), were measured in the upper water column (5–750 m) in the eastern Pacific. Inorganic nutrient, pigment concentrations, and picoplankton cell counts were measured to determine biogeochemical factors that affect the production and distribution of these BrVSLS. Elevated concentrations of BrVSLS were observed in coastal and tropical seawater. Concentration maxima for CHBr<sub>3</sub>, CH<sub>2</sub>Br<sub>2</sub>, and CHClBr<sub>2</sub> were observed below the mixed layer, near the subsurface chlorophyll <em>a</em> maxima, which suggest BrVSLS production may be related to photosynthetic biomass production. Our results also suggest that heterotrophic bacteria may also contribute to CH<sub>2</sub>Br<sub>2</sub> and CHBrCl<sub>2</sub> production in the water column. The maximum CHBrCl<sub>2</sub> concentration was observed at a depth much deeper than the euphotic zone, which suggests sources other than photosynthetic biomass. Elevated CHBrCl<sub>2</sub> concentrations in deeper waters were coincident with elevated CHCl<sub>3</sub> concentrations, which may be an evidence for successive chlorine substitution of CHBr<sub>3</sub> in deeper and older water masses.</p></div>
]]></content:encoded><description>Seawater concentrations and distributions of brominated very short-lived substances (BrVSLS), including bromoform (CHBr3), dibromomethane (CH2Br2), bromodichloromethane (CHBrCl2), chlorodibromomethane (CHClBr2), were measured in the upper water column (5–750 m) in the eastern Pacific. Inorganic nutrient, pigment concentrations, and picoplankton cell counts were measured to determine biogeochemical factors that affect the production and distribution of these BrVSLS. Elevated concentrations of BrVSLS were observed in coastal and tropical seawater. Concentration maxima for CHBr3, CH2Br2, and CHClBr2 were observed below the mixed layer, near the subsurface chlorophyll a maxima, which suggest BrVSLS production may be related to photosynthetic biomass production. Our results also suggest that heterotrophic bacteria may also contribute to CH2Br2 and CHBrCl2 production in the water column. The maximum CHBrCl2 concentration was observed at a depth much deeper than the euphotic zone, which suggests sources other than photosynthetic biomass. Elevated CHBrCl2 concentrations in deeper waters were coincident with elevated CHCl3 concentrations, which may be an evidence for successive chlorine substitution of CHBr3 in deeper and older water masses.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20171" xmlns="http://purl.org/rss/1.0/"><title>Two modes of sea-ice gravity drainage: A parameterization for large-scale modeling</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20171</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Two modes of sea-ice gravity drainage: A parameterization for large-scale modeling</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Adrian K. Turner, Elizabeth C. Hunke, Cecilia M. Bitz</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-07T14:52:45.897295-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20171</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20171</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20171</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20171-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We present a new one-dimensional parameterization of gravity drainage implemented in an all-new thermodynamic component of the Los Alamos Sea Ice Model (CICE), based on mushy layer theory. We solve a set of coupled, nonlinear equations for sea-ice temperature (enthalpy) and salinity using an implicit Jacobian-free Newton-Krylov method. Time resolved observations of gravity drainage show two modes of desalination during growth. Rapid drainage occurs in a thin region just above the ice/ocean interface, while slower drainage occurs throughout the ice. Parameterizations are designed to represent each of these modes and work simultaneously. Near the interface, desalination occurs primarily via the fast drainage, while slow drainage continues to desalinate ice above the interface. The rapid desalination is convectively driven and is parameterized based on a consideration of flow driven upward within the mush and downward in chimneys, modified by the Rayleigh number. The slow desalination is represented as a simple relaxation of bulk salinity to a value based on a critical porosity for sea-ice permeability. It is shown that these parameterizations can adequately reproduce observational data from laboratory experiments and field measurements.</p></div>]]></content:encoded><description>We present a new one-dimensional parameterization of gravity drainage implemented in an all-new thermodynamic component of the Los Alamos Sea Ice Model (CICE), based on mushy layer theory. We solve a set of coupled, nonlinear equations for sea-ice temperature (enthalpy) and salinity using an implicit Jacobian-free Newton-Krylov method. Time resolved observations of gravity drainage show two modes of desalination during growth. Rapid drainage occurs in a thin region just above the ice/ocean interface, while slower drainage occurs throughout the ice. Parameterizations are designed to represent each of these modes and work simultaneously. Near the interface, desalination occurs primarily via the fast drainage, while slow drainage continues to desalinate ice above the interface. The rapid desalination is convectively driven and is parameterized based on a consideration of flow driven upward within the mush and downward in chimneys, modified by the Rayleigh number. The slow desalination is represented as a simple relaxation of bulk salinity to a value based on a critical porosity for sea-ice permeability. It is shown that these parameterizations can adequately reproduce observational data from laboratory experiments and field measurements.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20182" xmlns="http://purl.org/rss/1.0/"><title>Relationships between inherent optical properties and the depth of penetration of solar radiation in optically complex coastal waters</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20182</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Relationships between inherent optical properties and the depth of penetration of solar radiation in optically complex coastal waters</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Alex Cunningham, Leanne Ramage, David McKee</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-07T14:36:05.97878-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20182</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20182</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20182</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The attenuation of downward planar irradiance can be quantified by 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20182/asset/equation/jgrc20182-math-0001.gif?v=1&amp;t=hi5l2okp&amp;s=3ecd332eb3e8a10dadb67765e666154a0948791e" class="inlineGraphic"/>, the diffuse attenuation coefficient calculated from the surface to the depth where the irradiance <em>E<sub>d</sub></em> at wavelength <em>λ</em> falls to 10% of its surface value. Theoretical studies by Gordon (1989) and Lee et al. (2005a) suggest that 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20182/asset/equation/jgrc20182-math-0002.gif?v=1&amp;t=hi5l2okq&amp;s=34953c99526f274af8b80d2dd240ad865a6170de" class="inlineGraphic"/>can be derived from the absorption coefficient, <em>a</em>(<em>λ</em>) and the backscattering coefficient, <em>b<sub>b</sub></em>(<em>λ</em>), using equations incorporating either the solar zenith angle (<em>θ<sub>a</sub></em>) or the subsurface distribution function (<em>D</em><sub>0</sub>) and empirical coefficients derived by radiative transfer modeling. These results have not, however, been validated against in situ measurements. We have therefore assessed the performance of both models using measurements of <em>a</em>(<em>λ</em>), <em>b<sub>b</sub></em>(<em>λ</em>), and 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20182/asset/equation/jgrc20182-math-0003.gif?v=1&amp;t=hi5l2oks&amp;s=dc9aa2845aa716b85b69a58efcda6dfb2606b143" class="inlineGraphic"/> for 100 stations in UK coastal waters. Best results were obtained from the Lee et al. (2005a) model, for which over 90% of the predicted 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20182/asset/equation/jgrc20182-math-0004.gif?v=1&amp;t=hi5l2okt&amp;s=007bd324c1172676a7d9c1b648e0ad1978d9d2e9" class="inlineGraphic"/> values in the 440 nm to 665 nm range were within ±0.1 m<sup>−1</sup> of those measured in situ. A strong linear relationship (<em>R</em><sup>2</sup>&gt; 0.95, mean relative difference 5.4%) was found between 
<img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20182/asset/equation/jgrc20182-math-0005.gif?v=1&amp;t=hi5l2okt&amp;s=34a215f48c9b03f82ad6af121383129c9e2faed8" class="inlineGraphic"/> at 490 nm and the reciprocal of the depth of the midpoint of the euphotic zone (<em>z</em><sub>10%</sub>, PAR). This allowed (<em>z</em><sub>10%</sub>, PAR) to be predicted from measured values of <em>a</em>(490 nm), <em>b<sub>b</sub></em>(490 nm) and <em>θ<sub>a</sub></em>, using the Lee et al. model as an intermediate step, with an RMS error of 1.25 m over the 2.5–25.0 m range covered by our data set.</p></div>
]]></content:encoded><description>The attenuation of downward planar irradiance can be quantified by 
K¯d(E10%,λ), the diffuse attenuation coefficient calculated from the surface to the depth where the irradiance Ed at wavelength λ falls to 10% of its surface value. Theoretical studies by Gordon (1989) and Lee et al. (2005a) suggest that 
K¯d(E10%,λ)can be derived from the absorption coefficient, a(λ) and the backscattering coefficient, bb(λ), using equations incorporating either the solar zenith angle (θa) or the subsurface distribution function (D0) and empirical coefficients derived by radiative transfer modeling. These results have not, however, been validated against in situ measurements. We have therefore assessed the performance of both models using measurements of a(λ), bb(λ), and 
K¯d(E10%,λ) for 100 stations in UK coastal waters. Best results were obtained from the Lee et al. (2005a) model, for which over 90% of the predicted 
K¯d(E10%,λ) values in the 440 nm to 665 nm range were within ±0.1 m−1 of those measured in situ. A strong linear relationship (R2&gt; 0.95, mean relative difference 5.4%) was found between 
K¯d(E10%) at 490 nm and the reciprocal of the depth of the midpoint of the euphotic zone (z10%, PAR). This allowed (z10%, PAR) to be predicted from measured values of a(490 nm), bb(490 nm) and θa, using the Lee et al. model as an intermediate step, with an RMS error of 1.25 m over the 2.5–25.0 m range covered by our data set.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20172" xmlns="http://purl.org/rss/1.0/"><title>Spatio-temporal distribution, along-channel transport, and post-riverflood recovery of salinity in the Guadalquivir estuary (SW Spain)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20172</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Spatio-temporal distribution, along-channel transport, and post-riverflood recovery of salinity in the Guadalquivir estuary (SW Spain)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">M. Díez-Minguito, E. Contreras, M. J. Polo, M. A. Losada</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-03T14:55:32.036294-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20172</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20172</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20172</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">n/a</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20172-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This paper presents an experimental analysis of the salinity distribution, the salt balance, and the variation of the saline intrusion in comparison to the freshwater discharge in the Guadalquivir estuary, which is a mesotidal system regulated and normally subjected to extremely low river flows. In such low-flow conditions, it is positive, well-mixed, and tidally dominated. The estuary is also characterized by a nonstationary, effective longitudinal dispersion coefficient, whose probability density becomes increasingly narrower and whose mean value is higher further upstream. The tidal-averaged salt flux is controlled by the following mechanisms (in order of importance): the nontidal transport, the Stokes transport, and the tidal pumping induced by the covariance between the current and salinity. These three factors account for more than 98<em>%</em> of the flux variation. In high river-flow conditions, the subtidal response and recovery of the estuary to changes in the river flow is analyzed. The increase in the tidal-averaged salinity during the first 2 weeks of the post-riverflood recovery in the middle and upper sections of the estuary is found to be linear in time. During that time, the celerity of the salt intrusion front was 4cm/s. The 2 psu isohaline salt intrusion <em>X</em><sub>2</sub> exhibits a complex dependence on the river flow <em>Q</em><sub><em>d</em></sub>, including the effects of human interventions in the estuary. Three regimes are identified for the intrusion: <em>X</em><sub>2</sub>=57.0± 2.1km for discharges of less than 20m <sup>3</sup>/s, <em>X</em><sub>2</sub> proportional to <img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20172/asset/equation/jgrc20172-math-0001.gif?v=1&amp;t=hi5l2ol3&amp;s=10a5114588310b49ae7a65c297abc4e3bc8abf17" class="inlineGraphic"/> between 20 and 1000m <sup>3</sup>/s, and <em>X</em><sub>2</sub>proportional to <img alt="inline image" src="http://onlinelibrary.wiley.com/store/10.1002/jgrc.20172/asset/equation/jgrc20172-math-0002.gif?v=1&amp;t=hi5l2ol3&amp;s=9df257a150d912e735ed2129a492bade83b92e58" class="inlineGraphic"/>for larger discharges.</p></div>]]></content:encoded><description>This paper presents an experimental analysis of the salinity distribution, the salt balance, and the variation of the saline intrusion in comparison to the freshwater discharge in the Guadalquivir estuary, which is a mesotidal system regulated and normally subjected to extremely low river flows. In such low-flow conditions, it is positive, well-mixed, and tidally dominated. The estuary is also characterized by a nonstationary, effective longitudinal dispersion coefficient, whose probability density becomes increasingly narrower and whose mean value is higher further upstream. The tidal-averaged salt flux is controlled by the following mechanisms (in order of importance): the nontidal transport, the Stokes transport, and the tidal pumping induced by the covariance between the current and salinity. These three factors account for more than 98% of the flux variation. In high river-flow conditions, the subtidal response and recovery of the estuary to changes in the river flow is analyzed. The increase in the tidal-averaged salinity during the first 2 weeks of the post-riverflood recovery in the middle and upper sections of the estuary is found to be linear in time. During that time, the celerity of the salt intrusion front was 4cm/s. The 2 psu isohaline salt intrusion X2 exhibits a complex dependence on the river flow Qd, including the effects of human interventions in the estuary. Three regimes are identified for the intrusion: X2=57.0± 2.1km for discharges of less than 20m 3/s, X2 proportional to Qd−0.428±0.016 between 20 and 1000m 3/s, and X2proportional to Qd−1.0±0.5for larger discharges.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20063" xmlns="http://purl.org/rss/1.0/"><title>Export of nutrients from the Arctic Ocean</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20063</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Export of nutrients from the Arctic Ocean</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sinhué Torres-Valdés, Takamasa Tsubouchi, Sheldon Bacon, Alberto C. Naveira-Garabato, Richards Sanders, Fiona A. McLaughlin, Brian Petrie, Gerhard Kattner, Kumiko Azetsu-Scott, Terry E. Whitledge</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T09:20:45.11361-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20063</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20063</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20063</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1625</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1644</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This study provides the first physically based mass-balanced transport estimates of dissolved inorganic nutrients (nitrate, phosphate, and silicate) for the Arctic Ocean. Using an inverse model-generated velocity field in combination with a quasi-synoptic assemblage of hydrographic and hydrochemical data, we quantify nutrient transports across the main Arctic Ocean gateways: Davis Strait, Fram Strait, the Barents Sea Opening (BSO), and Bering Strait. We found that the major exports of all three nutrients occur via Davis Strait. Transports associated with the East Greenland Current are almost balanced by transports associated with the West Spitsbergen Current. The most important imports of nitrate and phosphate to the Arctic occur via the BSO, and the most important import of silicate occurs via Bering Strait. Oceanic budgets show that statistically robust net silicate and phosphate exports exist, while the net nitrate flux is zero, within the uncertainty limits. The Arctic Ocean is a net exporter of silicate (−15.7 ± 3.2 kmol s<sup>−1</sup>) and phosphate (−1.0 ± 0.3 kmol s<sup>−1</sup>; net ± 1 standard error) to the North Atlantic. The export of excess phosphate (relative to nitrate) from the Arctic, calculated at −1.1 ± 0.3 kmol s<sup>−1</sup>, is almost twice as large as previously estimated. Net transports of silicate and phosphate from the Arctic Ocean provide 12% and 90%, respectively, of the net southward fluxes estimated at 47<em>°</em>N in the North Atlantic. Additional sources of nutrients that may offset nutrient imbalances are explored, and the relevance and the pathway of nutrient transports to the North Atlantic are discussed.</p></div>]]></content:encoded><description>
This study provides the first physically based mass-balanced transport estimates of dissolved inorganic nutrients (nitrate, phosphate, and silicate) for the Arctic Ocean. Using an inverse model-generated velocity field in combination with a quasi-synoptic assemblage of hydrographic and hydrochemical data, we quantify nutrient transports across the main Arctic Ocean gateways: Davis Strait, Fram Strait, the Barents Sea Opening (BSO), and Bering Strait. We found that the major exports of all three nutrients occur via Davis Strait. Transports associated with the East Greenland Current are almost balanced by transports associated with the West Spitsbergen Current. The most important imports of nitrate and phosphate to the Arctic occur via the BSO, and the most important import of silicate occurs via Bering Strait. Oceanic budgets show that statistically robust net silicate and phosphate exports exist, while the net nitrate flux is zero, within the uncertainty limits. The Arctic Ocean is a net exporter of silicate (−15.7 ± 3.2 kmol s−1) and phosphate (−1.0 ± 0.3 kmol s−1; net ± 1 standard error) to the North Atlantic. The export of excess phosphate (relative to nitrate) from the Arctic, calculated at −1.1 ± 0.3 kmol s−1, is almost twice as large as previously estimated. Net transports of silicate and phosphate from the Arctic Ocean provide 12% and 90%, respectively, of the net southward fluxes estimated at 47°N in the North Atlantic. Additional sources of nutrients that may offset nutrient imbalances are explored, and the relevance and the pathway of nutrient transports to the North Atlantic are discussed.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20107" xmlns="http://purl.org/rss/1.0/"><title>Increased CO2 outgassing in February-May 2010 in the tropical Atlantic following the 2009 Pacific El Niño</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20107</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Increased CO2 outgassing in February-May 2010 in the tropical Atlantic following the 2009 Pacific El Niño</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Nathalie Lefèvre, Guy Caniaux, Serge Janicot, Abdou Karim Gueye</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T09:21:19.146437-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20107</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20107</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20107</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1645</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1657</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20107-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The fugacity of CO<sub>2</sub> (fCO<sub>2</sub>) has been measured underway during the voyages of a merchant ship sailing from France to Brazil since 2008. High fCO<sub>2</sub> values are observed in 2010, between approximately 8°S and 8°N, and are particularly pronounced in boreal spring. These high values are explained by the anomalous situation occurring in the tropical Atlantic in 2010 after the 2009 El Niño in the Pacific. The weakening of the trade winds during the El Niño event contributes to an increase of sea surface temperatures in the tropical Atlantic and a northward shift of the intertropical convergence zone. The anomalous position of the intertropical convergence zone is accompanied by reduced precipitation in boreal spring and hence a higher than usual sea surface salinity. The year 2010 is also characterized by a strong positive Atlantic multidecadal oscillation index and a negative North Atlantic oscillation index that contribute to the tropical Atlantic warming. Positive anomalies of both surface temperature and salinity cause an increase of surface CO<sub>2</sub>, leading to a stronger outgassing of CO<sub>2</sub> in 2010 compared with 2009 and 2011. The main factor responsible for the CO<sub>2</sub> anomalies is the Pacific El Niño teleconnection. The Atlantic multidecadal oscillation index also contributes in the northern hemisphere, and the role of the North Atlantic oscillation is negligible.</p></div>]]></content:encoded><description>
The fugacity of CO2 (fCO2) has been measured underway during the voyages of a merchant ship sailing from France to Brazil since 2008. High fCO2 values are observed in 2010, between approximately 8°S and 8°N, and are particularly pronounced in boreal spring. These high values are explained by the anomalous situation occurring in the tropical Atlantic in 2010 after the 2009 El Niño in the Pacific. The weakening of the trade winds during the El Niño event contributes to an increase of sea surface temperatures in the tropical Atlantic and a northward shift of the intertropical convergence zone. The anomalous position of the intertropical convergence zone is accompanied by reduced precipitation in boreal spring and hence a higher than usual sea surface salinity. The year 2010 is also characterized by a strong positive Atlantic multidecadal oscillation index and a negative North Atlantic oscillation index that contribute to the tropical Atlantic warming. Positive anomalies of both surface temperature and salinity cause an increase of surface CO2, leading to a stronger outgassing of CO2 in 2010 compared with 2009 and 2011. The main factor responsible for the CO2 anomalies is the Pacific El Niño teleconnection. The Atlantic multidecadal oscillation index also contributes in the northern hemisphere, and the role of the North Atlantic oscillation is negligible.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20122" xmlns="http://purl.org/rss/1.0/"><title>MIMOC: A global monthly isopycnal upper-ocean climatology with mixed layers</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20122</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">MIMOC: A global monthly isopycnal upper-ocean climatology with mixed layers</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sunke Schmidtko, Gregory C. Johnson, John M. Lyman</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T10:33:39.102598-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20122</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20122</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20122</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1658</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1672</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A monthly, isopycnal/mixed-layer ocean climatology (MIMOC), global from 0 to 1950 dbar, is compared with other monthly ocean climatologies. All available quality-controlled profiles of temperature (<em>T</em>) and salinity (<em>S</em>) versus pressure (<em>P</em>) collected by conductivity-temperature-depth (CTD) instruments from the Argo Program, Ice-Tethered Profilers, and archived in the World Ocean Database are used. MIMOC provides maps of mixed layer properties (conservative temperature, <em>Θ</em>, absolute salinity, <em>S<sub>A</sub></em>, and maximum <em>P</em>) as well as maps of interior ocean properties (<em>Θ</em>, <em>S<sub>A</sub></em>, and <em>P</em>) to 1950 dbar on isopycnal surfaces. A third product merges the two onto a pressure grid spanning the upper 1950 dbar, adding more familiar potential temperature (<em>θ</em>) and practical salinity (<em>S</em>) maps. All maps are at monthly 0.5° × 0.5° resolution, spanning from 80°S to 90°N. Objective mapping routines used and described here incorporate an isobath-following component using a “Fast Marching” algorithm, as well as front-sharpening components in both the mixed layer and on interior isopycnals. Recent data are emphasized in the mapping. The goal is to compute a climatology that looks as much as possible like synoptic surveys sampled circa 2007–2011 during all phases of the seasonal cycle, minimizing transient eddy and wave signatures. MIMOC preserves a surface mixed layer, minimizes both diapycnal and isopycnal smoothing of <em>θ-S</em>, as well as preserves density structure in the vertical (pycnoclines and pycnostads) and the horizontal (fronts and their associated currents). It is statically stable and resolves water mass features, fronts, and currents with a high level of detail and fidelity.</p></div>]]></content:encoded><description>A monthly, isopycnal/mixed-layer ocean climatology (MIMOC), global from 0 to 1950 dbar, is compared with other monthly ocean climatologies. All available quality-controlled profiles of temperature (T) and salinity (S) versus pressure (P) collected by conductivity-temperature-depth (CTD) instruments from the Argo Program, Ice-Tethered Profilers, and archived in the World Ocean Database are used. MIMOC provides maps of mixed layer properties (conservative temperature, Θ, absolute salinity, SA, and maximum P) as well as maps of interior ocean properties (Θ, SA, and P) to 1950 dbar on isopycnal surfaces. A third product merges the two onto a pressure grid spanning the upper 1950 dbar, adding more familiar potential temperature (θ) and practical salinity (S) maps. All maps are at monthly 0.5° × 0.5° resolution, spanning from 80°S to 90°N. Objective mapping routines used and described here incorporate an isobath-following component using a “Fast Marching” algorithm, as well as front-sharpening components in both the mixed layer and on interior isopycnals. Recent data are emphasized in the mapping. The goal is to compute a climatology that looks as much as possible like synoptic surveys sampled circa 2007–2011 during all phases of the seasonal cycle, minimizing transient eddy and wave signatures. MIMOC preserves a surface mixed layer, minimizes both diapycnal and isopycnal smoothing of θ-S, as well as preserves density structure in the vertical (pycnoclines and pycnostads) and the horizontal (fronts and their associated currents). It is statically stable and resolves water mass features, fronts, and currents with a high level of detail and fidelity.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20127" xmlns="http://purl.org/rss/1.0/"><title>Seasonal to decadal variability of Arctic Ocean heat content: A model-based analysis and implications for autonomous observing systems</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20127</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seasonal to decadal variability of Arctic Ocean heat content: A model-based analysis and implications for autonomous observing systems</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Camille Lique, Michael Steele</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T09:56:02.256929-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20127</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20127</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20127</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1673</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1695</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20127-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A high-resolution global ocean/sea ice model is used to investigate the modes of Arctic Ocean heat content variability for the period 1968–2007. A rotated empirical orthogonal function analysis is performed on the monthly mean vertically integrated heat content to investigate the mechanisms governing its spatiotemporal variations. In the model, 28% of the heat content variability is driven by the seasonal and interannual fluctuations of the atmospheric heat flux in the seasonally ice free regions. The heat flux variability associated with Atlantic Water advected through Fram Strait drives 31% of the heat content variability. Changes of temperature and circulation drive Fram Strait heat transport variability, and these two effects project on different modes and thus drive heat content variations in different parts of the Eurasian Basin. A second branch of Atlantic Water is modified in the Barents Sea and the variations of the heat flux associated with the Barents Sea water branch penetrating the deep Arctic yield heat content variations in the Eurasian Basin. The effect of the Bering Strait heat flux variations remains limited to the Chukchi Sea. Autonomous observing system may be able to capture the Arctic heat content variability. Sea surface temperature satellite observations combined with temperature profiles of the top 800 m in the deep Arctic covered by sea ice are sufficient to capture most of the variability signal. The results emphasize the crucial need for measurements in the Eurasian Basin.</p></div>]]></content:encoded><description>A high-resolution global ocean/sea ice model is used to investigate the modes of Arctic Ocean heat content variability for the period 1968–2007. A rotated empirical orthogonal function analysis is performed on the monthly mean vertically integrated heat content to investigate the mechanisms governing its spatiotemporal variations. In the model, 28% of the heat content variability is driven by the seasonal and interannual fluctuations of the atmospheric heat flux in the seasonally ice free regions. The heat flux variability associated with Atlantic Water advected through Fram Strait drives 31% of the heat content variability. Changes of temperature and circulation drive Fram Strait heat transport variability, and these two effects project on different modes and thus drive heat content variations in different parts of the Eurasian Basin. A second branch of Atlantic Water is modified in the Barents Sea and the variations of the heat flux associated with the Barents Sea water branch penetrating the deep Arctic yield heat content variations in the Eurasian Basin. The effect of the Bering Strait heat flux variations remains limited to the Chukchi Sea. Autonomous observing system may be able to capture the Arctic heat content variability. Sea surface temperature satellite observations combined with temperature profiles of the top 800 m in the deep Arctic covered by sea ice are sufficient to capture most of the variability signal. The results emphasize the crucial need for measurements in the Eurasian Basin.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20139" xmlns="http://purl.org/rss/1.0/"><title>Evaluation and optimization of bio-optical inversion algorithms for remote sensing of Lake Superior's optical properties</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20139</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Evaluation and optimization of bio-optical inversion algorithms for remote sensing of Lake Superior's optical properties</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Colleen B. Mouw, Haidi Chen, Galen A. McKinley, Steven Effler, David O'Donnell, Mary Gail Perkins, Chris Strait</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T11:01:08.554399-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20139</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20139</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20139</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1696</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1714</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20139-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Satellite remote sensing offers one of the best spatial and temporal observational approaches. However, well-validated satellite imagery has remained elusive for Lake Superior. Lake Superior's optical properties are highly influenced by colored dissolved organic matter (CDOM), which has hindered the retrieval of chlorophyll concentration through band-ratio algorithms. This study evaluated seven existing inversion algorithms. The top-performing inversion algorithm was tuned to a Lake Superior optical data set and applied to satellite imagery. The retrieval of chlorophyll concentration via inversion algorithms was not possible due to errors in derived CDOM absorption being greater than phytoplankton absorption values and the very small contribution of phytoplankton absorption to the overall absorption budget. However, the retrieval of absorption due to CDOM from satellite imagery was encouraging. To ensure that the best satellite remotely sensed reflectance estimates were used in the retrieval of absorption due to CDOM, several atmospheric correction schemes were evaluated. The absorption due to CDOM was greatest in the western arm of Lake Superior and near river mouths and decreased with distance offshore. The absorption due to CDOM had a bimodal distribution over the annual cycle with the greatest peak in fall and a smaller peak in spring.</p></div>]]></content:encoded><description>Satellite remote sensing offers one of the best spatial and temporal observational approaches. However, well-validated satellite imagery has remained elusive for Lake Superior. Lake Superior's optical properties are highly influenced by colored dissolved organic matter (CDOM), which has hindered the retrieval of chlorophyll concentration through band-ratio algorithms. This study evaluated seven existing inversion algorithms. The top-performing inversion algorithm was tuned to a Lake Superior optical data set and applied to satellite imagery. The retrieval of chlorophyll concentration via inversion algorithms was not possible due to errors in derived CDOM absorption being greater than phytoplankton absorption values and the very small contribution of phytoplankton absorption to the overall absorption budget. However, the retrieval of absorption due to CDOM from satellite imagery was encouraging. To ensure that the best satellite remotely sensed reflectance estimates were used in the retrieval of absorption due to CDOM, several atmospheric correction schemes were evaluated. The absorption due to CDOM was greatest in the western arm of Lake Superior and near river mouths and decreased with distance offshore. The absorption due to CDOM had a bimodal distribution over the annual cycle with the greatest peak in fall and a smaller peak in spring.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20145" xmlns="http://purl.org/rss/1.0/"><title>Characteristics of interfacial signatures on a wind-driven gravity-capillary wave</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20145</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Characteristics of interfacial signatures on a wind-driven gravity-capillary wave</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Wu-ting Tsai, Shi-ming Chen, Guan-hung Lu, Christoph S. Garbe</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T10:08:28.622341-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20145</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20145</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20145</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1715</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1735</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20145-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Direct numerical simulation of a wind-driven gravity-capillary wave and the underlying turbulent flow is conducted to identify the characteristic signatures of various surface parameters, including temperature, gas flux, velocities, and roughness, and to reveal the impacts of the nonbreaking surface waves on these surface flow and tracer parameters. Three characteristic surface signatures and the corresponding flow processes are identified: the carrier gravity wave, the parasitic capillary wavelets, and the elongated streaks. The elongated streaks are induced by both the coherent streamwise vortices formed within the turbulent shear layer and the Langmuir circulations arising from nonlinear interaction between the carrier gravity wave and the drift current. All three surface signatures can be observed in the distributions of various quantities, although some are more apparent than the others. Image-processing techniques, employing empirical mode decomposition and phase averaging, are developed to decompose the distinct signatures thus to quantify the contributions by the responsible flow processes. It is found that elongated streaks prevail the distribution of surface temperature and gas flux, indicating that Langmuir cells and the coherent eddies contribute to the major interfacial heat and gas transport. These eddies also induced strong cross-stream velocity divergence at the water surface, which exhibits resemblant elongated distribution as that of gas flux (correlation coefficient ≈ 0.6). High correlation between the surface distributions of temperature and gas flux is observed (correlation coefficient ≈ 0.8 to 0.9), suggesting that the spatial and temporal distribution of surface temperature is a good proxy tracer of interfacial gas transfer.</p></div>]]></content:encoded><description>Direct numerical simulation of a wind-driven gravity-capillary wave and the underlying turbulent flow is conducted to identify the characteristic signatures of various surface parameters, including temperature, gas flux, velocities, and roughness, and to reveal the impacts of the nonbreaking surface waves on these surface flow and tracer parameters. Three characteristic surface signatures and the corresponding flow processes are identified: the carrier gravity wave, the parasitic capillary wavelets, and the elongated streaks. The elongated streaks are induced by both the coherent streamwise vortices formed within the turbulent shear layer and the Langmuir circulations arising from nonlinear interaction between the carrier gravity wave and the drift current. All three surface signatures can be observed in the distributions of various quantities, although some are more apparent than the others. Image-processing techniques, employing empirical mode decomposition and phase averaging, are developed to decompose the distinct signatures thus to quantify the contributions by the responsible flow processes. It is found that elongated streaks prevail the distribution of surface temperature and gas flux, indicating that Langmuir cells and the coherent eddies contribute to the major interfacial heat and gas transport. These eddies also induced strong cross-stream velocity divergence at the water surface, which exhibits resemblant elongated distribution as that of gas flux (correlation coefficient ≈ 0.6). High correlation between the surface distributions of temperature and gas flux is observed (correlation coefficient ≈ 0.8 to 0.9), suggesting that the spatial and temporal distribution of surface temperature is a good proxy tracer of interfacial gas transfer.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20148" xmlns="http://purl.org/rss/1.0/"><title>Particle dynamics of the Changjiang Estuary and adjacent coastal region determined by natural particle-reactive radionuclides (7Be, 210Pb, and 234Th)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20148</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Particle dynamics of the Changjiang Estuary and adjacent coastal region determined by natural particle-reactive radionuclides (7Be, 210Pb, and 234Th)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Dekun Huang, Jinzhou Du, Willard S. Moore, Jing Zhang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T10:28:26.091849-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20148</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20148</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20148</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1736</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1748</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The timescale of transport processes in estuarine and coastal regions can be evaluated using natural radionuclides with different half-lives. The distribution patterns of <sup>7</sup>Be, <sup>210</sup>Pb, and <sup>234</sup>Th in the water column from April to July 2008 were used to calculate the removal and residence times in the Changjiang Estuary. The results showed that the maximum particulate activities of <sup>7</sup>Be, <sup>210</sup>Pb, and <sup>234</sup>Th were observed approximately 150 km downstream (the turbidity maximum zone) of the freshwater end-number. The mean distribution coefficients (<em>K<sub>d</sub></em>, cm<sup>3</sup> g<sup>−1</sup>) of the high suspended particulate matter (SPM) group are higher than those of the lower-SPM group for <sup>7</sup>Be and <sup>210</sup>Pb; for <sup>234</sup>Th, the reverse is true. Based on a material balance in two-dimensional models of <sup>7</sup>Be, <sup>210</sup>Pb, and <sup>234</sup>Th in the Changjiang River mouth, the removal times of these nuclides were approximately 0.66–12, 1.6–21, and 1.2–5.4 days, respectively. The residence times increased toward the seaward side. In the coastal region, the removal times of <sup>7</sup>Be, <sup>210</sup>Pb, and <sup>234</sup>Th calculated by material balance in one-dimensional models were approximately 1.1–26, 1.2–27, and 0.70–23 days, respectively. Moreover, an enhanced resuspension process not only controlled the partitioning of <sup>7</sup>Be, <sup>210</sup>Pb, and <sup>234</sup>Th between the particulate and dissolved phases, but also, this process may play a dominant role in controlling the dynamic behavior of SPM in the water column compared with the advection input/output fluxes of the SPM in the river mouth areas. The removal and the resuspension fluxes were comparable in the estuary. Meanwhile, old composition (whose deposition into the seabed for a long time is enough for <sup>7</sup>Be to decay completely) occupied only a small part in the resuspended sediment during resuspension process.</p></div>]]></content:encoded><description>
The timescale of transport processes in estuarine and coastal regions can be evaluated using natural radionuclides with different half-lives. The distribution patterns of 7Be, 210Pb, and 234Th in the water column from April to July 2008 were used to calculate the removal and residence times in the Changjiang Estuary. The results showed that the maximum particulate activities of 7Be, 210Pb, and 234Th were observed approximately 150 km downstream (the turbidity maximum zone) of the freshwater end-number. The mean distribution coefficients (Kd, cm3 g−1) of the high suspended particulate matter (SPM) group are higher than those of the lower-SPM group for 7Be and 210Pb; for 234Th, the reverse is true. Based on a material balance in two-dimensional models of 7Be, 210Pb, and 234Th in the Changjiang River mouth, the removal times of these nuclides were approximately 0.66–12, 1.6–21, and 1.2–5.4 days, respectively. The residence times increased toward the seaward side. In the coastal region, the removal times of 7Be, 210Pb, and 234Th calculated by material balance in one-dimensional models were approximately 1.1–26, 1.2–27, and 0.70–23 days, respectively. Moreover, an enhanced resuspension process not only controlled the partitioning of 7Be, 210Pb, and 234Th between the particulate and dissolved phases, but also, this process may play a dominant role in controlling the dynamic behavior of SPM in the water column compared with the advection input/output fluxes of the SPM in the river mouth areas. The removal and the resuspension fluxes were comparable in the estuary. Meanwhile, old composition (whose deposition into the seabed for a long time is enough for 7Be to decay completely) occupied only a small part in the resuspended sediment during resuspension process.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20154" xmlns="http://purl.org/rss/1.0/"><title>Dynamic response of surface water-groundwater exchange to currents, tides, and waves in a shallow estuary</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20154</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Dynamic response of surface water-groundwater exchange to currents, tides, and waves in a shallow estuary</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Audrey H. Sawyer, Fengyan Shi, James T. Kirby, Holly A. Michael</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-03T11:04:48.391032-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20154</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20154</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20154</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1749</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1758</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20154-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> In shallow, fetch-limited estuaries, variations in current and wave energy promote heterogeneous surface water-groundwater mixing (benthic exchange), which influences biogeochemical activity. Here, we characterize heterogeneity in benthic exchange within the subtidal zone of the Delaware Inland Bays by linking hydrodynamic circulation models with mathematical solutions for benthic exchange forced by current-bedform interactions, tides, and waves. Benthic fluxes oscillate over tidal cycles as fluctuating water depths alter fluid interactions with the bed. Maximum current-driven fluxes (~1–10 cm/d) occur in channels with strong tidal currents. Maximum wave-driven fluxes (~1–10 cm/d) occur in downwind shoals. During high-energy storms, simulated wave pumping rates increase by orders of magnitude, demonstrating the importance of storms in solute transfer through the benthic layer. Under moderate wind conditions (~5 m/s), integrated benthic exchange rates due to wave, current, and tidal pumping are each ~1–10 m<sup>3</sup>/s, on the order of fluid contributions from runoff and fresh groundwater discharge to the estuary. Benthic exchange is thus a significant and dynamic component of an estuary's fluid budget that may influence estuarine geochemistry and ecology.</p></div>]]></content:encoded><description>In shallow, fetch-limited estuaries, variations in current and wave energy promote heterogeneous surface water-groundwater mixing (benthic exchange), which influences biogeochemical activity. Here, we characterize heterogeneity in benthic exchange within the subtidal zone of the Delaware Inland Bays by linking hydrodynamic circulation models with mathematical solutions for benthic exchange forced by current-bedform interactions, tides, and waves. Benthic fluxes oscillate over tidal cycles as fluctuating water depths alter fluid interactions with the bed. Maximum current-driven fluxes (~1–10 cm/d) occur in channels with strong tidal currents. Maximum wave-driven fluxes (~1–10 cm/d) occur in downwind shoals. During high-energy storms, simulated wave pumping rates increase by orders of magnitude, demonstrating the importance of storms in solute transfer through the benthic layer. Under moderate wind conditions (~5 m/s), integrated benthic exchange rates due to wave, current, and tidal pumping are each ~1–10 m3/s, on the order of fluid contributions from runoff and fresh groundwater discharge to the estuary. Benthic exchange is thus a significant and dynamic component of an estuary's fluid budget that may influence estuarine geochemistry and ecology.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20155" xmlns="http://purl.org/rss/1.0/"><title>A three-dimensional eddy census of a high-resolution global ocean simulation</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20155</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A three-dimensional eddy census of a high-resolution global ocean simulation</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mark R. Petersen, Sean J. Williams, Mathew E. Maltrud, Matthew W. Hecht, Bernd Hamann</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-04T13:23:33.833557-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20155</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20155</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20155</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1759</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1774</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20155-para-0002" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A three-dimensional eddy census data set was obtained from a global ocean simulation with one-tenth degree resolution and a duration of 7 years. The census includes 6.7 million eddies in daily data, which comprise 152,000 eddies tracked over their lifetimes, using a minimum lifetime cutoff of 28 days. Variables of interest include eddy diameter, thickness (vertical extent), minimum and maximum depth, location, rotational direction, lifetime, and translational speed. Distributions of these traits show a predominance of small, thin, short-lived, and slow eddies. Still, a significant number of eddies possess traits at the opposite extreme; thousands of eddies larger than 200 km in diameter appeared in daily data each year. A tracking algorithm found hundreds of eddies with lifetimes longer than 200 days. A third of the eddies are at least 1000 m tall and many penetrate the full depth of the water column. The Antarctic Circumpolar Current contains the thickest and highest density of eddies. Thick eddies are also common in the Gulf Stream, Kuroshio Current, and Agulhas ring pathway. The great majority of eddies extend all the way to the surface, confirming that eddy censuses from surface observations are a good proxy for the full-depth ocean. Correlations between variables show that larger-diameter eddies tend to be thicker and longer lived than small eddies.</p></div>]]></content:encoded><description>A three-dimensional eddy census data set was obtained from a global ocean simulation with one-tenth degree resolution and a duration of 7 years. The census includes 6.7 million eddies in daily data, which comprise 152,000 eddies tracked over their lifetimes, using a minimum lifetime cutoff of 28 days. Variables of interest include eddy diameter, thickness (vertical extent), minimum and maximum depth, location, rotational direction, lifetime, and translational speed. Distributions of these traits show a predominance of small, thin, short-lived, and slow eddies. Still, a significant number of eddies possess traits at the opposite extreme; thousands of eddies larger than 200 km in diameter appeared in daily data each year. A tracking algorithm found hundreds of eddies with lifetimes longer than 200 days. A third of the eddies are at least 1000 m tall and many penetrate the full depth of the water column. The Antarctic Circumpolar Current contains the thickest and highest density of eddies. Thick eddies are also common in the Gulf Stream, Kuroshio Current, and Agulhas ring pathway. The great majority of eddies extend all the way to the surface, confirming that eddy censuses from surface observations are a good proxy for the full-depth ocean. Correlations between variables show that larger-diameter eddies tend to be thicker and longer lived than small eddies.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20072" xmlns="http://purl.org/rss/1.0/"><title>Global teleconnections in the oceanic phosphorus cycle: Patterns, paths, and timescales</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20072</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Global teleconnections in the oceanic phosphorus cycle: Patterns, paths, and timescales</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mark Holzer, François W. Primeau</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-08T15:45:32.356626-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20072</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20072</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20072</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1775</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1796</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Nutrient transport and productivity teleconnections with the Southern Ocean are diagnosed in a data-assimilated circulation model coupled to a jointly optimized simple phosphorus cycling model. The North Atlantic has the strongest extratropical teleconnections with the Southern Ocean: phosphate (PO<sub>4</sub>) last utilized in the Southern Ocean sustains 29 ± 6% of the subpolar and 14 ± 6% of the subtropical, new production in the North Atlantic. A PO<sub>4</sub> path-density diagnostic shows that these teleconnections are mediated by thermocline paths and reveals that most paths to anywhere north of 40°S lie in the deep Pacific. Forcing nearly complete Southern-Ocean nutrient utilization increases the overall number of paths to anywhere north of 40°S, but reduces the number of paths from the Pacific to the North Atlantic by trapping nutrients in return paths to the Southern Ocean. At the same time, the mean export-to-uptake transit times to anywhere north of 40°S increase, while the mean transit times to the North Atlantic decrease. Correspondingly, the amount of North-Atlantic production sustained by Southern-Ocean export increases in spite of decreased total production in response to Southern-Ocean nutrient trapping. The distributions of export-to-uptake, export-to-surface, and surface-to-surface transit times are computed and summarized in terms of their mean transit times and their mean interior residence times. The combined particle and advective–diffusive transport of nutrients is characterized by broad, skewed transit-time distributions, which result in mean residence times much longer than the mean transit times, in turn much longer than the most probable transit times.</p></div>]]></content:encoded><description>
Nutrient transport and productivity teleconnections with the Southern Ocean are diagnosed in a data-assimilated circulation model coupled to a jointly optimized simple phosphorus cycling model. The North Atlantic has the strongest extratropical teleconnections with the Southern Ocean: phosphate (PO4) last utilized in the Southern Ocean sustains 29 ± 6% of the subpolar and 14 ± 6% of the subtropical, new production in the North Atlantic. A PO4 path-density diagnostic shows that these teleconnections are mediated by thermocline paths and reveals that most paths to anywhere north of 40°S lie in the deep Pacific. Forcing nearly complete Southern-Ocean nutrient utilization increases the overall number of paths to anywhere north of 40°S, but reduces the number of paths from the Pacific to the North Atlantic by trapping nutrients in return paths to the Southern Ocean. At the same time, the mean export-to-uptake transit times to anywhere north of 40°S increase, while the mean transit times to the North Atlantic decrease. Correspondingly, the amount of North-Atlantic production sustained by Southern-Ocean export increases in spite of decreased total production in response to Southern-Ocean nutrient trapping. The distributions of export-to-uptake, export-to-surface, and surface-to-surface transit times are computed and summarized in terms of their mean transit times and their mean interior residence times. The combined particle and advective–diffusive transport of nutrients is characterized by broad, skewed transit-time distributions, which result in mean residence times much longer than the mean transit times, in turn much longer than the most probable transit times.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20141" xmlns="http://purl.org/rss/1.0/"><title>A near-inertial mode observed within a Gulf Stream warm-core ring</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20141</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A near-inertial mode observed within a Gulf Stream warm-core ring</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Terrence M. Joyce, John M. Toole, Patrice Klein, Leif N. Thomas</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-08T16:20:36.540729-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20141</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20141</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20141</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1797</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1806</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20141-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Layering of ocean velocity “fine structure” has been coherently observed across the entire extent of a Gulf Stream warm-core ring using a shipboard acoustic Doppler current profiler system in September 2009 and independently sampled as the ring transited a moored array. Lines of constant velocity phase generally followed isopycnals as they deepened within the ring center. We also observed a clear separation of the vertical structure of the flows associated with the ring (of order 0.5 m/s) with the shorter (200 m) and less energetic (~0.2 m/s) flows of the velocity fine structure, which was further observed to rotate clockwise with increasing depth, consistent with downward propagating near-inertial waves (NIWs). Observations are consistent with a ring-scale NIW packet, probably wind forced, that shows enhanced NIW energy within the sloping pycnocline at depths of 300–700 m. Evidence of wind-forced NIWs within anticylonic eddies in a numerical simulation shows some similar features to our observations, which we try to understand physically with basic WKB-type wave/current dynamics along the lines of previously published work and a new calculation of NIW trapping within an isolated, baroclinic vortex.</p></div>]]></content:encoded><description>Layering of ocean velocity “fine structure” has been coherently observed across the entire extent of a Gulf Stream warm-core ring using a shipboard acoustic Doppler current profiler system in September 2009 and independently sampled as the ring transited a moored array. Lines of constant velocity phase generally followed isopycnals as they deepened within the ring center. We also observed a clear separation of the vertical structure of the flows associated with the ring (of order 0.5 m/s) with the shorter (200 m) and less energetic (~0.2 m/s) flows of the velocity fine structure, which was further observed to rotate clockwise with increasing depth, consistent with downward propagating near-inertial waves (NIWs). Observations are consistent with a ring-scale NIW packet, probably wind forced, that shows enhanced NIW energy within the sloping pycnocline at depths of 300–700 m. Evidence of wind-forced NIWs within anticylonic eddies in a numerical simulation shows some similar features to our observations, which we try to understand physically with basic WKB-type wave/current dynamics along the lines of previously published work and a new calculation of NIW trapping within an isolated, baroclinic vortex.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20095" xmlns="http://purl.org/rss/1.0/"><title>Air-sea and oceanic heat flux contributions to the heat budget of the northern Gulf of Alaska shelf</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20095</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Air-sea and oceanic heat flux contributions to the heat budget of the northern Gulf of Alaska shelf</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Markus A. Janout, Thomas J. Weingartner, Phyllis J. Stabeno</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-09T14:21:17.004229-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20095</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20095</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20095</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1807</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1820</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20095-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We constructed annual cycles of National Centers for Environmental Prediction air-sea fluxes and temporal oceanic heat content change from Seward Line hydrographic surveys to quantify the different contributions to the oceanic heat budget within the Alaska Coastal Current (ACC) on the northern Gulf of Alaska shelf. The deficit between air-sea fluxes and the temporal change in oceanic heat content throughout the cooling season (October–April) varies from ~40 to 110 W m<sup>−2</sup> and is balanced by ocean heat flux convergence. Cross-shelf heat flux convergence is insignificant on annual average, and the nearshore heat budget is likely entirely balanced by the ACC, which resupplies ~15%–50% of the heat removed by air-sea fluxes during the cooling season. Furthermore, we estimated spatial heat flux gradients and conclude that air-sea fluxes increase from east to west and from offshore to onshore. The cross-shore gradients are governed by wind speed gradients, likely due to ageostrophic nearshore wind events during the cooling season, while the along-shelf heat flux gradients are governed by the occurrence of low-pressure systems in the northern GOA that result in cold northerly winds over the northwestern GOA. These results underline the ACC's role as the dominant oceanic heat source to the northern GOA shelf and further imply an increased cooling rate of the ACC west of the Seward Line. Furthermore, our analysis showed that nearshore regions, particularly waters in the ACC, are subjected to stronger winter cooling than the middle and outer shelves.</p></div>]]></content:encoded><description>We constructed annual cycles of National Centers for Environmental Prediction air-sea fluxes and temporal oceanic heat content change from Seward Line hydrographic surveys to quantify the different contributions to the oceanic heat budget within the Alaska Coastal Current (ACC) on the northern Gulf of Alaska shelf. The deficit between air-sea fluxes and the temporal change in oceanic heat content throughout the cooling season (October–April) varies from ~40 to 110 W m−2 and is balanced by ocean heat flux convergence. Cross-shelf heat flux convergence is insignificant on annual average, and the nearshore heat budget is likely entirely balanced by the ACC, which resupplies ~15%–50% of the heat removed by air-sea fluxes during the cooling season. Furthermore, we estimated spatial heat flux gradients and conclude that air-sea fluxes increase from east to west and from offshore to onshore. The cross-shore gradients are governed by wind speed gradients, likely due to ageostrophic nearshore wind events during the cooling season, while the along-shelf heat flux gradients are governed by the occurrence of low-pressure systems in the northern GOA that result in cold northerly winds over the northwestern GOA. These results underline the ACC's role as the dominant oceanic heat source to the northern GOA shelf and further imply an increased cooling rate of the ACC west of the Seward Line. Furthermore, our analysis showed that nearshore regions, particularly waters in the ACC, are subjected to stronger winter cooling than the middle and outer shelves.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20109" xmlns="http://purl.org/rss/1.0/"><title>Optical properties of the Dead Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20109</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Optical properties of the Dead Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Emmanuel Boss, Hezi Gildor, Wayne Slade, Leonid Sokoletsky, Aharon Oren, James Loftin</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-09T13:48:46.459935-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20109</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20109</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20109</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1821</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1829</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20109-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The Dead Sea, located in the rift valley between Jordan and Israel, is a hypersaline lake, resulting in unique biogeochemistry and optical properties. In the spring of 2004 we conducted two days of physical and optical measurements in the lake. Because of the significant effect of dissolved salts on the optical properties of water, our analysis required a novel processing approach to obtain dissolved and total inherent optical properties from the measurements. In addition, we show that the lake's salinity can be estimated from measurements of hyper-spectral absorption or attenuation spectra in the red and infrared parts of the spectrum, using published values of specific absorption of dissolved NaCl, despite the fact that the lake's salt chemistry is complex. In situ observations demonstrated that the lake has a two-layer structure with a warm and more turbid layer at the top 20–30 m and a clearer colder layer below. Both the particulate and dissolved absorption are well approximated by exponentially decreasing functions with the spectral slope of the particulate absorption about half that of the dissolved fraction and consistent with other aquatic environments. Both have relatively low and similar magnitudes in the blue (O(0.15 m<sup>–1</sup>)). Mean particle size was observed to increase with depth, consistent with precipitating salt crystals (observed in past campaigns) shown here to play a major role in the lake's optical properties.</p></div>]]></content:encoded><description>The Dead Sea, located in the rift valley between Jordan and Israel, is a hypersaline lake, resulting in unique biogeochemistry and optical properties. In the spring of 2004 we conducted two days of physical and optical measurements in the lake. Because of the significant effect of dissolved salts on the optical properties of water, our analysis required a novel processing approach to obtain dissolved and total inherent optical properties from the measurements. In addition, we show that the lake's salinity can be estimated from measurements of hyper-spectral absorption or attenuation spectra in the red and infrared parts of the spectrum, using published values of specific absorption of dissolved NaCl, despite the fact that the lake's salt chemistry is complex. In situ observations demonstrated that the lake has a two-layer structure with a warm and more turbid layer at the top 20–30 m and a clearer colder layer below. Both the particulate and dissolved absorption are well approximated by exponentially decreasing functions with the spectral slope of the particulate absorption about half that of the dissolved fraction and consistent with other aquatic environments. Both have relatively low and similar magnitudes in the blue (O(0.15 m–1)). Mean particle size was observed to increase with depth, consistent with precipitating salt crystals (observed in past campaigns) shown here to play a major role in the lake's optical properties.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20135" xmlns="http://purl.org/rss/1.0/"><title>Assessment of Southern Ocean water mass circulation and characteristics in CMIP5 models: Historical bias and forcing response</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20135</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Assessment of Southern Ocean water mass circulation and characteristics in CMIP5 models: Historical bias and forcing response</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J.-B. Sallée, E. Shuckburgh, N. Bruneau, A. J. S. Meijers, T. J. Bracegirdle, Z. Wang, T. Roy</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-09T11:20:32.850715-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20135</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20135</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20135</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1830</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1844</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20135-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The ability of the models contributing to the fifth Coupled Models Intercomparison Project (CMIP5) to represent the Southern Ocean hydrological properties and its overturning is investigated in a water mass framework. Models have a consistent warm and light bias spread over the entire water column. The greatest bias occurs in the ventilated layers, which are volumetrically dominated by mode and intermediate layers. The ventilated layers have been observed to have a strong fingerprint of climate change and to impact climate by sequestrating a significant amount of heat and carbon dioxide. The mode water layer is poorly represented in the models and both mode and intermediate water have a significant fresh bias. Under increased radiative forcing, models simulate a warming and lightening of the entire water column, which is again greatest in the ventilated layers, highlighting the importance of these layers for propagating the climate signal into the deep ocean. While the intensity of the water mass overturning is relatively consistent between models, when compared to observation-based reconstructions, they exhibit a slightly larger rate of overturning at shallow to intermediate depths, and a slower rate of overturning deeper in the water column. Under increased radiative forcing, atmospheric fluxes increase the rate of simulated upper cell overturning, but this increase is counterbalanced by diapycnal fluxes, including mixed-layer horizontal mixing, and mostly vanishes.</p></div>]]></content:encoded><description>The ability of the models contributing to the fifth Coupled Models Intercomparison Project (CMIP5) to represent the Southern Ocean hydrological properties and its overturning is investigated in a water mass framework. Models have a consistent warm and light bias spread over the entire water column. The greatest bias occurs in the ventilated layers, which are volumetrically dominated by mode and intermediate layers. The ventilated layers have been observed to have a strong fingerprint of climate change and to impact climate by sequestrating a significant amount of heat and carbon dioxide. The mode water layer is poorly represented in the models and both mode and intermediate water have a significant fresh bias. Under increased radiative forcing, models simulate a warming and lightening of the entire water column, which is again greatest in the ventilated layers, highlighting the importance of these layers for propagating the climate signal into the deep ocean. While the intensity of the water mass overturning is relatively consistent between models, when compared to observation-based reconstructions, they exhibit a slightly larger rate of overturning at shallow to intermediate depths, and a slower rate of overturning deeper in the water column. Under increased radiative forcing, atmospheric fluxes increase the rate of simulated upper cell overturning, but this increase is counterbalanced by diapycnal fluxes, including mixed-layer horizontal mixing, and mostly vanishes.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20157" xmlns="http://purl.org/rss/1.0/"><title>Assessment of Southern Ocean mixed-layer depths in CMIP5 models: Historical bias and forcing response</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20157</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Assessment of Southern Ocean mixed-layer depths in CMIP5 models: Historical bias and forcing response</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J.-B. Sallée, E. Shuckburgh, N. Bruneau, A. J. S. Meijers, T. J. Bracegirdle, Z. Wang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-09T13:56:18.979457-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20157</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20157</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20157</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1845</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1862</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20157-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The development of the deep Southern Ocean winter mixed layer in the climate models participating in the fifth Coupled Models Intercomparison Project (CMIP5) is assessed. The deep winter convection regions are key to the ventilation of the ocean interior, and changes in their properties have been related to climate change in numerous studies. Their simulation in climate models is consistently too shallow, too light and shifted equatorward compared to observations. The shallow bias is mostly associated with an excess annual-mean freshwater input at the sea surface that over-stratifies the surface layer and prevents deep convection from developing in winter. In contrast, modeled future changes are mostly associated with a reduced heat loss in winter that leads to even shallower winter mixed layers. The mixed layers shallow most strongly in the Pacific basin under future scenarios, and this is associated with a reduction of the ventilated water volume in the interior. We find a strong state dependency for the future change of mixed-layer depth, with larger future shallowing being simulated by models with larger historical mixed-layer depths. Given that most models are biased shallow, we expect that most CMIP5 climate models might underestimate the future winter mixed-layer shallowing, with important implications for the sequestration of heat, and gases such as carbon dioxide, and therefore for climate.</p></div>]]></content:encoded><description>The development of the deep Southern Ocean winter mixed layer in the climate models participating in the fifth Coupled Models Intercomparison Project (CMIP5) is assessed. The deep winter convection regions are key to the ventilation of the ocean interior, and changes in their properties have been related to climate change in numerous studies. Their simulation in climate models is consistently too shallow, too light and shifted equatorward compared to observations. The shallow bias is mostly associated with an excess annual-mean freshwater input at the sea surface that over-stratifies the surface layer and prevents deep convection from developing in winter. In contrast, modeled future changes are mostly associated with a reduced heat loss in winter that leads to even shallower winter mixed layers. The mixed layers shallow most strongly in the Pacific basin under future scenarios, and this is associated with a reduction of the ventilated water volume in the interior. We find a strong state dependency for the future change of mixed-layer depth, with larger future shallowing being simulated by models with larger historical mixed-layer depths. Given that most models are biased shallow, we expect that most CMIP5 climate models might underestimate the future winter mixed-layer shallowing, with important implications for the sequestration of heat, and gases such as carbon dioxide, and therefore for climate.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20090" xmlns="http://purl.org/rss/1.0/"><title>Small-scale variability of the cross-shelf flow over the outer shelf of the Ross Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20090</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Small-scale variability of the cross-shelf flow over the outer shelf of the Ross Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Josh Kohut, Elias Hunter, Bruce Huber</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-10T16:17:29.728461-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20090</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20090</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20090</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1863</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1876</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20090-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The importance of cross-shelf transport across the Ross Sea on local and remote processes has been well documented. In the Ross Sea, mid-water intrusions of Circumpolar Deep Water (CDW) are modified by shelf water near the shelf break to form Modified Circumpolar Deep Water (MCDW). In 2010–2011, we deployed multi-platform technologies focused on this MCDW intrusion in the vicinity of Mawson and Pennell Banks to better understand its role in ecosystem processes across the shelf. The high-resolution time and space sampling provided by an underwater glider, a short-term mooring, and a ship-based survey highlight the scales over which these critical cross-shelf transport processes occur. MCDW cores were observed as small-scale well-defined features over the western slopes of Pennell and Mawson Banks. The mean transport along Pennell Bank was estimated to be about 0.24 <em>Sv</em> but was highly variable in time (hours to days). The observations suggest that the core of MCDW is transported by a predominately barotropic flow that follows topography around the banks toward the south until the slope of the bank flattens and the warmer water moves up and over the bank. This pathway is shown to link the source MCDW with an area of high productivity over the shallows of Pennell Bank.</p></div>]]></content:encoded><description>
The importance of cross-shelf transport across the Ross Sea on local and remote processes has been well documented. In the Ross Sea, mid-water intrusions of Circumpolar Deep Water (CDW) are modified by shelf water near the shelf break to form Modified Circumpolar Deep Water (MCDW). In 2010–2011, we deployed multi-platform technologies focused on this MCDW intrusion in the vicinity of Mawson and Pennell Banks to better understand its role in ecosystem processes across the shelf. The high-resolution time and space sampling provided by an underwater glider, a short-term mooring, and a ship-based survey highlight the scales over which these critical cross-shelf transport processes occur. MCDW cores were observed as small-scale well-defined features over the western slopes of Pennell and Mawson Banks. The mean transport along Pennell Bank was estimated to be about 0.24 Sv but was highly variable in time (hours to days). The observations suggest that the core of MCDW is transported by a predominately barotropic flow that follows topography around the banks toward the south until the slope of the bank flattens and the warmer water moves up and over the bank. This pathway is shown to link the source MCDW with an area of high productivity over the shallows of Pennell Bank.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20149" xmlns="http://purl.org/rss/1.0/"><title>Subtidal water flux through a multiple-inlet system: Observations before and during a cold front event and numerical experiments</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20149</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Subtidal water flux through a multiple-inlet system: Observations before and during a cold front event and numerical experiments</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Chunyan Li</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-10T16:18:52.77768-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20149</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20149</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20149</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1877</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1892</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20149-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This paper examines the net transport through a multiple-inlet bay under a combined force of strong wind and tide, with observations and a model experiment. The observations were made in central Georgia in Sapelo and Altamaha Sounds between 13 and 17 September 2000. Wind was weak in the beginning of the survey. An air pressure trough (as a weak cold front) passed the area on 16 September, when the wind changed to the northeast and increased in magnitude. This front was associated with a midlatitude cyclone in the New England area. This weather event with an episode of strong northeasterly winds prompted a numerical model experiment on an idealized three-inlet bay, with a set of nonlinear 2-D shallow water equations on an <em>f</em> plane, which provides some insight to the wind-driven circulation under the presence of tidal forcing. It is found that tidally induced currents are small compared to wind-induced flows. When the wind direction is not perpendicular to the alignment of the three inlets, the net outward flow tends to occur at the inlet farther away in the downwind direction. This is associated with a net inward transport in the inlet opposite of the downwind direction. As a result, the middle inlet has the minimum of the net flow. When the wind is perpendicular to the barrier islands, and if the three inlets have different maximum depth values, the deeper inlet tends to have a net flow against the wind, while the shallower inlet tends to have a net flow in the direction of the wind. Offshore (onshore) currents may develop outside of the inlet with outward (inward) flow, as an effect of fluxes through the inlets on the coastal ocean.</p></div>]]></content:encoded><description>This paper examines the net transport through a multiple-inlet bay under a combined force of strong wind and tide, with observations and a model experiment. The observations were made in central Georgia in Sapelo and Altamaha Sounds between 13 and 17 September 2000. Wind was weak in the beginning of the survey. An air pressure trough (as a weak cold front) passed the area on 16 September, when the wind changed to the northeast and increased in magnitude. This front was associated with a midlatitude cyclone in the New England area. This weather event with an episode of strong northeasterly winds prompted a numerical model experiment on an idealized three-inlet bay, with a set of nonlinear 2-D shallow water equations on an f plane, which provides some insight to the wind-driven circulation under the presence of tidal forcing. It is found that tidally induced currents are small compared to wind-induced flows. When the wind direction is not perpendicular to the alignment of the three inlets, the net outward flow tends to occur at the inlet farther away in the downwind direction. This is associated with a net inward transport in the inlet opposite of the downwind direction. As a result, the middle inlet has the minimum of the net flow. When the wind is perpendicular to the barrier islands, and if the three inlets have different maximum depth values, the deeper inlet tends to have a net flow against the wind, while the shallower inlet tends to have a net flow in the direction of the wind. Offshore (onshore) currents may develop outside of the inlet with outward (inward) flow, as an effect of fluxes through the inlets on the coastal ocean.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20161" xmlns="http://purl.org/rss/1.0/"><title>The effects of geothermal heating on the East/Japan Sea circulation</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20161</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The effects of geothermal heating on the East/Japan Sea circulation</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Young-Gyu Park, Jae-Hun Park, Ho Jin Lee, Hong Sik Min, Seon-Dong Kim</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-10T15:42:24.621067-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20161</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20161</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20161</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1893</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1905</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The magnitude of geothermal heating in the East/Japan Sea is about 100 mW/m<sup>2</sup>, twice that of a typical abyssal plain. In addition, bottom stratification in the East/Japan Sea is much weaker than that typical of the open ocean. Thus, geothermal heating could have more prominent effects in the East/Japan Sea than in the open ocean, and we tested this hypothesis via numerical modeling. With less than 100 mW/m<sup>2</sup> bottom heat flux, we were able to reproduce bottom mixed layers that are thicker than ~1000 m as observed. Previously, no numerical model has been successful in reproducing such bottom mixed layers. Geothermal heating intensifies the bottom flows but the simulated flows are not as strong as the observed ones. Over the northern part of the East/Japan Sea, reduction in deep stratification strengthens deep water mass formation, intensifying cyclonic circulations located over this area, so the effects of the heating extend to the surface. As the cyclonic circulation becomes stronger, the water at the center of the gyre is trapped and more exposed to cold air, so it becomes cooler, and colder deep water is produced. When the geothermal heating is strong enough, the surface cooling effect dominates the bottom heating and the deep layer becomes cooler showing that the nonlinear effects of geothermal heating are far reaching. Thus, to account for the observed dynamics, the full three-dimensional circulation at the basin scale is needed.</p></div>]]></content:encoded><description>The magnitude of geothermal heating in the East/Japan Sea is about 100 mW/m2, twice that of a typical abyssal plain. In addition, bottom stratification in the East/Japan Sea is much weaker than that typical of the open ocean. Thus, geothermal heating could have more prominent effects in the East/Japan Sea than in the open ocean, and we tested this hypothesis via numerical modeling. With less than 100 mW/m2 bottom heat flux, we were able to reproduce bottom mixed layers that are thicker than ~1000 m as observed. Previously, no numerical model has been successful in reproducing such bottom mixed layers. Geothermal heating intensifies the bottom flows but the simulated flows are not as strong as the observed ones. Over the northern part of the East/Japan Sea, reduction in deep stratification strengthens deep water mass formation, intensifying cyclonic circulations located over this area, so the effects of the heating extend to the surface. As the cyclonic circulation becomes stronger, the water at the center of the gyre is trapped and more exposed to cold air, so it becomes cooler, and colder deep water is produced. When the geothermal heating is strong enough, the surface cooling effect dominates the bottom heating and the deep layer becomes cooler showing that the nonlinear effects of geothermal heating are far reaching. Thus, to account for the observed dynamics, the full three-dimensional circulation at the basin scale is needed.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20164" xmlns="http://purl.org/rss/1.0/"><title>Mesoscale eddies in the northwestern subtropical Pacific Ocean: Statistical characteristics and three-dimensional structures</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20164</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Mesoscale eddies in the northwestern subtropical Pacific Ocean: Statistical characteristics and three-dimensional structures</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Guang Yang, Fan Wang, Yuanlong Li, Pengfei Lin</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-10T15:52:36.065544-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20164</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20164</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20164</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1906</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1925</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Mesoscale eddy properties in the northwestern subtropical Pacific Ocean are investigated by analyzing 22,567 cyclonic eddies (CEs) and 26,365 anticyclonic eddies (AEs) detected from 19 year altimetric sea level records. Eddy occurrence frequency and kinetic energy are prevailingly high in the Subtropical Countercurrent zonal band between 19°N and 26°N and further elevated near the Luzon-Taiwan coast. A general superiority of AEs is observed at most latitudes except between 19°N and 22°N, where the CE number is larger. The modal radius and mean lifespan of the CEs (AEs) are 134 km and 11.2 weeks (121 km and 10.9 weeks), respectively. After generation, most eddies propagate westward with a mean speed of 7.2 cm s<sup>−1</sup> and deflect northward following the Kuroshio along the Luzon-Taiwan coast. Three-dimensional eddy structures are further explored with composite eddy images in five subregions constructed by surfacing Argo temperature/salinity data into altimeter-detected eddy areas. Due to the existence of mode waters in the main thermocline, eddy-induced temperature anomaly exhibits a double-core vertical structure which is especially evident in CE images. Because of the vertical water mass distribution, salinity anomaly features a sandwich-like pattern which is more evident in AE images. Also revealed is the significant structure difference in these five subregions. Eddies are greatly intensified as they approach the western boundary, inducing larger temperature and salinity anomalies and influencing deeper ocean. Along the Luzon-Taiwan coast, AEs are preferentially strengthened by the northward background flow.</p></div>]]></content:encoded><description>Mesoscale eddy properties in the northwestern subtropical Pacific Ocean are investigated by analyzing 22,567 cyclonic eddies (CEs) and 26,365 anticyclonic eddies (AEs) detected from 19 year altimetric sea level records. Eddy occurrence frequency and kinetic energy are prevailingly high in the Subtropical Countercurrent zonal band between 19°N and 26°N and further elevated near the Luzon-Taiwan coast. A general superiority of AEs is observed at most latitudes except between 19°N and 22°N, where the CE number is larger. The modal radius and mean lifespan of the CEs (AEs) are 134 km and 11.2 weeks (121 km and 10.9 weeks), respectively. After generation, most eddies propagate westward with a mean speed of 7.2 cm s−1 and deflect northward following the Kuroshio along the Luzon-Taiwan coast. Three-dimensional eddy structures are further explored with composite eddy images in five subregions constructed by surfacing Argo temperature/salinity data into altimeter-detected eddy areas. Due to the existence of mode waters in the main thermocline, eddy-induced temperature anomaly exhibits a double-core vertical structure which is especially evident in CE images. Because of the vertical water mass distribution, salinity anomaly features a sandwich-like pattern which is more evident in AE images. Also revealed is the significant structure difference in these five subregions. Eddies are greatly intensified as they approach the western boundary, inducing larger temperature and salinity anomalies and influencing deeper ocean. Along the Luzon-Taiwan coast, AEs are preferentially strengthened by the northward background flow.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20113" xmlns="http://purl.org/rss/1.0/"><title>Large-eddy simulation and low-order modeling of sediment-oxygen uptake in a transitional oscillatory flow</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20113</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Large-eddy simulation and low-order modeling of sediment-oxygen uptake in a transitional oscillatory flow</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. Scalo, L. Boegman, U. Piomelli</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-11T09:25:54.749042-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20113</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20113</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20113</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1926</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1939</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20113-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We have tested a dissolved oxygen (DO) transport model based on large-eddy simulation (LES) of a transitional oscillatory flow observed in the bottom boundary layer of Lake Alpnach, Switzerland. The transition from a quasi-laminar to a fully turbulent state makes this flow difficult to study with a Reynolds-averaged Navier-Stokes equation (RANSE) model. By resolving the full range of governing transport processes, LES provides a reliable prediction of the sediment-oxygen uptake (SOU). The model biogeochemical and flow parameters have been calibrated against DO and velocity measurements from published in situ data at the earliest phase available in the cycle. The fully developed flow thus obtained is used as an initial condition for the imposed oscillatory forcing. Numerical predictions show that transport in the outer layer is in equilibrium with the main current throughout most of the cycle and that nonequilibrium effects are limited to the diffusive sublayer response to the external forcing. During flow deceleration, the concentration boundary layer slowly expands as turbulence decays; later, during re-transition, mixing is restored by rapid and intense turbulent production events enhancing the SOU with a well-defined time lag. An algebraic model for the SOU is proposed for eventual inclusion in RANSE biogeochemical management-type models developed based on parameterizations used in turbulent mass transfer and with the support of published numerical data and the present simulation. The only input parameters required are the sediment oxidation rate, bulk temperature and DO concentration, and friction velocity.</p></div>]]></content:encoded><description>We have tested a dissolved oxygen (DO) transport model based on large-eddy simulation (LES) of a transitional oscillatory flow observed in the bottom boundary layer of Lake Alpnach, Switzerland. The transition from a quasi-laminar to a fully turbulent state makes this flow difficult to study with a Reynolds-averaged Navier-Stokes equation (RANSE) model. By resolving the full range of governing transport processes, LES provides a reliable prediction of the sediment-oxygen uptake (SOU). The model biogeochemical and flow parameters have been calibrated against DO and velocity measurements from published in situ data at the earliest phase available in the cycle. The fully developed flow thus obtained is used as an initial condition for the imposed oscillatory forcing. Numerical predictions show that transport in the outer layer is in equilibrium with the main current throughout most of the cycle and that nonequilibrium effects are limited to the diffusive sublayer response to the external forcing. During flow deceleration, the concentration boundary layer slowly expands as turbulence decays; later, during re-transition, mixing is restored by rapid and intense turbulent production events enhancing the SOU with a well-defined time lag. An algebraic model for the SOU is proposed for eventual inclusion in RANSE biogeochemical management-type models developed based on parameterizations used in turbulent mass transfer and with the support of published numerical data and the present simulation. The only input parameters required are the sediment oxidation rate, bulk temperature and DO concentration, and friction velocity.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20158" xmlns="http://purl.org/rss/1.0/"><title>Sea ice motion and open water area at the Ronne Polynia, Antarctica: Synthetic aperture radar observations versus model results</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20158</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea ice motion and open water area at the Ronne Polynia, Antarctica: Synthetic aperture radar observations versus model results</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">T. Hollands, V. Haid, W. Dierking, R. Timmermann, L. Ebner</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-11T14:06:55.480357-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20158</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20158</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20158</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1940</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1954</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20158-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This study deals with observations and simulations of the evolution of coastal polynias focusing on the Ronne Polynia. We compare differences in polynia extent and ice drift patterns derived from satellite radar images and from simulations with the Finite Element Sea Ice Ocean Model, employing three atmospheric forcing data sets that differ in spatial and temporal resolution. Two polynia events are analyzed, one from austral summer and one from late fall 2008. The open water area in the polynia is of similar size in the satellite images and in the model simulations, but its temporal evolution differs depending on katabatic winds being resolved in the atmospheric forcing data sets. Modeled ice drift is slower than the observed and reveals greater turning angles relative to the wind direction in many cases. For the summer event, model results obtained with high-resolution forcing are closer to the drift field derived from radar imagery than those from coarse resolution forcing. For the late fall event, none of the forcing data yields outstanding results. Our study demonstrates that a dense (1–3 km) model grid and atmospheric forcing provided at high spatial resolution ( &lt; 50 km) are critical to correctly simulate coastal polynias with a coupled sea-ice ocean model.</p></div>]]></content:encoded><description>This study deals with observations and simulations of the evolution of coastal polynias focusing on the Ronne Polynia. We compare differences in polynia extent and ice drift patterns derived from satellite radar images and from simulations with the Finite Element Sea Ice Ocean Model, employing three atmospheric forcing data sets that differ in spatial and temporal resolution. Two polynia events are analyzed, one from austral summer and one from late fall 2008. The open water area in the polynia is of similar size in the satellite images and in the model simulations, but its temporal evolution differs depending on katabatic winds being resolved in the atmospheric forcing data sets. Modeled ice drift is slower than the observed and reveals greater turning angles relative to the wind direction in many cases. For the summer event, model results obtained with high-resolution forcing are closer to the drift field derived from radar imagery than those from coarse resolution forcing. For the late fall event, none of the forcing data yields outstanding results. Our study demonstrates that a dense (1–3 km) model grid and atmospheric forcing provided at high spatial resolution ( &lt; 50 km) are critical to correctly simulate coastal polynias with a coupled sea-ice ocean model.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20162" xmlns="http://purl.org/rss/1.0/"><title>Field observations of wave-induced streaming through a submerged seagrass (Posidonia oceanica) meadow</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20162</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Field observations of wave-induced streaming through a submerged seagrass (Posidonia oceanica) meadow</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Mitul Luhar, Eduardo Infantes, Alejandro Orfila, Jorge Terrados, Heidi M. Nepf</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-11T09:47:59.313611-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20162</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20162</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20162</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1955</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1968</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This paper reports the findings of a 2 week field campaign designed to study wave-induced flows within a meadow of <em>Posidonia oceanica</em> at water depth 9 <em>m</em>. Previous laboratory experiments suggest that waves induce a mean mass drift in the direction of wave propagation (“streaming”) through submerged canopies of vegetation. This paper provides the first field measurements of this wave-induced streaming. During periods of high wave activity, streaming flows with magnitudes as high as 20% of the near-bed oscillatory velocity were measured within the meadow. In addition to presenting field measurements of wave-induced streaming, this paper also considers the damping of wave-induced oscillatory flow within the seagrass meadow. Oscillatory velocities measured within the meadow were reduced by less than 30% relative to those above the meadow over the duration of the study. This is in agreement with previous laboratory and field measurements which show that oscillatory flows are damped less within submerged canopies compared to unidirectional flows. Existing analytical models underpredict the magnitude of the streaming flow and overpredict oscillatory velocity reductions. These discrepancies are thought to arise because the drag generated by flexible seagrasses moving with wave-induced flow is not well described.</p></div>]]></content:encoded><description>
This paper reports the findings of a 2 week field campaign designed to study wave-induced flows within a meadow of Posidonia oceanica at water depth 9 m. Previous laboratory experiments suggest that waves induce a mean mass drift in the direction of wave propagation (“streaming”) through submerged canopies of vegetation. This paper provides the first field measurements of this wave-induced streaming. During periods of high wave activity, streaming flows with magnitudes as high as 20% of the near-bed oscillatory velocity were measured within the meadow. In addition to presenting field measurements of wave-induced streaming, this paper also considers the damping of wave-induced oscillatory flow within the seagrass meadow. Oscillatory velocities measured within the meadow were reduced by less than 30% relative to those above the meadow over the duration of the study. This is in agreement with previous laboratory and field measurements which show that oscillatory flows are damped less within submerged canopies compared to unidirectional flows. Existing analytical models underpredict the magnitude of the streaming flow and overpredict oscillatory velocity reductions. These discrepancies are thought to arise because the drag generated by flexible seagrasses moving with wave-induced flow is not well described.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20119" xmlns="http://purl.org/rss/1.0/"><title>Bathymetric effects on estuarine plume dynamics</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20119</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Bathymetric effects on estuarine plume dynamics</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jungwoo Lee, Arnoldo Valle-Levinson</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-16T14:37:21.665811-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20119</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20119</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20119</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1969</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1981</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The influence of bathymetry on an estuary plume at an estuary-shelf transition is studied with a three-dimensional ocean circulation model. To understand the response of the plume to bathymetry, several types of estuarine shapes and shelf geometries were adopted in this numerical study. The channel's shape and its width-to-depth aspect ratio affected the fate of the plume by determining flow characteristics inside the estuary. Moreover, the bathymetry of the shelf such as the shelf slope and the direction of a submarine channel defined the plume characteristics on the shelf. An estuarine channel with a triangular cross section generated relatively stronger exchange flows at midestuary than a rectangular cross section, which resulted in a larger surface plume over the shelf. The extension of the submarine channel onto the shelf favored increased plume water transport out to the shelf, a result of reduced frictional effects on the shelf. The orientation of the submarine channel changed the direction of the plume over the shelf, with no additional external forces. Two fronts developed at the edges of the submarine channel because of enhanced lateral shears in the flow. When the estuary was relatively wide compared to the internal Rossby radius (Kelvin number <em>Ke</em> ≥ 5), or when the relative strength of the freshwater discharge compared to the estuary width was weak (Rossby number <em>Ro</em> ≤ 0.05), the coastal plume did not expand up-shelf. In fact, results indicated that freshwater up-shelf transport in a coastal current, moving against Coriolis’ accelerations, was proportional to <em>Ro</em>.</p></div>]]></content:encoded><description>
The influence of bathymetry on an estuary plume at an estuary-shelf transition is studied with a three-dimensional ocean circulation model. To understand the response of the plume to bathymetry, several types of estuarine shapes and shelf geometries were adopted in this numerical study. The channel's shape and its width-to-depth aspect ratio affected the fate of the plume by determining flow characteristics inside the estuary. Moreover, the bathymetry of the shelf such as the shelf slope and the direction of a submarine channel defined the plume characteristics on the shelf. An estuarine channel with a triangular cross section generated relatively stronger exchange flows at midestuary than a rectangular cross section, which resulted in a larger surface plume over the shelf. The extension of the submarine channel onto the shelf favored increased plume water transport out to the shelf, a result of reduced frictional effects on the shelf. The orientation of the submarine channel changed the direction of the plume over the shelf, with no additional external forces. Two fronts developed at the edges of the submarine channel because of enhanced lateral shears in the flow. When the estuary was relatively wide compared to the internal Rossby radius (Kelvin number Ke ≥ 5), or when the relative strength of the freshwater discharge compared to the estuary width was weak (Rossby number Ro ≤ 0.05), the coastal plume did not expand up-shelf. In fact, results indicated that freshwater up-shelf transport in a coastal current, moving against Coriolis’ accelerations, was proportional to Ro.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20152" xmlns="http://purl.org/rss/1.0/"><title>Formation of salinity maximum water and its contribution to the overturning circulation in the North Atlantic as revealed by a global general circulation model</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20152</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Formation of salinity maximum water and its contribution to the overturning circulation in the North Atlantic as revealed by a global general circulation model</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Tangdong Qu, Shan Gao, Ichiro Fukumori</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-16T04:11:45.254327-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20152</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20152</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20152</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1982</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1994</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20152-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The formation of salinity maximum water in the North Atlantic is investigated using a simulated passive tracer and its adjoint. The results reveal that most salinity maximum water in the North Atlantic comes from the northwestern part of the subtropical gyre, and direct contribution from the evaporation-precipitation maximum region via the surface Ekman current is minor. Water originating from the evaporation-precipitation maximum region has to recirculate in the subtropical gyre before entering the sea surface salinity maximum region from the northwest. Once subducted, some portion (~10%) of the salinity maximum water enters the equatorial region in the shallow subtropical cell, but most (~70%) of it appears to turn northward to join the North Atlantic Deep Water. The latter pathway involves a three-dimensional circulation. When the warm, fresh surface water flows northward along the western boundary, it turns eastward in the northern subtropical gyre. As a result of the large excess of evaporation over precipitation, this water gradually gains its salinity on the route, until it reaches the sea surface salinity maximum region in the central subtropical gyre. From there, the salinity maximum water is subducted and flows back to the western boundary in the depth range of the thermocline. With its high-salinity nature, a major portion of this water penetrates into the subpolar region and directly contributes to the deep thermohaline circulation.</p></div>]]></content:encoded><description>
The formation of salinity maximum water in the North Atlantic is investigated using a simulated passive tracer and its adjoint. The results reveal that most salinity maximum water in the North Atlantic comes from the northwestern part of the subtropical gyre, and direct contribution from the evaporation-precipitation maximum region via the surface Ekman current is minor. Water originating from the evaporation-precipitation maximum region has to recirculate in the subtropical gyre before entering the sea surface salinity maximum region from the northwest. Once subducted, some portion (~10%) of the salinity maximum water enters the equatorial region in the shallow subtropical cell, but most (~70%) of it appears to turn northward to join the North Atlantic Deep Water. The latter pathway involves a three-dimensional circulation. When the warm, fresh surface water flows northward along the western boundary, it turns eastward in the northern subtropical gyre. As a result of the large excess of evaporation over precipitation, this water gradually gains its salinity on the route, until it reaches the sea surface salinity maximum region in the central subtropical gyre. From there, the salinity maximum water is subducted and flows back to the western boundary in the depth range of the thermocline. With its high-salinity nature, a major portion of this water penetrates into the subpolar region and directly contributes to the deep thermohaline circulation.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20159" xmlns="http://purl.org/rss/1.0/"><title>Influence of Amur River discharge on phytoplankton photophysiology in the Sea of Okhotsk during late summer</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20159</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Influence of Amur River discharge on phytoplankton photophysiology in the Sea of Okhotsk during late summer</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Tomonori Isada, Takahiro Iida, Hongbin Liu, Sei-Ichi Saitoh, Jun Nishioka, Takeshi Nakatsuka, Koji Suzuki</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-16T14:46:48.563248-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20159</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20159</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20159</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1995</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2013</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20159-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We investigated the photosynthetic parameters of phytoplankton in the Sea of Okhotsk during the late summer of 2006 to characterize their spatiotemporal variability and to test the hypothesis that discharge from the Amur River could influence the algal photophysiology. The highest maximum quantum yield of carbon fixation in photosynthesis (Φ<sub>cmax</sub>; 0.098 mol C mol photons<sup>-1</sup>) was found near the Amur River mouth, where nitrate was depleted. However, none of the photosynthetic parameters, including primary productivity (<em>PP</em>) at the surface, were correlated with temperature, daily photosynthetically available radiation (PAR), or ambient nutrient concentrations. Variations in Φ<sub>cmax</sub> depended on the variations in not only the mean chlorophyll <em>a</em> specific absorption coefficient of phytoplankton (<em>ā</em><sup>*</sup><sub>ph</sub>) but also the slope index of the absorption coefficient of phytoplankton (<em>a</em><sub>ph</sub> slope), an indicator for the ratio of nonphotosynthetic carotenoids to photosynthetic carotenoids. These results indicated that the phytoplankton assemblages acclimated to the ambient light conditions by regulating their cellular pigments. Additionally, <em>ā</em><sup>*</sup><sub>ph</sub> and euphotic depth (<em>Z</em><sub>eu</sub>) were significantly correlated with salinity, suggesting that photoacclimation of the phytoplankton assemblages observed in this study could be induced by discharge of Amur River. Because spatiotemporal variations in <em>PP</em> were concomitant with Φ<sub>cmax</sub>, <em>ā<sup>*</sup></em><sub>ph</sub>, and the chlorophyll <em>a</em> concentration, <em>PP</em> models based on inherent optical property (IOP) were suitable for estimating <em>PP</em> in the Sea of Okhotsk. This study is the first to investigate the factors controlling phytoplankton photophysiology in the Sea of Okhotsk, one of the highest primary production areas in the world.</p></div>]]></content:encoded><description>
We investigated the photosynthetic parameters of phytoplankton in the Sea of Okhotsk during the late summer of 2006 to characterize their spatiotemporal variability and to test the hypothesis that discharge from the Amur River could influence the algal photophysiology. The highest maximum quantum yield of carbon fixation in photosynthesis (Φcmax; 0.098 mol C mol photons-1) was found near the Amur River mouth, where nitrate was depleted. However, none of the photosynthetic parameters, including primary productivity (PP) at the surface, were correlated with temperature, daily photosynthetically available radiation (PAR), or ambient nutrient concentrations. Variations in Φcmax depended on the variations in not only the mean chlorophyll a specific absorption coefficient of phytoplankton (ā*ph) but also the slope index of the absorption coefficient of phytoplankton (aph slope), an indicator for the ratio of nonphotosynthetic carotenoids to photosynthetic carotenoids. These results indicated that the phytoplankton assemblages acclimated to the ambient light conditions by regulating their cellular pigments. Additionally, ā*ph and euphotic depth (Zeu) were significantly correlated with salinity, suggesting that photoacclimation of the phytoplankton assemblages observed in this study could be induced by discharge of Amur River. Because spatiotemporal variations in PP were concomitant with Φcmax, ā*ph, and the chlorophyll a concentration, PP models based on inherent optical property (IOP) were suitable for estimating PP in the Sea of Okhotsk. This study is the first to investigate the factors controlling phytoplankton photophysiology in the Sea of Okhotsk, one of the highest primary production areas in the world.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20096" xmlns="http://purl.org/rss/1.0/"><title>Sea level and heat content changes in the western North Pacific</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20096</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sea level and heat content changes in the western North Pacific</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jae-Hong Moon, Y. Tony Song</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-17T14:12:56.411052-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20096</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20096</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20096</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2014</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2022</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Altimetry-observed sea level rise (SLR) over the western North Pacific (WNP), including the South China Sea, Yellow Sea, East China Sea, and East/Japan Sea, has a rate of ~5 mm/year over 1993–2010, which is about 1.5 times the rate of the global mean. Here we have examined sea level changes and related ocean heat content (OHC) in the WNP by comparing results from a non-Boussinesq ocean general circulation model (mass-conserved) with data sets from altimeters, the Gravity Recovery and Climate Experiment (GRACE), and in situ profiles. Our model reproduces the altimetry regional trends as well as their seasonal/interannual variations. Adding a GRACE-estimated mass to the model result further explains the altimetry SLR in a way that mass-induced effect contributes more in the midlatitudes than in the tropical WNP over the GRACE period. In addition, interannual variability and linear trend of regional sea levels are explained mainly by changes in the OHC due to heat convergence and divergence by ocean circulations, while seasonal variability is caused mainly by surface air-sea fluxes. To understand the underline physics, a comparative experiment was carried out, showing that the recent strengthening trends of SLR and OHC in the tropical regions are significantly attributed to the heat and water mass redistribution in the upper ocean caused by the intensified easterly trade wind over the past two decades.</p></div>]]></content:encoded><description>
Altimetry-observed sea level rise (SLR) over the western North Pacific (WNP), including the South China Sea, Yellow Sea, East China Sea, and East/Japan Sea, has a rate of ~5 mm/year over 1993–2010, which is about 1.5 times the rate of the global mean. Here we have examined sea level changes and related ocean heat content (OHC) in the WNP by comparing results from a non-Boussinesq ocean general circulation model (mass-conserved) with data sets from altimeters, the Gravity Recovery and Climate Experiment (GRACE), and in situ profiles. Our model reproduces the altimetry regional trends as well as their seasonal/interannual variations. Adding a GRACE-estimated mass to the model result further explains the altimetry SLR in a way that mass-induced effect contributes more in the midlatitudes than in the tropical WNP over the GRACE period. In addition, interannual variability and linear trend of regional sea levels are explained mainly by changes in the OHC due to heat convergence and divergence by ocean circulations, while seasonal variability is caused mainly by surface air-sea fluxes. To understand the underline physics, a comparative experiment was carried out, showing that the recent strengthening trends of SLR and OHC in the tropical regions are significantly attributed to the heat and water mass redistribution in the upper ocean caused by the intensified easterly trade wind over the past two decades.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20069" xmlns="http://purl.org/rss/1.0/"><title>Intraseasonal Kelvin wave in Makassar Strait</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20069</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Intraseasonal Kelvin wave in Makassar Strait</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">K. Pujiana, A. L. Gordon, J. Sprintall</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-18T09:05:16.862402-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20069</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20069</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20069</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2023</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2034</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20069-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Time series observations during 2004–2006 reveal the presence of 60–90 days intraseasonal events that impact the transport and mixing environment within Makassar Strait. The observed velocity and temperature fluctuations within the pycnocline reveal the presence of Kelvin waves including vertical energy propagation, energy equipartition, and nondispersive relationship. Two current meters at 750 and 1500 m provide further evidence that the vertical structure of the downwelling Kelvin wave resembles that of the second baroclinic wave mode. The Kelvin waves derive their energy from the equatorial Indian Ocean winds, including those associated with the Madden-Julian oscillations, and propagate from Lombok Strait to Makassar Strait along the 100-m isobath. The northward propagating Kelvin waves within the pycnocline reduce the southward Makassar Strait throughflow by up to 2 Sv and induce a marked increase of vertical diffusivity.</p></div>]]></content:encoded><description>
Time series observations during 2004–2006 reveal the presence of 60–90 days intraseasonal events that impact the transport and mixing environment within Makassar Strait. The observed velocity and temperature fluctuations within the pycnocline reveal the presence of Kelvin waves including vertical energy propagation, energy equipartition, and nondispersive relationship. Two current meters at 750 and 1500 m provide further evidence that the vertical structure of the downwelling Kelvin wave resembles that of the second baroclinic wave mode. The Kelvin waves derive their energy from the equatorial Indian Ocean winds, including those associated with the Madden-Julian oscillations, and propagate from Lombok Strait to Makassar Strait along the 100-m isobath. The northward propagating Kelvin waves within the pycnocline reduce the southward Makassar Strait throughflow by up to 2 Sv and induce a marked increase of vertical diffusivity.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20094" xmlns="http://purl.org/rss/1.0/"><title>Pathways of the North Pacific Intermediate Water identified through the tangent linear and adjoint models of an ocean general circulation model</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20094</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Pathways of the North Pacific Intermediate Water identified through the tangent linear and adjoint models of an ocean general circulation model</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Yosuke Fujii, Toshiya Nakano, Norihisa Usui, Satoshi Matsumoto, Hiroyuki Tsujino, Masafumi Kamachi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-18T09:11:34.885901-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20094</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20094</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20094</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2035</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2051</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20094-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This study develops a strategy for tracing a target water mass, and applies it to analyzing the pathway of the North Pacific Intermediate Water (NPIW) from the subarctic gyre to the northwestern part of the subtropical gyre south of Japan in a simulation of an ocean general circulation model. This strategy estimates the pathway of the water mass that travels from an origin to a destination area during a specific period using a conservation property concerning tangent linear and adjoint models. In our analysis, a large fraction of the low salinity origin water mass of NPIW initially comes from the Okhotsk or Bering Sea, flows through the southeastern side of the Kuril Islands, and is advected to the Mixed Water Region (MWR) by the Oyashio current. It then enters the Kuroshio Extension (KE) at the first KE ridge, and is advected eastward by the KE current. However, it deviates southward from the KE axis around 158°E over the Shatsky Rise, or around 170°E on the western side of the Emperor Seamount Chain, and enters the subtropical gyre. It is finally transported westward by the recirculation flow. This pathway corresponds well to the shortcut route of NPIW from MWR to the region south of Japan inferred from analysis of the long-term freshening trend of NPIW observation. Copyright © 2013 John Wiley &amp; Sons, Ltd.</p></div>]]></content:encoded><description>This study develops a strategy for tracing a target water mass, and applies it to analyzing the pathway of the North Pacific Intermediate Water (NPIW) from the subarctic gyre to the northwestern part of the subtropical gyre south of Japan in a simulation of an ocean general circulation model. This strategy estimates the pathway of the water mass that travels from an origin to a destination area during a specific period using a conservation property concerning tangent linear and adjoint models. In our analysis, a large fraction of the low salinity origin water mass of NPIW initially comes from the Okhotsk or Bering Sea, flows through the southeastern side of the Kuril Islands, and is advected to the Mixed Water Region (MWR) by the Oyashio current. It then enters the Kuroshio Extension (KE) at the first KE ridge, and is advected eastward by the KE current. However, it deviates southward from the KE axis around 158°E over the Shatsky Rise, or around 170°E on the western side of the Emperor Seamount Chain, and enters the subtropical gyre. It is finally transported westward by the recirculation flow. This pathway corresponds well to the shortcut route of NPIW from MWR to the region south of Japan inferred from analysis of the long-term freshening trend of NPIW observation. Copyright © 2013 John Wiley &amp; Sons, Ltd.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20144" xmlns="http://purl.org/rss/1.0/"><title>Subantarctic mode water in the southeast Pacific: Effect of exchange across the Subantarctic Front</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20144</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Subantarctic mode water in the southeast Pacific: Effect of exchange across the Subantarctic Front</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J. W. Holte, L. D. Talley, T. K. Chereskin, B. M. Sloyan</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-23T10:03:02.239358-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20144</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20144</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20144</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2052</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2066</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20144-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> This study considered cross-frontal exchange as a possible mechanism for the observed along-front freshening and cooling between the 27.0 and 27.3 kg m<sup> − 3</sup> isopycnals north of the Subantarctic Front (SAF) in the southeast Pacific Ocean. This isopycnal range, which includes the densest Subantarctic Mode Water (SAMW) formed in this region, is mostly below the mixed layer, and so experiences little direct air-sea forcing. Data from two cruises in the southeast Pacific were examined for evidence of cross-frontal exchange; numerous eddies and intrusions containing Polar Frontal Zone (PFZ) water were observed north of the SAF, as well as a fresh surface layer during the summer cruise that was likely due to Ekman transport. These features penetrated north of the SAF, even though the potential vorticity structure of the SAF should have acted as a barrier to exchange. An optimum multiparameter (OMP) analysis incorporating a range of observed properties was used to estimate the cumulative cross-frontal exchange. The OMP analysis revealed an along-front increase in PFZ water fractional content in the region north of the SAF between the 27.1 and 27.3 kg m<sup> − 3</sup> isopycnals; the increase was approximately 0.13 for every 15° of longitude. Between the 27.0 and 27.1 kg m<sup> − 3</sup> isopycnals, the increase was approximately 0.15 for every 15° of longitude. A simple bulk calculation revealed that this magnitude of cross-frontal exchange could have caused the downstream evolution of SAMW temperature and salinity properties observed by Argo profiling floats.</p></div>]]></content:encoded><description>This study considered cross-frontal exchange as a possible mechanism for the observed along-front freshening and cooling between the 27.0 and 27.3 kg m − 3 isopycnals north of the Subantarctic Front (SAF) in the southeast Pacific Ocean. This isopycnal range, which includes the densest Subantarctic Mode Water (SAMW) formed in this region, is mostly below the mixed layer, and so experiences little direct air-sea forcing. Data from two cruises in the southeast Pacific were examined for evidence of cross-frontal exchange; numerous eddies and intrusions containing Polar Frontal Zone (PFZ) water were observed north of the SAF, as well as a fresh surface layer during the summer cruise that was likely due to Ekman transport. These features penetrated north of the SAF, even though the potential vorticity structure of the SAF should have acted as a barrier to exchange. An optimum multiparameter (OMP) analysis incorporating a range of observed properties was used to estimate the cumulative cross-frontal exchange. The OMP analysis revealed an along-front increase in PFZ water fractional content in the region north of the SAF between the 27.1 and 27.3 kg m − 3 isopycnals; the increase was approximately 0.13 for every 15° of longitude. Between the 27.0 and 27.1 kg m − 3 isopycnals, the increase was approximately 0.15 for every 15° of longitude. A simple bulk calculation revealed that this magnitude of cross-frontal exchange could have caused the downstream evolution of SAMW temperature and salinity properties observed by Argo profiling floats.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20168" xmlns="http://purl.org/rss/1.0/"><title>(Sub-)inertial wave boundary turbulence in the Gulf of Valencia</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20168</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">(Sub-)inertial wave boundary turbulence in the Gulf of Valencia</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Hans Haren, Marta Ribó, Pere Puig</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-25T09:46:35.084911-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20168</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20168</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20168</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2067</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2073</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The bottom boundary layer above sloping topography can be highly turbulent, even in deep seas. This is demonstrated here using high-resolution 1-Hz sampling temperature sensors that were moored for 5 months every 0.5 m between 6.5 and 61 m above a 572 m deep seafloor promontory on the continental slope off Valencia, Spain. Using these data, turbulence parameters have been estimated. With time and in the vertical, values vary over four orders of magnitude. They have a dominant local inertial period which is modulated by an about 11 day periodicity associated with variations in a baroclinic unstable boundary current. When this current is strong and Eastward, the upslope phase of inertial wave generates convective turbulence which reaches closest to the bottom and therefore can effect sediment dispersal. In late winter, equally strong shear-induced turbulence in 50 m high Kelvin-Helmholtz (K-H) overturns is forced by 0.2 m s<sup>−1</sup> off/downslope motions, which are preceded by periods of warming of a few 0.01°C before the cooler near-bottom water is suddenly flushed over the promontory into the basin. Such anomalously large K-H overturns occurred 6 times in the investigated winter period.</p></div>]]></content:encoded><description>The bottom boundary layer above sloping topography can be highly turbulent, even in deep seas. This is demonstrated here using high-resolution 1-Hz sampling temperature sensors that were moored for 5 months every 0.5 m between 6.5 and 61 m above a 572 m deep seafloor promontory on the continental slope off Valencia, Spain. Using these data, turbulence parameters have been estimated. With time and in the vertical, values vary over four orders of magnitude. They have a dominant local inertial period which is modulated by an about 11 day periodicity associated with variations in a baroclinic unstable boundary current. When this current is strong and Eastward, the upslope phase of inertial wave generates convective turbulence which reaches closest to the bottom and therefore can effect sediment dispersal. In late winter, equally strong shear-induced turbulence in 50 m high Kelvin-Helmholtz (K-H) overturns is forced by 0.2 m s−1 off/downslope motions, which are preceded by periods of warming of a few 0.01°C before the cooler near-bottom water is suddenly flushed over the promontory into the basin. Such anomalously large K-H overturns occurred 6 times in the investigated winter period.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20176" xmlns="http://purl.org/rss/1.0/"><title>Detecting Labrador Sea Water formation from space</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20176</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Detecting Labrador Sea Water formation from space</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">R. Gelderloos, C. A. Katsman, K. Våge</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-25T09:15:33.556421-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20176</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20176</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20176</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2074</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2086</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20176-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> In situ monitoring of deep water formation in the Labrador Sea is severely hampered by the harsh winter conditions in this area. Furthermore, the ongoing monitoring programs do not cover the entire Labrador Sea and are often summer observations. The network of satellite altimeters does not suffer from these limitations and could therefore give valuable additional information. Altimeters can in theory detect deep water formation, because the water column becomes denser during convection and therefore the sea surface becomes lower. This signal is small compared to variability in sea surface height induced by other sources, but when properly filtered and appropriately averaged in time and space, all four winters with Labrador Sea Water formation or renewal in the 1994–2009 period (1994, 1995, 2000, and 2008) have a clear large negative anomaly. The magnitude of this anomaly compares favorably with the range predicted by theory and in situ data analysis. Out of 16 winters, only one winter (2006) would be falsely identified as a deep convection winter based on its sea surface height anomaly signal, while the method did not miss a single deep convection winter. For most deep‒water‒formation winters even the spatial structure of the mixed layer depth distribution can be inferred.</p></div>]]></content:encoded><description>In situ monitoring of deep water formation in the Labrador Sea is severely hampered by the harsh winter conditions in this area. Furthermore, the ongoing monitoring programs do not cover the entire Labrador Sea and are often summer observations. The network of satellite altimeters does not suffer from these limitations and could therefore give valuable additional information. Altimeters can in theory detect deep water formation, because the water column becomes denser during convection and therefore the sea surface becomes lower. This signal is small compared to variability in sea surface height induced by other sources, but when properly filtered and appropriately averaged in time and space, all four winters with Labrador Sea Water formation or renewal in the 1994–2009 period (1994, 1995, 2000, and 2008) have a clear large negative anomaly. The magnitude of this anomaly compares favorably with the range predicted by theory and in situ data analysis. Out of 16 winters, only one winter (2006) would be falsely identified as a deep convection winter based on its sea surface height anomaly signal, while the method did not miss a single deep convection winter. For most deep‒water‒formation winters even the spatial structure of the mixed layer depth distribution can be inferred.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20178" xmlns="http://purl.org/rss/1.0/"><title>Mechanisms of aerosol-forced AMOC variability in a state of the art climate model</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20178</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Mechanisms of aerosol-forced AMOC variability in a state of the art climate model</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Matthew B. Menary, Christopher D. Roberts, Matthew D. Palmer, Paul R. Halloran, Laura Jackson, Richard A. Wood, Wolfgang A. Müller, Daniela Matei, Sang-Ki Lee</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-25T10:47:32.280783-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20178</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20178</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20178</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2087</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2096</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[
<h3 xhtml="http://www.w3.org/1999/xhtml" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib">Abstract</h3><div class="para" id="jgrc20178-para-0001" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Mechanisms of sustained multidecadal changes in the strength of the Atlantic Meridional Overturning Circulation (AMOC) are investigated in a set of simulations with a new state-of-the-art Earth system model. Anthropogenic aerosols have previously been highlighted as a potential mitigator of AMOC weakening. In this study, we explain the oceanic mechanisms behind how anthropogenic aerosols force a strengthening of the AMOC by up to 20% in our state-of-the-art Earth system model. This strengthening is driven via atmospheric circulation changes which subsequently modulate the salinity budget of the North Atlantic subpolar gyre. Gradual salinification occurs via increased evaporation and decreased fluxes of ice through the Fram Straits. A component of the salinification is a positive feedback from the AMOC bringing more saline water northwards from the subtropical Atlantic. Salinification of the subpolar gyre results in increased deep convection and a strengthening of the AMOC. Following a reduction in aerosol concentrations, the AMOC rapidly weakens, approximately 3 times faster than in the case where anthropogenic aerosol concentrations had never been increased. Similarities and differences with available observational records and long term reanalysis products are also discussed.</p></div>]]></content:encoded><description>
Mechanisms of sustained multidecadal changes in the strength of the Atlantic Meridional Overturning Circulation (AMOC) are investigated in a set of simulations with a new state-of-the-art Earth system model. Anthropogenic aerosols have previously been highlighted as a potential mitigator of AMOC weakening. In this study, we explain the oceanic mechanisms behind how anthropogenic aerosols force a strengthening of the AMOC by up to 20% in our state-of-the-art Earth system model. This strengthening is driven via atmospheric circulation changes which subsequently modulate the salinity budget of the North Atlantic subpolar gyre. Gradual salinification occurs via increased evaporation and decreased fluxes of ice through the Fram Straits. A component of the salinification is a positive feedback from the AMOC bringing more saline water northwards from the subtropical Atlantic. Salinification of the subpolar gyre results in increased deep convection and a strengthening of the AMOC. Following a reduction in aerosol concentrations, the AMOC rapidly weakens, approximately 3 times faster than in the case where anthropogenic aerosol concentrations had never been increased. Similarities and differences with available observational records and long term reanalysis products are also discussed.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20150" xmlns="http://purl.org/rss/1.0/"><title>Vertical structure and temporal evolution of an anticyclonic eddy in the Balearic Sea (western Mediterranean)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20150</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Vertical structure and temporal evolution of an anticyclonic eddy in the Balearic Sea (western Mediterranean)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Angel Amores, Sebastià Monserrat, Marta Marcos</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-26T09:02:28.568826-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20150</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20150</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20150</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2097</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2106</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> An anticyclonic eddy in the Balearic Sea (western Mediterranean) was described using data from a mooring line deployed at the northern slope of Mallorca Island at about 900 m deep. Its surface signature was investigated using sea surface height and sea surface temperature images. The eddy, which lasted around 1 month, modified the thermohaline characteristics and the currents of the entire water column. Levantine Intermediate Waters, usually resident in the region, were displaced by colder and fresher Western Mediterranean Intermediate Waters associated with the eddy. Along-slope main currents (toward NE) were completely reversed at 500 m and significantly deviated at 900 m. Interestingly, near-bottom velocities were found to be systematically larger than those at intermediate depths. Furthermore, during the eddy, velocities reached values up to 26 cm/s at the bottom, 5 times larger than the bottom average speed. The recurrence of the phenomenon was explored with an eddy detection tool applied to satellite observations. Results indicated that anticyclonic eddies are common structures in the Balearic Current.</p></div>]]></content:encoded><description>An anticyclonic eddy in the Balearic Sea (western Mediterranean) was described using data from a mooring line deployed at the northern slope of Mallorca Island at about 900 m deep. Its surface signature was investigated using sea surface height and sea surface temperature images. The eddy, which lasted around 1 month, modified the thermohaline characteristics and the currents of the entire water column. Levantine Intermediate Waters, usually resident in the region, were displaced by colder and fresher Western Mediterranean Intermediate Waters associated with the eddy. Along-slope main currents (toward NE) were completely reversed at 500 m and significantly deviated at 900 m. Interestingly, near-bottom velocities were found to be systematically larger than those at intermediate depths. Furthermore, during the eddy, velocities reached values up to 26 cm/s at the bottom, 5 times larger than the bottom average speed. The recurrence of the phenomenon was explored with an eddy detection tool applied to satellite observations. Results indicated that anticyclonic eddies are common structures in the Balearic Current.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20170" xmlns="http://purl.org/rss/1.0/"><title>Multiple jets in the Malvinas Current</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20170</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Multiple jets in the Malvinas Current</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Alberto R. Piola, Bárbara C. Franco, Elbio D. Palma, Martín Saraceno</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-26T14:22:16.82236-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20170</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20170</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20170</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2107</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2117</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The velocity structure of the Malvinas Current is described based on the analysis of high-resolution hydrographic data and direct current observations. The data show that though the current width exceeds 150 km, the flow is concentrated in two relatively narrow (~10–20 km) jets. Within these cores, the direct observations indicate surface velocities exceeding 0.5 m.s<sup>−1</sup>. Surface drifter, satellite-derived mean dynamic topography, and sea surface temperature data suggest that the high-velocity jets are also ubiquitous features of the time mean circulation. Both jets appear to be continuous features extending more than 900 km along the western slope of the Argentine Basin. These jets closely follow the 200 and 1400 m isobaths. Additional high-velocity cores are apparent in direct current measurements and hydrographic observations, but these features are weaker and not continuous along the slope. Though the Malvinas Current transport is mostly barotropic, baroclinic jets are also identified in relative geostrophic velocity sections. The baroclinic jets are colocated with the barotropic jets. Our results suggest that the main Malvinas Current core is located over a relatively flat portion of the bottom, referred to as the Perito Moreno terrace. This observation is in agreement with recent seismic and geological evidence suggesting that in geological time scales the Malvinas Current played a key role in the configuration of the bottom sediments over the western slope of the Argentine Basin.</p></div>]]></content:encoded><description>The velocity structure of the Malvinas Current is described based on the analysis of high-resolution hydrographic data and direct current observations. The data show that though the current width exceeds 150 km, the flow is concentrated in two relatively narrow (~10–20 km) jets. Within these cores, the direct observations indicate surface velocities exceeding 0.5 m.s−1. Surface drifter, satellite-derived mean dynamic topography, and sea surface temperature data suggest that the high-velocity jets are also ubiquitous features of the time mean circulation. Both jets appear to be continuous features extending more than 900 km along the western slope of the Argentine Basin. These jets closely follow the 200 and 1400 m isobaths. Additional high-velocity cores are apparent in direct current measurements and hydrographic observations, but these features are weaker and not continuous along the slope. Though the Malvinas Current transport is mostly barotropic, baroclinic jets are also identified in relative geostrophic velocity sections. The baroclinic jets are colocated with the barotropic jets. Our results suggest that the main Malvinas Current core is located over a relatively flat portion of the bottom, referred to as the Perito Moreno terrace. This observation is in agreement with recent seismic and geological evidence suggesting that in geological time scales the Malvinas Current played a key role in the configuration of the bottom sediments over the western slope of the Argentine Basin.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20086" xmlns="http://purl.org/rss/1.0/"><title>The settling velocity of mineral, biomineral, and biological particles and aggregates in water</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20086</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The settling velocity of mineral, biomineral, and biological particles and aggregates in water</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Federico Maggi</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-29T08:38:48.61718-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20086</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20086</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20086</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2118</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2132</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> A new equation was developed to relate the size and settling velocity of particulate matter commonly recurring in aqueous ecosystems. This equation explicitly balanced the gravitational, buoyancy, viscous, and inertial forces as in Rubey (<a href="#jgrc20086-bib-0058" rel="references:#jgrc20086-bib-0058"/>) but was amended to describe in one instance both individual particles and granular aggregates with an internal fractal architecture. This approach allowed for an algebraic solution of the settling velocity, thus overcoming earlier approaches that required iterative numerical solutions. The equation was tested with mineral, biomineral, and biological suspended particles and granular aggregates from 52 existing experimental data sets, and resulted in average correlation coefficients R between 71% and 93.9%, and normilized residuals between 14.3% and 24.8% over Reynolds numbers ranging within 10<sup>−7</sup> and 10<sup>2</sup>. Accuracy of these results was generally better than for the Stokes' law, the Stokes' law modified with the Schiller-Naumann drag coefficient, and Rubey's equation. Estimated parameters ranged within observed ones, thus suggesting that the equation was robust. An analysis of the drag showed that inertial force was negligible only for biological cells (isolated cysts), whereas it contributed by not less than 5% to the drag on large mineral particles and up to 20% for biomineral and biological aggregates. Finally, a correlation was found between the organic matter content and fractal properties of granular aggregates, which were described by empirical equations proposed here for the first time. The hypothesis that the settling velocity is a function of linear and nonlinear drag, and is ultimately determined by physical characteristics as much as biological composition and internal aggregate geometry, is supported here by quantitative analyses.</p></div>]]></content:encoded><description>A new equation was developed to relate the size and settling velocity of particulate matter commonly recurring in aqueous ecosystems. This equation explicitly balanced the gravitational, buoyancy, viscous, and inertial forces as in Rubey () but was amended to describe in one instance both individual particles and granular aggregates with an internal fractal architecture. This approach allowed for an algebraic solution of the settling velocity, thus overcoming earlier approaches that required iterative numerical solutions. The equation was tested with mineral, biomineral, and biological suspended particles and granular aggregates from 52 existing experimental data sets, and resulted in average correlation coefficients R between 71% and 93.9%, and normilized residuals between 14.3% and 24.8% over Reynolds numbers ranging within 10−7 and 102. Accuracy of these results was generally better than for the Stokes' law, the Stokes' law modified with the Schiller-Naumann drag coefficient, and Rubey's equation. Estimated parameters ranged within observed ones, thus suggesting that the equation was robust. An analysis of the drag showed that inertial force was negligible only for biological cells (isolated cysts), whereas it contributed by not less than 5% to the drag on large mineral particles and up to 20% for biomineral and biological aggregates. Finally, a correlation was found between the organic matter content and fractal properties of granular aggregates, which were described by empirical equations proposed here for the first time. The hypothesis that the settling velocity is a function of linear and nonlinear drag, and is ultimately determined by physical characteristics as much as biological composition and internal aggregate geometry, is supported here by quantitative analyses.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20101" xmlns="http://purl.org/rss/1.0/"><title>Canadian Basin freshwater sources and changes: Results from the 2005 Arctic Ocean Section</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20101</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Canadian Basin freshwater sources and changes: Results from the 2005 Arctic Ocean Section</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Robert Newton, Peter Schlosser, Richard Mortlock, James Swift, Robie MacDonald</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-29T08:50:29.668707-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20101</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20101</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20101</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2133</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2154</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> We present measurements of oxygen isotope ratios and nutrient concentrations along the 2005 Arctic Ocean Section aboard the icebreaker Oden. The data are used to estimate freshwater contributions from meteoric water (mainly river runoff), sea-ice meltwater, and Chukchi Sea shelf water, itself a combination of Pacific and indigenous Arctic water types. Nutrients ratios are combined to form quasi-conservative water-mass tracers (phosphate-star, N-star, and the empirical Arctic N-P relationship) and used along with salinity and δ<sup>18</sup>O, which are conservative in the ocean interior. Disagreements between two different freshwater analyses in the Western Arctic are largely resolved using a salinity-dependent Redfield ratio, a new estimate of the Pacific end-member, and an analysis of the Bering Strait inflow contribution to detraining shelf waters. Freshwater components from 2005 are placed into the context of the overlapping 1994 Arctic Ocean Section (aboard the Louis St. Laurent) and a time series of hydrographic/tracer casts between 1987 and 1992 in the Canada Basin. Compared to 1987–1994; the 2005 transect exhibits increased meteoric water concentrations in the northern part of the Canadian Basin and a decrease in the southern part. This pattern is related to changes in the distribution of wind-stress curl during the several years prior to each sampling campaign. In addition, a previously observed correlation between sea-ice formation and river runoff disappears over the Central Arctic in 2005, a change that we attribute to a northward shift of sea-ice formation. Resampling approximately every 3 years should resolve the dynamics driving changes in freshwater and nutrient distributions.</p></div>]]></content:encoded><description>We present measurements of oxygen isotope ratios and nutrient concentrations along the 2005 Arctic Ocean Section aboard the icebreaker Oden. The data are used to estimate freshwater contributions from meteoric water (mainly river runoff), sea-ice meltwater, and Chukchi Sea shelf water, itself a combination of Pacific and indigenous Arctic water types. Nutrients ratios are combined to form quasi-conservative water-mass tracers (phosphate-star, N-star, and the empirical Arctic N-P relationship) and used along with salinity and δ18O, which are conservative in the ocean interior. Disagreements between two different freshwater analyses in the Western Arctic are largely resolved using a salinity-dependent Redfield ratio, a new estimate of the Pacific end-member, and an analysis of the Bering Strait inflow contribution to detraining shelf waters. Freshwater components from 2005 are placed into the context of the overlapping 1994 Arctic Ocean Section (aboard the Louis St. Laurent) and a time series of hydrographic/tracer casts between 1987 and 1992 in the Canada Basin. Compared to 1987–1994; the 2005 transect exhibits increased meteoric water concentrations in the northern part of the Canadian Basin and a decrease in the southern part. This pattern is related to changes in the distribution of wind-stress curl during the several years prior to each sampling campaign. In addition, a previously observed correlation between sea-ice formation and river runoff disappears over the Central Arctic in 2005, a change that we attribute to a northward shift of sea-ice formation. Resampling approximately every 3 years should resolve the dynamics driving changes in freshwater and nutrient distributions.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20115" xmlns="http://purl.org/rss/1.0/"><title>A model based on stacked-constraints approach for partitioning the light absorption coefficient of seawater into phytoplankton and non-phytoplankton components</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20115</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A model based on stacked-constraints approach for partitioning the light absorption coefficient of seawater into phytoplankton and non-phytoplankton components</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Guangming Zheng, Dariusz Stramski</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-29T08:37:32.664956-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20115</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20115</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20115</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2155</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2174</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Partitioning of the total non-water absorption coefficient of seawater, <em>a</em><sub><em>nw</em></sub>(λ) (i.e., the light absorption coefficient after subtraction of pure water contribution), into phytoplankton, <em>a</em><sub><em>ph</em></sub>(λ), and non-phytoplankton, <em>a</em><sub><em>dg</em></sub>(λ), components is important in the areas of ocean optics, biology, and biogeochemistry. We propose a partitioning model based on stacked-constraints approach, which requires input of <em>a</em><sub><em>nw</em></sub>(λ) at a minimum of six specific light wavelengths. Compared with existing models, our approach requires much less restrictive assumptions about the spectral slope of <em>a</em><sub><em>dg</em></sub>(λ) and the spectral shape of <em>a</em><sub><em>ph</em></sub>(λ). Our model is based on several inequality constraints determined from an extensive, quality-verified set of field data covering oceanic and coastal waters from low to high-latitudes. With these constraints, the model first derives a wide range of speculative solutions for <em>a</em><sub><em>dg</em></sub>(λ) and <em>a</em><sub><em>ph</em></sub>(λ) and then identifies feasible solutions. Final model outputs include the optimal solution and a range of feasible solutions for <em>a</em><sub><em>dg</em></sub>(λ) and <em>a</em><sub><em>ph</em></sub>(λ). The optimal solutions agree well with measurements. For example, the median ratio of the model-derived optimal solutions to measured <em>a</em><sub><em>dg</em></sub>(λ) and <em>a</em><sub><em>ph</em></sub>(λ) at 443 nm is very close to 1, i.e., 1.004 and 0.988, respectively. The median absolute percent difference between the optimal solutions and measured values of <em>a</em><sub><em>dg</em></sub>(443) and <em>a</em><sub><em>ph</em></sub>(443) is 6.5% and 12%, respectively. The range of feasible solutions encompasses the measured <em>a</em><sub><em>dg</em></sub>(λ) and <em>a</em><sub><em>ph</em></sub>(λ) with a probability &gt;90% at most wavelengths. Our results support the prospect for the applications of the partitioning model using the input data of <em>a</em><sub><em>nw</em></sub>(λ) collected from various oceanographic and remote-sensing platforms.</p></div>]]></content:encoded><description>Partitioning of the total non-water absorption coefficient of seawater, anw(λ) (i.e., the light absorption coefficient after subtraction of pure water contribution), into phytoplankton, aph(λ), and non-phytoplankton, adg(λ), components is important in the areas of ocean optics, biology, and biogeochemistry. We propose a partitioning model based on stacked-constraints approach, which requires input of anw(λ) at a minimum of six specific light wavelengths. Compared with existing models, our approach requires much less restrictive assumptions about the spectral slope of adg(λ) and the spectral shape of aph(λ). Our model is based on several inequality constraints determined from an extensive, quality-verified set of field data covering oceanic and coastal waters from low to high-latitudes. With these constraints, the model first derives a wide range of speculative solutions for adg(λ) and aph(λ) and then identifies feasible solutions. Final model outputs include the optimal solution and a range of feasible solutions for adg(λ) and aph(λ). The optimal solutions agree well with measurements. For example, the median ratio of the model-derived optimal solutions to measured adg(λ) and aph(λ) at 443 nm is very close to 1, i.e., 1.004 and 0.988, respectively. The median absolute percent difference between the optimal solutions and measured values of adg(443) and aph(443) is 6.5% and 12%, respectively. The range of feasible solutions encompasses the measured adg(λ) and aph(λ) with a probability &gt;90% at most wavelengths. Our results support the prospect for the applications of the partitioning model using the input data of anw(λ) collected from various oceanographic and remote-sensing platforms.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20153" xmlns="http://purl.org/rss/1.0/"><title>Formation and entrainment of fluid mud layers in troughs of subtidal dunes in an estuarine turbidity zone</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20153</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Formation and entrainment of fluid mud layers in troughs of subtidal dunes in an estuarine turbidity zone</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Marius Becker, Kerstin Schrottke, Alexander Bartholomä, Verner Ernstsen, Christian Winter, Dierk Hebbeln</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-29T09:25:56.479228-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20153</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20153</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20153</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2175</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2187</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The formation and entrainment of fluid mud layers in troughs of subtidal dunes were investigated in the Weser Estuary, North Sea, Germany, based on hydroacoustic measurements. Near-bed suspension layers were found to consist of a suspension of large mud flocs of variable concentration, ranging from 25 g/L below the lutocline to 70 g/L at the river bed, whereas the gelling concentration was below 70 g/L. Sites of fluid mud formation coincided with the location of the estuarine turbidity zone during slack water. On average, near-bed density gradients were initially observed in dune troughs 1.2 h before slack water, and all fluid mud layers were entrained 2.3 h after slack water. No shear instabilities occurred until 1.8 h after slack water. While the flow was oriented in the dune direction, rapid entrainment was related to the development of the turbulent flow field behind dunes and is explained to be induced by advection of strong turbulence during accelerating currents. Fluid mud layers in dune troughs were entrained at an earlier point in time after slack water, compared to adjacent layers formed on a comparatively flat bed, where dune crests did not protrude from the lutocline.</p></div>]]></content:encoded><description>The formation and entrainment of fluid mud layers in troughs of subtidal dunes were investigated in the Weser Estuary, North Sea, Germany, based on hydroacoustic measurements. Near-bed suspension layers were found to consist of a suspension of large mud flocs of variable concentration, ranging from 25 g/L below the lutocline to 70 g/L at the river bed, whereas the gelling concentration was below 70 g/L. Sites of fluid mud formation coincided with the location of the estuarine turbidity zone during slack water. On average, near-bed density gradients were initially observed in dune troughs 1.2 h before slack water, and all fluid mud layers were entrained 2.3 h after slack water. No shear instabilities occurred until 1.8 h after slack water. While the flow was oriented in the dune direction, rapid entrainment was related to the development of the turbulent flow field behind dunes and is explained to be induced by advection of strong turbulence during accelerating currents. Fluid mud layers in dune troughs were entrained at an earlier point in time after slack water, compared to adjacent layers formed on a comparatively flat bed, where dune crests did not protrude from the lutocline.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20125" xmlns="http://purl.org/rss/1.0/"><title>Surf zone cross-shore boundary layer velocity asymmetry and skewness: An experimental study on a mobile bed</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20125</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Surf zone cross-shore boundary layer velocity asymmetry and skewness: An experimental study on a mobile bed</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C. Berni, E. Barthélemy, H. Michallet</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T11:18:17.83362-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20125</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20125</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20125</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2188</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2200</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20125-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> An experimental study on a physical model of a beach in a two-dimensional wave flume was designed to investigate velocity nonlinearities in the wave boundary layer. The cross-shore velocity was measured in the surf zone along a vertical profile every 3mm from free-stream elevation down to the still bed level. The skewness and the asymmetry of the phase averaged velocity were computed at each elevation. Observations indicate that the free-stream asymmetry transforms into bottom velocity skewness. A linear experimental relation between free-stream asymmetry to skewness ratio and bottom skewness to free-stream skewness ratio is established. A theoretical linear relationship is discussed, which predicts the phase lead of the bottom velocity. This phase lead is also determined by Fourier analyzing the velocity time series. The first two Fourier components yield the same phase lead at the bed that is found to be about 30° and nearly constant over all the experiments made.</p></div>]]></content:encoded><description>An experimental study on a physical model of a beach in a two-dimensional wave flume was designed to investigate velocity nonlinearities in the wave boundary layer. The cross-shore velocity was measured in the surf zone along a vertical profile every 3mm from free-stream elevation down to the still bed level. The skewness and the asymmetry of the phase averaged velocity were computed at each elevation. Observations indicate that the free-stream asymmetry transforms into bottom velocity skewness. A linear experimental relation between free-stream asymmetry to skewness ratio and bottom skewness to free-stream skewness ratio is established. A theoretical linear relationship is discussed, which predicts the phase lead of the bottom velocity. This phase lead is also determined by Fourier analyzing the velocity time series. The first two Fourier components yield the same phase lead at the bed that is found to be about 30° and nearly constant over all the experiments made.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20174" xmlns="http://purl.org/rss/1.0/"><title>Seasonal variability of water masses and transport on the Antarctic continental shelf and slope in the southeastern Weddell Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20174</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Seasonal variability of water masses and transport on the Antarctic continental shelf and slope in the southeastern Weddell Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jennifer A. Graham, Karen J. Heywood, Cédric P. Chavanne, Paul R. Holland</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T15:37:01.975928-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20174</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20174</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20174</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2201</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2214</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> An array of five moorings was deployed from February 2009 to February 2010 across the Antarctic shelf and slope in the southeastern Weddell Sea (~18°W). Observations demonstrate the key processes responsible for variability in water masses and transport in the region. Rapid fluctuations in temperature and salinity throughout the year are linked with variability in wind stress over the array. This causes the deepening or shoaling of the pycnocline, past the depth of the moorings. In the upper 500 m, the seasonal cycle in salinity shows freshening in autumn, with the strongest freshening at the shallowest mooring (~250 m), furthest on-shelf. The sea ice concentration over the array exceeds 90% during this period and contributes a positive salt flux into the ocean during autumn. Freshening begins during strong along-shore (easterly) winds in late April 2009. This demonstrates that variations in Ekman transport and wind-driven mixing play a key role in determining the salinity of shelf waters around Antarctica. Transport of the Antarctic Slope Current also shows a seasonal cycle with a maximum during late April. Model simulations show the importance of along-shore advection, as the arrival of a fresh anomaly from upstream determines the timing of the salinity minimum at the array. These processes are likely to be important for other regions around the Antarctic continent.</p></div>]]></content:encoded><description>An array of five moorings was deployed from February 2009 to February 2010 across the Antarctic shelf and slope in the southeastern Weddell Sea (~18°W). Observations demonstrate the key processes responsible for variability in water masses and transport in the region. Rapid fluctuations in temperature and salinity throughout the year are linked with variability in wind stress over the array. This causes the deepening or shoaling of the pycnocline, past the depth of the moorings. In the upper 500 m, the seasonal cycle in salinity shows freshening in autumn, with the strongest freshening at the shallowest mooring (~250 m), furthest on-shelf. The sea ice concentration over the array exceeds 90% during this period and contributes a positive salt flux into the ocean during autumn. Freshening begins during strong along-shore (easterly) winds in late April 2009. This demonstrates that variations in Ekman transport and wind-driven mixing play a key role in determining the salinity of shelf waters around Antarctica. Transport of the Antarctic Slope Current also shows a seasonal cycle with a maximum during late April. Model simulations show the importance of along-shore advection, as the arrival of a fresh anomaly from upstream determines the timing of the salinity minimum at the array. These processes are likely to be important for other regions around the Antarctic continent.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20177" xmlns="http://purl.org/rss/1.0/"><title>Impact of bio-optical data assimilation on short-term coupled physical, bio-optical model predictions</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20177</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Impact of bio-optical data assimilation on short-term coupled physical, bio-optical model predictions</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Igor Shulman, Sergey Frolov, Stephanie Anderson, Brad Penta, Rick Gould, Peter Sakalaukus, Sherwin Ladner</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T15:08:30.948894-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20177</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20177</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20177</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2215</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2230</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Data assimilation experiments with the coupled physical, bio-optical model of Monterey Bay are presented. The objective of this study is to investigate whether the assimilation of satellite-derived bio-optical properties can improve the model predictions (phytoplankton population, chlorophyll) in a coastal ocean on time scales of 1–5 days. The Monterey Bay model consists of a physical model based on the Navy Coastal Ocean Model and a biochemical model which includes three nutrients, two phytoplankton groups (diatoms and small phytoplankton), two groups of zooplankton grazers, and two detrital pools. The Navy Coupled Ocean Data Assimilation system is used for the assimilation of physical observations. For the assimilation of bio-optical observations, we used reduced-order Kalman filter with a stationary forecast error covariance. The forecast error covariance is specified in the subspace of the multivariate (bio-optical, physical) empirical orthogonal functions estimated from a monthlong model run. With the assimilation of satellite-derived bio-optical properties (chlorophyll <em>a</em> or absorption due to phytoplankton), the model was able to reproduce intensity and tendencies in subsurface chlorophyll distributions observed at water sample locations in the Monterey Bay, CA. Data assimilation also improved agreement between the observed and model-predicted ratios between diatoms and small phytoplankton populations. Model runs with or without assimilation of satellite-derived bio-optical observations show underestimated values of nitrate as compared to the water sample observations. We found that an instantaneous update of nitrate based on statistical relations between temperature and nitrate corrected the model underestimation of the nitrate fields during the multivariate update.</p></div>]]></content:encoded><description>Data assimilation experiments with the coupled physical, bio-optical model of Monterey Bay are presented. The objective of this study is to investigate whether the assimilation of satellite-derived bio-optical properties can improve the model predictions (phytoplankton population, chlorophyll) in a coastal ocean on time scales of 1–5 days. The Monterey Bay model consists of a physical model based on the Navy Coastal Ocean Model and a biochemical model which includes three nutrients, two phytoplankton groups (diatoms and small phytoplankton), two groups of zooplankton grazers, and two detrital pools. The Navy Coupled Ocean Data Assimilation system is used for the assimilation of physical observations. For the assimilation of bio-optical observations, we used reduced-order Kalman filter with a stationary forecast error covariance. The forecast error covariance is specified in the subspace of the multivariate (bio-optical, physical) empirical orthogonal functions estimated from a monthlong model run. With the assimilation of satellite-derived bio-optical properties (chlorophyll a or absorption due to phytoplankton), the model was able to reproduce intensity and tendencies in subsurface chlorophyll distributions observed at water sample locations in the Monterey Bay, CA. Data assimilation also improved agreement between the observed and model-predicted ratios between diatoms and small phytoplankton populations. Model runs with or without assimilation of satellite-derived bio-optical observations show underestimated values of nitrate as compared to the water sample observations. We found that an instantaneous update of nitrate based on statistical relations between temperature and nitrate corrected the model underestimation of the nitrate fields during the multivariate update.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20160" xmlns="http://purl.org/rss/1.0/"><title>The Eastern Mediterranean Sea biogeochemical dynamics in the 1990s: A numerical study</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20160</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The Eastern Mediterranean Sea biogeochemical dynamics in the 1990s: A numerical study</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Gelsomina Mattia, Marco Zavatarelli, Marcello Vichi, Paolo Oddo</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T19:23:18.867049-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20160</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20160</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20160</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2231</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2248</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> The coupled physical-biogeochemical dynamics of the Mediterranean Sea have been hindcasted for the decade 1990–2000 with the Nucleus for European Modeling of the Ocean-Biogeochemical Flux Model coupled modeling system. This work describes and discusses the simulated changes in the Eastern Mediterranean Sea physical and biogeochemical dynamics occurring in the 1990s, contemporary to the establishment of the Eastern Mediterranean Transient. The physical component of the modeling system reproduces several changes in the Eastern Mediterranean physical dynamics and thermohaline structure that are consistent with observations pertinent to the transient period. The simulated change in the atmospheric forcing during the early 1990s is considered sufficient to develop upwelling favorable conditions that determine an overall upward displacement of the simulated deep Eastern Mediterranean nutrient pool. Model results indicate that in the post transient period, the displaced nutrients were advected westward along with the reestablishment of the Levantine Intermediate Water pathway, and together with the occurrence of strong winter mixing events in the Ionian Sea, they determined an increase of the primary production processes in the euphotic layer along the eastern coast of Ionian Sea and northern Levantine basin. The biogeochemical model suggests that such an increase in productivity apparently impacted mostly the microbial branch of the marine trophic web.</p></div>]]></content:encoded><description>The coupled physical-biogeochemical dynamics of the Mediterranean Sea have been hindcasted for the decade 1990–2000 with the Nucleus for European Modeling of the Ocean-Biogeochemical Flux Model coupled modeling system. This work describes and discusses the simulated changes in the Eastern Mediterranean Sea physical and biogeochemical dynamics occurring in the 1990s, contemporary to the establishment of the Eastern Mediterranean Transient. The physical component of the modeling system reproduces several changes in the Eastern Mediterranean physical dynamics and thermohaline structure that are consistent with observations pertinent to the transient period. The simulated change in the atmospheric forcing during the early 1990s is considered sufficient to develop upwelling favorable conditions that determine an overall upward displacement of the simulated deep Eastern Mediterranean nutrient pool. Model results indicate that in the post transient period, the displaced nutrients were advected westward along with the reestablishment of the Levantine Intermediate Water pathway, and together with the occurrence of strong winter mixing events in the Ionian Sea, they determined an increase of the primary production processes in the euphotic layer along the eastern coast of Ionian Sea and northern Levantine basin. The biogeochemical model suggests that such an increase in productivity apparently impacted mostly the microbial branch of the marine trophic web.</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20169" xmlns="http://purl.org/rss/1.0/"><title>Sediment-generated noise and bed stress in a tidal channel</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20169</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sediment-generated noise and bed stress in a tidal channel</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Christopher Bassett, Jim Thomson, Brian Polagye</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-30T19:25:36.178985-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1002/jgrc.20169</dc:identifier><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc.</dc:publisher><prism:doi xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">10.1002/jgrc.20169</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fjgrc.20169</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Regular Article</prism:section><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2249</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2265</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[<div class="para" id="jgrc20169-para-0001" xmlns:ol="http://www.wiley.com/namespaces/ol/xsl-lib" xmlns="http://www.w3.org/1999/xhtml"><p><span class="paraNumber">[1]</span> Tidally driven currents and bed stresses can result in noise generated by moving sediments. At a site in Admiralty Inlet, Puget Sound, Washington State (USA), peak bed stresses exceed 20 Pa. Significant increases in noise levels are attributed to mobilized sediments at frequencies from 4–30 kHz with more modest increases noted from 1–4 kHz. Sediment-generated noise during strong currents masks background noise from other sources, including vessel traffic. Inversions of the acoustic spectra for equivalent grain sizes are consistent with qualitative data of the seabed composition. Bed stress calculations using log layer, Reynolds stress, and inertial dissipation techniques generally agree well and are used to estimate the shear stresses at which noise levels increase for different grain sizes. Regressions of the acoustic intensity versus near-bed hydrodynamic power demonstrate that noise levels are highly predictable above a critical threshold despite the scatter introduced by the localized nature of mobilization events.</p></div>]]></content:encoded><description>Tidally driven currents and bed stresses can result in noise generated by moving sediments. At a site in Admiralty Inlet, Puget Sound, Washington State (USA), peak bed stresses exceed 20 Pa. Significant increases in noise levels are attributed to mobilized sediments at frequencies from 4–30 kHz with more modest increases noted from 1–4 kHz. Sediment-generated noise during strong currents masks background noise from other sources, including vessel traffic. Inversions of the acoustic spectra for equivalent grain sizes are consistent with qualitative data of the seabed composition. Bed stress calculations using log layer, Reynolds stress, and inertial dissipation techniques generally agree well and are used to estimate the shear stresses at which noise levels increase for different grain sizes. Regressions of the acoustic intensity versus near-bed hydrodynamic power demonstrate that noise levels are highly predictable above a critical threshold despite the scatter introduced by the localized nature of mobilization events.</description></item></rdf:RDF>