<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"><channel rdf:about="http://onlinelibrary.wiley.com/rss/journal/10.1111/(ISSN)1365-3091" xmlns="http://purl.org/rss/1.0/"><title>Sedimentology</title><description> Wiley Online Library : Sedimentology</description><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2F%28ISSN%291365-3091</link><dc:publisher xmlns:dc="http://purl.org/dc/elements/1.1/">John Wiley &amp; Sons, Inc</dc:publisher><dc:language xmlns:dc="http://purl.org/dc/elements/1.1/">en</dc:language><dc:rights xmlns:dc="http://purl.org/dc/elements/1.1/">© International Association of Sedimentologists</dc:rights><prism:issn xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">0037-0746</prism:issn><prism:eIssn xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">1365-3091</prism:eIssn><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-02-01T00:00:00-05:00</dc:date><prism:coverDisplayDate xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">February 2013</prism:coverDisplayDate><prism:volume xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">60</prism:volume><prism:number xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">2</prism:number><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">359</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">636</prism:endingPage><image rdf:resource="http://onlinelibrary.wiley.com/store/10.1111/sed.2013.60.issue-2/asset/cover.gif?v=1&amp;s=cffd59ebd3044af3e5a2486af3983618d1d18ee5"/><items><rdf:Seq><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12057"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12056"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12055"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12054"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12053"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12052"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12051"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12046"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12044"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12045"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12041"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12037"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12035"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12028"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12036"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12040"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12042"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12043"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12029"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12030"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12039"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12032"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12031"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12033"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12038"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12026"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12025"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12027"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12024"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01344.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01345.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01346.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01347.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01348.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01349.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01350.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01351.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01352.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01363.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01362.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01360.x"/><rdf:li rdf:resource="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12034"/></rdf:Seq></items></channel><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12057" xmlns="http://purl.org/rss/1.0/"><title>A numerical study of particle motion and two-phase interaction in aeolian sand transport using a coupled large eddy simulation – discrete element method</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12057</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">A numerical study of particle motion and two-phase interaction in aeolian sand transport using a coupled large eddy simulation – discrete element method</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Zhiqiang Li, Yuan Wang, Yang Zhang</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-27T09:01:38.78166-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12057</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/">10.1111/sed.12057</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12057</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Wind-blown sand movement, considered as a particle-laden two-phase flow, was simulated by a new numerical code developed in the present study. The discrete element method was employed to model the contact force between sand particles. Large eddy simulation was used to solve the turbulent atmospheric boundary layer. Motions of sand particles were traced in the Lagrangian frame. Within the near-surface region of the atmospheric boundary layer, interparticle collisions will significantly alter the velocity of sand. The sand phase is quite dense in this region, and its feedback force on fluid motion cannot be ignored. By considering the interparticle collision and two-phase interaction, four-way coupling was achieved in the numerical code. Profiles of sand velocity from the simulations were in good agreement with experimental measurements. The mass flux shows an exponential decay and is comparable with reported experimental and field measurements. The turbulence intensities and shear stress of sand particles were estimated from particle root-mean-square velocities. Distributions of slip velocity and feedback force were analyzed to reveal the interactions between sand particles and the continuous fluid phase.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

Wind-blown sand movement, considered as a particle-laden two-phase flow, was simulated by a new numerical code developed in the present study. The discrete element method was employed to model the contact force between sand particles. Large eddy simulation was used to solve the turbulent atmospheric boundary layer. Motions of sand particles were traced in the Lagrangian frame. Within the near-surface region of the atmospheric boundary layer, interparticle collisions will significantly alter the velocity of sand. The sand phase is quite dense in this region, and its feedback force on fluid motion cannot be ignored. By considering the interparticle collision and two-phase interaction, four-way coupling was achieved in the numerical code. Profiles of sand velocity from the simulations were in good agreement with experimental measurements. The mass flux shows an exponential decay and is comparable with reported experimental and field measurements. The turbulence intensities and shear stress of sand particles were estimated from particle root-mean-square velocities. Distributions of slip velocity and feedback force were analyzed to reveal the interactions between sand particles and the continuous fluid phase.
This article is protected by copyright. All rights reserved.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12056" xmlns="http://purl.org/rss/1.0/"><title>An Empirical Model of Subcritical Bedform Migration</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12056</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">An Empirical Model of Subcritical Bedform Migration</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">C.-Y.Martin Lin, Jeremy G. Venditti</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-25T04:10:25.377221-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12056</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/">10.1111/sed.12056</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12056</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 ability to predict bedform migration in rivers is critical for estimating bed material load, yet there is no relation for predicting bedform migration (downstream translation) that covers the full range of conditions under which subcritical bedforms develop. Here, the relation between bedform migration rates and transport stage is explored using a field and several flume data sets. Transport stage is defined as the non-dimensional Shields stress divided by its value at the threshold for sediment entrainment. Statistically significant positive correlations between both ripple and dune migration rates and transport stage are found. Stratification of the data by the flow depth to grain-size ratio improved the amount of variability in migration rates that was explained by transport stage to <em>ca</em> 70%. As transport stage increases for a given depth to grain-size ratio, migration rates increase. For a given transport stage, the migration rate increases as the flow-depth to grain-size ratio gets smaller. In coarser sediment, bedforms move faster than in finer sediment at the same transport stage. Normalization of dune migration rates by the settling velocity of bed sediment partially collapses the data. Given the large amount of variability that arises from combining data sets from different sources, using different equipment, the partial collapse is remarkable and warrants further testing in the laboratory and field.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

The ability to predict bedform migration in rivers is critical for estimating bed material load, yet there is no relation for predicting bedform migration (downstream translation) that covers the full range of conditions under which subcritical bedforms develop. Here, the relation between bedform migration rates and transport stage is explored using a field and several flume data sets. Transport stage is defined as the non-dimensional Shields stress divided by its value at the threshold for sediment entrainment. Statistically significant positive correlations between both ripple and dune migration rates and transport stage are found. Stratification of the data by the flow depth to grain-size ratio improved the amount of variability in migration rates that was explained by transport stage to ca 70%. As transport stage increases for a given depth to grain-size ratio, migration rates increase. For a given transport stage, the migration rate increases as the flow-depth to grain-size ratio gets smaller. In coarser sediment, bedforms move faster than in finer sediment at the same transport stage. Normalization of dune migration rates by the settling velocity of bed sediment partially collapses the data. Given the large amount of variability that arises from combining data sets from different sources, using different equipment, the partial collapse is remarkable and warrants further testing in the laboratory and field.
This article is protected by copyright. All rights reserved.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12055" xmlns="http://purl.org/rss/1.0/"><title>Depositional processes on oceanic island shelves – evidence from storm-generated Neogene deposits from the mid-North Atlantic</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12055</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Depositional processes on oceanic island shelves – evidence from storm-generated Neogene deposits from the mid-North Atlantic</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Ricardo P. Meireles, Rui Quartau, Ricardo S. Ramalho, Ana C. Rebelo, José Madeira, Vittorio Zanon, Sérgio P. Ávila</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-20T01:58:22.223426-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12055</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/">10.1111/sed.12055</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12055</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Oceanic islands - such as the Azores in the mid-North Atlantic - are periodically exposed to large storms that often remobilize and transport marine sediments along coastlines, and into deeper environments. Such disruptive events create deposits – denominated tempestites – whose characteristics reflect the highly dynamic environment in which they were formed. Tempestites from oceanic islands, however, are seldom described in the literature and little is known about storm-related sediment dynamics affecting oceanic island shelves. Therefore, the geological record of tempestite deposits at oceanic islands can provide invaluable information on the processes of sediment remobilization, transport and deposition taking place on insular shelves during and after major storms. In Santa Maria Island (Azores), a sequence of Neogene tempestite deposits was incorporated in the island edifice by the ongoing volcanic activity (thus preserved) and later exposed through uplift and erosion. Since it was overlain by a contemporary coastal lava delta, the water depth at the time of deposition could be inferred, constituting an excellent case-study to gain insight on the still enigmatic processes of insular shelf deposition. Sedimentological, palaeontological, petrographic and palaeo-water depth information, allowed the reconstruction of the depositional environment of these sediments. The sequence typifies the characteristics of a tempestite (or successive tempestites) formed at <em>ca</em> 50 m depth, in a steep, energetic open insular shelf, and with evidence for massive sediment remobilization from the nearshore to the middle or outer shelf. The authors claim that cross-shelf transport induced by storm events is the main process of sediment deposition acting on steep and narrow shelves subjected to high energetic environments, such as the insular shelves of open-sea volcanic islands.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

Oceanic islands - such as the Azores in the mid-North Atlantic - are periodically exposed to large storms that often remobilize and transport marine sediments along coastlines, and into deeper environments. Such disruptive events create deposits – denominated tempestites – whose characteristics reflect the highly dynamic environment in which they were formed. Tempestites from oceanic islands, however, are seldom described in the literature and little is known about storm-related sediment dynamics affecting oceanic island shelves. Therefore, the geological record of tempestite deposits at oceanic islands can provide invaluable information on the processes of sediment remobilization, transport and deposition taking place on insular shelves during and after major storms. In Santa Maria Island (Azores), a sequence of Neogene tempestite deposits was incorporated in the island edifice by the ongoing volcanic activity (thus preserved) and later exposed through uplift and erosion. Since it was overlain by a contemporary coastal lava delta, the water depth at the time of deposition could be inferred, constituting an excellent case-study to gain insight on the still enigmatic processes of insular shelf deposition. Sedimentological, palaeontological, petrographic and palaeo-water depth information, allowed the reconstruction of the depositional environment of these sediments. The sequence typifies the characteristics of a tempestite (or successive tempestites) formed at ca 50 m depth, in a steep, energetic open insular shelf, and with evidence for massive sediment remobilization from the nearshore to the middle or outer shelf. The authors claim that cross-shelf transport induced by storm events is the main process of sediment deposition acting on steep and narrow shelves subjected to high energetic environments, such as the insular shelves of open-sea volcanic islands.
This article is protected by copyright. All rights reserved.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12054" xmlns="http://purl.org/rss/1.0/"><title>Formation and preservation of an overstepped segmented lagoon complex on a high-energy continental shelf</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12054</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Formation and preservation of an overstepped segmented lagoon complex on a high-energy continental shelf</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Andrew N. Green, J. Andrew G. Cooper, R. Leuci, Z. Thackeray</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-12T10:36:47.001602-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12054</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/">10.1111/sed.12054</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12054</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 duration of shoreline occupation at a given sea-level, coastal response to sea-level change and the controls on preservation of various shoreline elements can be recognised by detailed examination of submerged shorelines on the continental shelf. Using bathymetric and seismic observations, this article documents the evolution and preservation of an incised valley and lithified barrier complex between -65 m and -50 m mean sea-level on a wave-dominated continental shelf. The barrier complex is preserved as a series of aeolianite/beachrock ridges backed by laterally extensive backbarrier sediments. The ridges include prograded cuspate lagoonal shoreline features similar to those found in contemporary lagoons. The incised valley trends shore-parallel behind the barrier complex and records an early phase of valley filling, followed by a phase of extensive lagoonal sedimentation beyond the margins of the incised bedrock valley. Sea-level stability at the outer barrier position (<em>ca</em> -65 m) enabled accumulation of a substantial coastal barrier that remained intact during a phase of subsequent slow sea-level rise to -58 m when the lagoon formed. These lagoonal sediments are stripped seawards by bay ravinement processes which caused the formation of several prograded marginal cuspate features. An abrupt rise in sea-level to -40 m, correlated with melt water pulse 1B, enabled the preservation of thick lagoonal sediments at the top of the incised valley fill and preservation on the sea bed of the cemented core of the barriers. This situation is unique to subtropical coastlines where early diagenesis is possible. The overlying sandy sediment from the uncemented upper portion of the barriers is dispersed by ravinement, partly burying the ridges and protecting the underlying sediments. The high degree of barrier/shoreline preservation is attributed to rapid overstepping of the shoreline, early cementation in favourable climatic conditions and the protection of the barrier cores by sand sheet draping.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

The duration of shoreline occupation at a given sea-level, coastal response to sea-level change and the controls on preservation of various shoreline elements can be recognised by detailed examination of submerged shorelines on the continental shelf. Using bathymetric and seismic observations, this article documents the evolution and preservation of an incised valley and lithified barrier complex between -65 m and -50 m mean sea-level on a wave-dominated continental shelf. The barrier complex is preserved as a series of aeolianite/beachrock ridges backed by laterally extensive backbarrier sediments. The ridges include prograded cuspate lagoonal shoreline features similar to those found in contemporary lagoons. The incised valley trends shore-parallel behind the barrier complex and records an early phase of valley filling, followed by a phase of extensive lagoonal sedimentation beyond the margins of the incised bedrock valley. Sea-level stability at the outer barrier position (ca -65 m) enabled accumulation of a substantial coastal barrier that remained intact during a phase of subsequent slow sea-level rise to -58 m when the lagoon formed. These lagoonal sediments are stripped seawards by bay ravinement processes which caused the formation of several prograded marginal cuspate features. An abrupt rise in sea-level to -40 m, correlated with melt water pulse 1B, enabled the preservation of thick lagoonal sediments at the top of the incised valley fill and preservation on the sea bed of the cemented core of the barriers. This situation is unique to subtropical coastlines where early diagenesis is possible. The overlying sandy sediment from the uncemented upper portion of the barriers is dispersed by ravinement, partly burying the ridges and protecting the underlying sediments. The high degree of barrier/shoreline preservation is attributed to rapid overstepping of the shoreline, early cementation in favourable climatic conditions and the protection of the barrier cores by sand sheet draping.
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</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12053" xmlns="http://purl.org/rss/1.0/"><title>Sedimentology and depositional architecture of tufas deposited in stepped fluvial systems of changing slope: Lessons from the Quaternary Añamaza valley (Iberian Range, Spain)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12053</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Sedimentology and depositional architecture of tufas deposited in stepped fluvial systems of changing slope: Lessons from the Quaternary Añamaza valley (Iberian Range, Spain)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Concha Arenas, Marta Vázquez-Urbez, Gonzalo Pardo, Carlos Sancho</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-12T10:36:35.185582-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12053</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/">10.1111/sed.12053</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12053</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Themed Issue Paper</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 Pleistocene and Holocene tufas of the Añamaza valley (stepped build-ups, up to 70 m thick, along the valley) consist of several depositional stages separated by erosional surfaces. Eight associations of tufa and related carbonate facies, plus minor polygenic detrital facies, represent the processes that occurred in different fluvial and related environments. The bedrock lithology and structure controlled the location of the knickpoints along the valley and allowed to separate two stepped stretches with distinct conceptual facies models. The moderate-slope model includes extensive standing-water areas dammed by barrage-cascades. In the lakes, bioclastic silts, sands and limestones along with phytoclastic and marly, at places peaty, sediments formed. Abundant stem phytoherms account for extensive palustrine areas. The high-slope model consists of smaller dammed areas between close-up cascades and barrage-cascades, which were composed primarily of moss phytoherms and phytoclastic tufas. An outstanding feature is the extensive steep reach with phytoclastic and polygenic detrital sediments, and stepped cascades made of stromatolitic and moss phytoherms. There, the steep slope limited the preservation of stem phytoherms and favoured erosion. The geometry and thickness of the sedimentary fill (wedge-shaped units composed of cascade and barrage-cascade deposits downstream, and dammed and gentle-sloped channel deposits upstream) are therefore different for each model. Multi-storey wedges are a distinctive feature of the high-slope model. The initial knickpoint geometry and the tufa aggradation/progradation ratio on such steep surfaces (for example, related to changes in discharge) controlled the growth style of the cascades or barrage-cascades, and hence, the extent, thickness and vertical evolution of the upstream deposits. The sedimentological attributes and stable-isotope composition of the carbonate facies suggest higher and more variable precipitation/evaporation ratio during the Pleistocene than during the Holocene, consistent with an overall decrease in the river discharge. This evolution was coupled with warm conditions, which prevailed during the stages of tufa formation. These results may help assess architectural patterns in interpreting other basins, and underscore the significance of tufas as records of past hydrology and climate.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

The Pleistocene and Holocene tufas of the Añamaza valley (stepped build-ups, up to 70 m thick, along the valley) consist of several depositional stages separated by erosional surfaces. Eight associations of tufa and related carbonate facies, plus minor polygenic detrital facies, represent the processes that occurred in different fluvial and related environments. The bedrock lithology and structure controlled the location of the knickpoints along the valley and allowed to separate two stepped stretches with distinct conceptual facies models. The moderate-slope model includes extensive standing-water areas dammed by barrage-cascades. In the lakes, bioclastic silts, sands and limestones along with phytoclastic and marly, at places peaty, sediments formed. Abundant stem phytoherms account for extensive palustrine areas. The high-slope model consists of smaller dammed areas between close-up cascades and barrage-cascades, which were composed primarily of moss phytoherms and phytoclastic tufas. An outstanding feature is the extensive steep reach with phytoclastic and polygenic detrital sediments, and stepped cascades made of stromatolitic and moss phytoherms. There, the steep slope limited the preservation of stem phytoherms and favoured erosion. The geometry and thickness of the sedimentary fill (wedge-shaped units composed of cascade and barrage-cascade deposits downstream, and dammed and gentle-sloped channel deposits upstream) are therefore different for each model. Multi-storey wedges are a distinctive feature of the high-slope model. The initial knickpoint geometry and the tufa aggradation/progradation ratio on such steep surfaces (for example, related to changes in discharge) controlled the growth style of the cascades or barrage-cascades, and hence, the extent, thickness and vertical evolution of the upstream deposits. The sedimentological attributes and stable-isotope composition of the carbonate facies suggest higher and more variable precipitation/evaporation ratio during the Pleistocene than during the Holocene, consistent with an overall decrease in the river discharge. This evolution was coupled with warm conditions, which prevailed during the stages of tufa formation. These results may help assess architectural patterns in interpreting other basins, and underscore the significance of tufas as records of past hydrology and climate.
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</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12052" xmlns="http://purl.org/rss/1.0/"><title>Three-dimensional gravity-current flow within a subaqueous bend: Spatial evolution and force balance variations</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12052</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Three-dimensional gravity-current flow within a subaqueous bend: Spatial evolution and force balance variations</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Taoyuan Wei, Jeff Peakall, Daniel R. Parsons, Zhongyuan Chen, Baocheng Zhao, Jim Best</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-11T02:30:11.003471-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12052</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/">10.1111/sed.12052</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12052</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 nature of three-dimensional flow in submarine channel bends is poorly understood, largely due to the absence of detailed data from natural channels. Herein data from density-driven flows in a large reservoir on the Huang He (Yellow) River are presented showing the spatio-temporal variation of flow around a subaqueous bend. The data demonstrate for the first time that reversed helical flow, relative to that found in river channel bends, can occur from the centrifugal forcing of flow, even when the Coriolis force acts in the opposite direction. The data also suggest that reversed helical flow fields in submarine channels may be more frequent than currently estimated, notably for bends where Coriolis and centrifugal forces combine in the same direction. Additionally, this study provides the first field evidence suggesting that sinuous submarine channels can exhibit an asymmetry in helical flow orientation between left and right-turning bends, which will have major implications for the morphodynamics of submarine channels, their resultant patterns of sedimentation and, ultimately, the distribution of depositional units across submarine fan systems.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

The nature of three-dimensional flow in submarine channel bends is poorly understood, largely due to the absence of detailed data from natural channels. Herein data from density-driven flows in a large reservoir on the Huang He (Yellow) River are presented showing the spatio-temporal variation of flow around a subaqueous bend. The data demonstrate for the first time that reversed helical flow, relative to that found in river channel bends, can occur from the centrifugal forcing of flow, even when the Coriolis force acts in the opposite direction. The data also suggest that reversed helical flow fields in submarine channels may be more frequent than currently estimated, notably for bends where Coriolis and centrifugal forces combine in the same direction. Additionally, this study provides the first field evidence suggesting that sinuous submarine channels can exhibit an asymmetry in helical flow orientation between left and right-turning bends, which will have major implications for the morphodynamics of submarine channels, their resultant patterns of sedimentation and, ultimately, the distribution of depositional units across submarine fan systems.
This article is protected by copyright. All rights reserved.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12051" xmlns="http://purl.org/rss/1.0/"><title>Microbiological processes in banded iron formation deposition</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12051</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Microbiological processes in banded iron formation deposition</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">NICOLE R. POSTH, KURT O. KONHAUSER, ANDREAS KAPPLER</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-08T07:24:21.119988-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12051</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/">10.1111/sed.12051</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12051</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Banded iron formations have been studied for decades, particularly regarding their potential as archives of the Precambrian environment. In spite of this effort, the mechanism of their deposition and specifically, the role that microbes played in the precipitation of banded iron formation minerals remains unresolved. Evidence of an anoxic Earth with only localised oxic areas until the Great Oxidation Event <em>ca</em> 2.45 to 2.32 Ga makes the investigation of O<sub>2</sub>-independent mechanisms for banded iron formation deposition relevant. Recent studies have explored the long-standing proposition that Archean banded iron formations may have been formed, and diagenetically modified, by anaerobic microbial metabolisms. These efforts encompass a wide array of approaches including isotope, eco-physiological and phylogeny studies, molecular and mineral marker analysis, and sedimentological reconstructions. Herein, the current theories of microbial processes in banded iron formation mineral deposition with particular regard to the mechanisms of chemical sedimentation and post-depositional alteration are described. The main findings of recent years are summarised and compared here and suggestions are made regarding cross disciplinary information still required to constrain the role of the biosphere in banded iron formation deposition.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>This article is protected by copyright. All rights reserved.</p></div>
]]></content:encoded><description>

Banded iron formations have been studied for decades, particularly regarding their potential as archives of the Precambrian environment. In spite of this effort, the mechanism of their deposition and specifically, the role that microbes played in the precipitation of banded iron formation minerals remains unresolved. Evidence of an anoxic Earth with only localised oxic areas until the Great Oxidation Event ca 2.45 to 2.32 Ga makes the investigation of O2-independent mechanisms for banded iron formation deposition relevant. Recent studies have explored the long-standing proposition that Archean banded iron formations may have been formed, and diagenetically modified, by anaerobic microbial metabolisms. These efforts encompass a wide array of approaches including isotope, eco-physiological and phylogeny studies, molecular and mineral marker analysis, and sedimentological reconstructions. Herein, the current theories of microbial processes in banded iron formation mineral deposition with particular regard to the mechanisms of chemical sedimentation and post-depositional alteration are described. The main findings of recent years are summarised and compared here and suggestions are made regarding cross disciplinary information still required to constrain the role of the biosphere in banded iron formation deposition.
This article is protected by copyright. All rights reserved.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12046" xmlns="http://purl.org/rss/1.0/"><title>Autogenic Incision-Backfilling Cycles and Lobe Formation During the Growth of Alluvial Fans with Supercritical Distributaries</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12046</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Autogenic Incision-Backfilling Cycles and Lobe Formation During the Growth of Alluvial Fans with Supercritical Distributaries</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Paul B. Hamilton, Kyle Strom, David C. J. D. Hoyal</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-23T10:17:06.135911-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12046</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/">10.1111/sed.12046</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12046</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Autogenic cycles of channelization, terminal deposit formation, channel backfilling, and channel abandonment have been observed in the formation of fans and deltas. In subcritical flow, these terminal deposits are characterized as mouth bars that lead to flow bifurcation, backwater, and eventual channel backfilling. Similar, though less well characterized, cycles also take place on supercritical subaerial and submarine fans. This study investigates the hydraulics and morphodynamics of autogenic incision and backfilling cycles associated with supercritical distributive channel flow in alluvial fans. The research questions of the study are: (1) how are supercritical autogenic cycles on alluvial fans different from the subcritical cycles? (2) What are the hydraulic and sediment transport characteristics at the various stages of autogenic feedback cycles? And, (3) what role do the cycles play in the overall fan evolution? These questions are investigated in the laboratory and emphasis is placed on measuring the hydraulic and topographic evolution of the systems during the cycles. The cycles arise quasi-periodically under constant water and sediment discharge. Periods of sheet-like flow are competent to move sediment (<em>t*</em>_ &gt; <em>t</em>*cr) but not competent enough to carry the full imposed load.</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>The net result is preferential deposition near the inlet, resulting in fan steepening and an increase in flow competency with time. At a sediment supply to capacity ratio of Qs/Qc ≈ 0.75, the sheet-like flow is unstable to small erosional events near the inlet resulting in the collapse of the distributed flow to a strong channelized state. During channelization, a graded (Qs/Qc ≈ 1) supercritical (Fr &gt; 1) channel develops and transports eroded and fed sediment up to and through the fan front — extending the fan, initiating a lobe shaped deposit, and reducing the local slope. The slopes defined by a sheet-like flow with Qs/Qc ≈ 0.75 and channelized flow with Qs/Qc ≈ 1 set the maximum and minimum slopes on the fan respectively. Once formed, graded channels act as bypass conduits linking the inlet with the terminal deposit. On average deposits are up to 6 channel depths in thickness and have volumes approximately 5 times that of the excavated channel. The main distinctive characteristics of the supercritical cycles has to do with how the flow interacts with the terminal deposit. At the channel to deposit transition, the flow undergoes a weak hydraulic jump, resulting in rapid sedimentation, dechannelization and lateral expansion of the flow, and deposition of any remaining sediment on top of the channel fill and floodplain. This process often caps the channel as the deposit propagates up channel erasing memory of the excavated channel.</p></div>
]]></content:encoded><description>

Autogenic cycles of channelization, terminal deposit formation, channel backfilling, and channel abandonment have been observed in the formation of fans and deltas. In subcritical flow, these terminal deposits are characterized as mouth bars that lead to flow bifurcation, backwater, and eventual channel backfilling. Similar, though less well characterized, cycles also take place on supercritical subaerial and submarine fans. This study investigates the hydraulics and morphodynamics of autogenic incision and backfilling cycles associated with supercritical distributive channel flow in alluvial fans. The research questions of the study are: (1) how are supercritical autogenic cycles on alluvial fans different from the subcritical cycles? (2) What are the hydraulic and sediment transport characteristics at the various stages of autogenic feedback cycles? And, (3) what role do the cycles play in the overall fan evolution? These questions are investigated in the laboratory and emphasis is placed on measuring the hydraulic and topographic evolution of the systems during the cycles. The cycles arise quasi-periodically under constant water and sediment discharge. Periods of sheet-like flow are competent to move sediment (t*_ &gt; t*cr) but not competent enough to carry the full imposed load.
The net result is preferential deposition near the inlet, resulting in fan steepening and an increase in flow competency with time. At a sediment supply to capacity ratio of Qs/Qc ≈ 0.75, the sheet-like flow is unstable to small erosional events near the inlet resulting in the collapse of the distributed flow to a strong channelized state. During channelization, a graded (Qs/Qc ≈ 1) supercritical (Fr &gt; 1) channel develops and transports eroded and fed sediment up to and through the fan front — extending the fan, initiating a lobe shaped deposit, and reducing the local slope. The slopes defined by a sheet-like flow with Qs/Qc ≈ 0.75 and channelized flow with Qs/Qc ≈ 1 set the maximum and minimum slopes on the fan respectively. Once formed, graded channels act as bypass conduits linking the inlet with the terminal deposit. On average deposits are up to 6 channel depths in thickness and have volumes approximately 5 times that of the excavated channel. The main distinctive characteristics of the supercritical cycles has to do with how the flow interacts with the terminal deposit. At the channel to deposit transition, the flow undergoes a weak hydraulic jump, resulting in rapid sedimentation, dechannelization and lateral expansion of the flow, and deposition of any remaining sediment on top of the channel fill and floodplain. This process often caps the channel as the deposit propagates up channel erasing memory of the excavated channel.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12044" xmlns="http://purl.org/rss/1.0/"><title>Microbial mats implicated in the generation of intrastratal shrinkage (‘synaeresis’) cracks</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12044</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Microbial mats implicated in the generation of intrastratal shrinkage (‘synaeresis’) cracks</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">D. Harazim, R.H.T. Callow, D. Mcilroy</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-16T17:57:49.140305-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12044</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/">10.1111/sed.12044</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12044</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Intrastratal shrinkage (often termed ‘synaeresis’) cracks are commonly employed as diagnostic environmental indicators for ancient salinity-stressed, transitional fluvial-marine or marginal-marine depositional environments. Despite their abundance and use in facies interpretations, the mechanism of synaeresis crack formation remains controversial and widely-accepted explanations for their formation have hitherto been lacking. Sedimentological, ichnological, petrographic and geochemical study of shallow marine mudstone beds from the Ordovician Beach Formation of Bell Island, Newfoundland has revealed that crack development (cf. synaeresis cracks) on the upper surface of mudstone beds is correlated with specific organic, geochemical and sedimentological parameters. Contorted, sinuous, sand-filled cracks are common at contacts between unbioturbated mudstone and overlying sandstone beds. Cracks are absent in highly bioturbated mudstone, and are considered to pre-date firmground assemblages of trace fossils that include <em>Planolites</em> and <em>Trichophycus</em>. The tops of cracked mudstone beds contain up to 2.1 wt% total organic carbon (TOC, wt%), relative to underlying mudstone beds which contain around 0.5 wt% total organic carbon. High-resolution carbon isotope analyses reveal low δ<sup>13</sup>C<sub>org</sub> values (-27.6‰) on bed tops, compared with sandy intervals lacking cracks</p></div>
<div class="para" xmlns="http://www.w3.org/1999/xhtml"><p>(-24.4 to -24.6‰). Cracked mudstone facies show evidence for microbial matgrounds, including microbially induced sedimentary structures on bedding planes and carbonaceous laminae and tubular carbonaceous microfossils in thin section. Non-cracked mudstone lacks evidence for development of microbial mats. Microbial mat development is proposed as an important prerequisite for intrastratal shrinkage crack formation. Both microbial mats and intrastratal shrinkage cracks have broad palaeoenvironmental distributions in the Precambrian and early Phanerozoic. In later Phanerozoic strata, matgrounds are restricted to depositional environments that are inhospitable to burrowing and surface-grazing macrofauna. Unless evidence of synaeresis (i.e. contraction of clay mineral lattices in response to salinity change) can be independently demonstrated, the general term ‘intrastratal shrinkage crack’ is proposed to describe sinuous and tapering cracks in mudstone beds.</p></div>
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Intrastratal shrinkage (often termed ‘synaeresis’) cracks are commonly employed as diagnostic environmental indicators for ancient salinity-stressed, transitional fluvial-marine or marginal-marine depositional environments. Despite their abundance and use in facies interpretations, the mechanism of synaeresis crack formation remains controversial and widely-accepted explanations for their formation have hitherto been lacking. Sedimentological, ichnological, petrographic and geochemical study of shallow marine mudstone beds from the Ordovician Beach Formation of Bell Island, Newfoundland has revealed that crack development (cf. synaeresis cracks) on the upper surface of mudstone beds is correlated with specific organic, geochemical and sedimentological parameters. Contorted, sinuous, sand-filled cracks are common at contacts between unbioturbated mudstone and overlying sandstone beds. Cracks are absent in highly bioturbated mudstone, and are considered to pre-date firmground assemblages of trace fossils that include Planolites and Trichophycus. The tops of cracked mudstone beds contain up to 2.1 wt% total organic carbon (TOC, wt%), relative to underlying mudstone beds which contain around 0.5 wt% total organic carbon. High-resolution carbon isotope analyses reveal low δ13Corg values (-27.6‰) on bed tops, compared with sandy intervals lacking cracks
(-24.4 to -24.6‰). Cracked mudstone facies show evidence for microbial matgrounds, including microbially induced sedimentary structures on bedding planes and carbonaceous laminae and tubular carbonaceous microfossils in thin section. Non-cracked mudstone lacks evidence for development of microbial mats. Microbial mat development is proposed as an important prerequisite for intrastratal shrinkage crack formation. Both microbial mats and intrastratal shrinkage cracks have broad palaeoenvironmental distributions in the Precambrian and early Phanerozoic. In later Phanerozoic strata, matgrounds are restricted to depositional environments that are inhospitable to burrowing and surface-grazing macrofauna. Unless evidence of synaeresis (i.e. contraction of clay mineral lattices in response to salinity change) can be independently demonstrated, the general term ‘intrastratal shrinkage crack’ is proposed to describe sinuous and tapering cracks in mudstone beds.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12045" xmlns="http://purl.org/rss/1.0/"><title>Intrinsic and extrinsic controls of spatial and temporal variations in modern fluvial tufa sedimentation: A thirteen-year record from a semi-arid environment</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12045</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Intrinsic and extrinsic controls of spatial and temporal variations in modern fluvial tufa sedimentation: A thirteen-year record from a semi-arid environment</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Concha Arenas, Marta Vázquez-Urbez, Luis Auqué, Carlos Sancho, Cinta Osácar, Gonzalo Pardo</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-16T17:41:37.024369-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12045</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/">10.1111/sed.12045</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12045</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Themed Issue Paper</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>Sedimentological and hydrochemical parameters of the River Piedra (north-east Spain) were monitored every six months (from 1999 to 2012) at 24 sites, at which tablets were installed all along the river. The river water is of HCO<sub>3</sub>–SO<sub>4</sub>–Ca type and is notably influenced by inputs from upstream karstic springs. Tufa deposition was first detected 8 km downstream of these springs and greatly increased from there, primarily along the steeper stretch (i.e. within the Monasterio de Piedra Natural Park); then, deposition decreased through the most downstream stretch, with smaller ground water inputs. The spatial evolution of the tufa thickness (with parallel variations of PWP rates) was thus determined by the river water pCO<sub>2</sub> which was controlled by ground water inputs and by the riverbed slope. Five fluvial subenvironments and seven sedimentary facies were characterised. The water flow conditions are the primary factor responsible for the distinct deposition rates of facies, mainly through CO<sub>2</sub>-outgassing. Stromatolites and moss-tufa and alga-tufa had the highest rates, whereas loose tufa formed in slow-flowing water and tufa of spray areas had thinner deposition. A six-month pattern in the deposition rate was detected through thickness measurements. That pattern was parallel to the seasonal PWP rates. The increased deposition during warm periods (spring and summer; mean: 5.08 mm) compared with cool periods (autumn and winter; mean: 2.77 mm) is linked chiefly to temperature, which controlled the seasonal changes in the physico-chemical and biological processes; this finding is supported by a principal components analysis. Seasonal variations of insolation and day duration also contributed to such a deposition pattern. Large discharge events, which provoked erosion of tufa deposits and dilution of water, caused the reversal of the seasonal deposition rate pattern. Stromatolites are likely to preserve the most complete sedimentary record. Although tufas are a potentially sensitive record of climate-related parameters, erosion is an intrinsic process that may overwhelm the effects of such parameters. This issue should be considered in palaeoclimatic studies based on the tufa record, particularly in semi-arid conditions.</p></div>
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Sedimentological and hydrochemical parameters of the River Piedra (north-east Spain) were monitored every six months (from 1999 to 2012) at 24 sites, at which tablets were installed all along the river. The river water is of HCO3–SO4–Ca type and is notably influenced by inputs from upstream karstic springs. Tufa deposition was first detected 8 km downstream of these springs and greatly increased from there, primarily along the steeper stretch (i.e. within the Monasterio de Piedra Natural Park); then, deposition decreased through the most downstream stretch, with smaller ground water inputs. The spatial evolution of the tufa thickness (with parallel variations of PWP rates) was thus determined by the river water pCO2 which was controlled by ground water inputs and by the riverbed slope. Five fluvial subenvironments and seven sedimentary facies were characterised. The water flow conditions are the primary factor responsible for the distinct deposition rates of facies, mainly through CO2-outgassing. Stromatolites and moss-tufa and alga-tufa had the highest rates, whereas loose tufa formed in slow-flowing water and tufa of spray areas had thinner deposition. A six-month pattern in the deposition rate was detected through thickness measurements. That pattern was parallel to the seasonal PWP rates. The increased deposition during warm periods (spring and summer; mean: 5.08 mm) compared with cool periods (autumn and winter; mean: 2.77 mm) is linked chiefly to temperature, which controlled the seasonal changes in the physico-chemical and biological processes; this finding is supported by a principal components analysis. Seasonal variations of insolation and day duration also contributed to such a deposition pattern. Large discharge events, which provoked erosion of tufa deposits and dilution of water, caused the reversal of the seasonal deposition rate pattern. Stromatolites are likely to preserve the most complete sedimentary record. Although tufas are a potentially sensitive record of climate-related parameters, erosion is an intrinsic process that may overwhelm the effects of such parameters. This issue should be considered in palaeoclimatic studies based on the tufa record, particularly in semi-arid conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12041" xmlns="http://purl.org/rss/1.0/"><title>Stratal architecture and platform evolution of an early Frasnian syn-tectonic carbonate platform, Canning Basin, Australia</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12041</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Stratal architecture and platform evolution of an early Frasnian syn-tectonic carbonate platform, Canning Basin, Australia</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Nancy Chow, Annette D. George, Kate M. Trinajstic, Z.Q. Chen</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-02-12T06:24:44.024066-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12041</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/">10.1111/sed.12041</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12041</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Facies architecture and platform evolution of an early Frasnian reef complex in the northern Canning Basin of north-western Australia were strongly controlled by syn-depositional faulting during a phase of basin extension. The margin-attached Hull platform developed on a fault block of Precambrian basement with accommodation largely generated by movement along the Mount Elma Fault Zone. Recognition of major subaerial exposure and flooding surfaces in the Hull platform (from outcrop and drillcore) has enabled comparison of facies associations within a temporal framework and led to identification of three stages of platform evolution. Stage 1 records initial ramp development on the hangingwall dip slope with predominantly deep subtidal conditions that prevented any cyclic facies arrangements. This stage is characterised by basal siliciclastic deposits and a major deepening-upward facies pattern that is capped by a sequence boundary towards the footwall (north-west) and a major flooding surface towards the hangingwall. Stage 2 reflects the bulk of platform aggradation, significant platform growth towards the hangingwall and the development of reef margins and cyclic facies arrangements. Thickening of this stage towards the hangingwall indicates that accommodation was generated by rotation of the fault block and overlying platform. Stage 3 records a major flooding and backstep of the platform margin. The Hull platform illustrates important elements of margin-attached carbonate platforms in a half-graben setting, including: (i) prominent, but limited, coarse siliciclastic input that does not have a major detrimental effect on carbonate production near the rift margin in arid to semi-arid settings; (ii) wedge-shaped accommodation created by syn-depositional rotation of fault blocks and tilting of the hangingwall dip slope, resulting in shallow-water facies and subaerial exposure up-dip of the rotational axis and deeper water facies down-dip; and (iii) evolution of a ramp to rimmed shelf, coincident with a sequence boundary–flooding surface, that is accelerated by tilting of the hangingwall dip slope during fault-block rotation.</p></div>
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Facies architecture and platform evolution of an early Frasnian reef complex in the northern Canning Basin of north-western Australia were strongly controlled by syn-depositional faulting during a phase of basin extension. The margin-attached Hull platform developed on a fault block of Precambrian basement with accommodation largely generated by movement along the Mount Elma Fault Zone. Recognition of major subaerial exposure and flooding surfaces in the Hull platform (from outcrop and drillcore) has enabled comparison of facies associations within a temporal framework and led to identification of three stages of platform evolution. Stage 1 records initial ramp development on the hangingwall dip slope with predominantly deep subtidal conditions that prevented any cyclic facies arrangements. This stage is characterised by basal siliciclastic deposits and a major deepening-upward facies pattern that is capped by a sequence boundary towards the footwall (north-west) and a major flooding surface towards the hangingwall. Stage 2 reflects the bulk of platform aggradation, significant platform growth towards the hangingwall and the development of reef margins and cyclic facies arrangements. Thickening of this stage towards the hangingwall indicates that accommodation was generated by rotation of the fault block and overlying platform. Stage 3 records a major flooding and backstep of the platform margin. The Hull platform illustrates important elements of margin-attached carbonate platforms in a half-graben setting, including: (i) prominent, but limited, coarse siliciclastic input that does not have a major detrimental effect on carbonate production near the rift margin in arid to semi-arid settings; (ii) wedge-shaped accommodation created by syn-depositional rotation of fault blocks and tilting of the hangingwall dip slope, resulting in shallow-water facies and subaerial exposure up-dip of the rotational axis and deeper water facies down-dip; and (iii) evolution of a ramp to rimmed shelf, coincident with a sequence boundary–flooding surface, that is accelerated by tilting of the hangingwall dip slope during fault-block rotation.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12037" xmlns="http://purl.org/rss/1.0/"><title>Facies model of a fine-grained, tide-dominated delta: Lower Dir Abu Lifa Member (Eocene), Western Desert, Egypt</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12037</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Facies model of a fine-grained, tide-dominated delta: Lower Dir Abu Lifa Member (Eocene), Western Desert, Egypt</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Berit Legler, Howard D. Johnson, Gary J. Hampson, Benoit Y.G. Massart, Chris A-L. Jackson, Matthew D. Jackson, Ahmed El-Barkooky, Rodmar Ravnas</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-21T06:50:42.166018-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12037</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/">10.1111/sed.12037</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12037</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Existing facies models of tide-dominated deltas largely omit fine-grained, mud-rich successions. Sedimentary facies and sequence stratigraphic analysis of the exceptionally well-preserved Late Eocene Dir Abu Lifa Member (Western Desert, Egypt) aims to bridge this gap. The succession was deposited in a structurally controlled, shallow, macrotidal embayment and deposition was supplemented by fluvial processes but lacked wave influence. The succession contains two stacked, progradational parasequence sets bounded by regionally extensive flooding surfaces. Within this succession two main genetic elements are identified: non-channelized tidal bars and tidal channels. Non-channelized tidal bars comprise coarsening-upward sandbodies, including large, downcurrent-dipping accretion surfaces, sometimes capped by palaeosols indicating emergence. Tidal channels are preserved as single-storey and multilateral bodies filled by: (i) laterally migrating, elongate tidal bars (inclined heterolithic strata, 5 to 25 m thick); (ii) forward-facing lobate bars (sigmoidal heterolithic strata, up to 10 m thick); (iii) side bars displaying oblique to vertical accretion (4 to 7 m thick); or (iv) vertically-accreting mud (1 to 4 m thick). Palaeocurrent data show that channels were swept by bidirectional tidal currents and typically were mutually evasive. Along-strike variability defines a similar large-scale architecture in both parasequence sets: a deeply scoured channel belt characterized by widespread inclined heterolithic strata is eroded from the parasequence-set top, and flanked by stacked, non-channelized tidal bars and smaller channelized bodies. The tide-dominated delta is characterized by: (i) the regressive stratigraphic context; (ii) net-progradational stratigraphic architecture within the succession; (iii) the absence of upward deepening trends and tidal ravinement surfaces; and (iv) architectural relations that demonstrate contemporaneous tidal distributary channel infill and tidal bar accretion at the delta front. The detailed facies analysis of this fine-grained, tide-dominated deltaic succession expands the range of depositional models available for the evaluation of ancient tidal successions, which are currently biased towards transgressive, valley-confined estuarine and coarser grained deltaic depositional systems.</p></div>
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Existing facies models of tide-dominated deltas largely omit fine-grained, mud-rich successions. Sedimentary facies and sequence stratigraphic analysis of the exceptionally well-preserved Late Eocene Dir Abu Lifa Member (Western Desert, Egypt) aims to bridge this gap. The succession was deposited in a structurally controlled, shallow, macrotidal embayment and deposition was supplemented by fluvial processes but lacked wave influence. The succession contains two stacked, progradational parasequence sets bounded by regionally extensive flooding surfaces. Within this succession two main genetic elements are identified: non-channelized tidal bars and tidal channels. Non-channelized tidal bars comprise coarsening-upward sandbodies, including large, downcurrent-dipping accretion surfaces, sometimes capped by palaeosols indicating emergence. Tidal channels are preserved as single-storey and multilateral bodies filled by: (i) laterally migrating, elongate tidal bars (inclined heterolithic strata, 5 to 25 m thick); (ii) forward-facing lobate bars (sigmoidal heterolithic strata, up to 10 m thick); (iii) side bars displaying oblique to vertical accretion (4 to 7 m thick); or (iv) vertically-accreting mud (1 to 4 m thick). Palaeocurrent data show that channels were swept by bidirectional tidal currents and typically were mutually evasive. Along-strike variability defines a similar large-scale architecture in both parasequence sets: a deeply scoured channel belt characterized by widespread inclined heterolithic strata is eroded from the parasequence-set top, and flanked by stacked, non-channelized tidal bars and smaller channelized bodies. The tide-dominated delta is characterized by: (i) the regressive stratigraphic context; (ii) net-progradational stratigraphic architecture within the succession; (iii) the absence of upward deepening trends and tidal ravinement surfaces; and (iv) architectural relations that demonstrate contemporaneous tidal distributary channel infill and tidal bar accretion at the delta front. The detailed facies analysis of this fine-grained, tide-dominated deltaic succession expands the range of depositional models available for the evaluation of ancient tidal successions, which are currently biased towards transgressive, valley-confined estuarine and coarser grained deltaic depositional systems.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12035" xmlns="http://purl.org/rss/1.0/"><title>Variations in the architecture of hydraulic-jump bar complexes on non-eroding beds</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12035</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Variations in the architecture of hydraulic-jump bar complexes on non-eroding beds</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Robert G. Macdonald, Jan Alexander, John C. Bacon, Mark J. Cooker</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-14T05:55:50.415098-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12035</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/">10.1111/sed.12035</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12035</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Sediment accumulation downstream of hydraulic jumps can occur in many settings but the architectures of such deposits are poorly documented. Here, three flume runs were used to examine the influence of sediment grain size and transport rate on the characteristics of <em>hydraulic-jump unit bars</em>. In one of these runs six <em>hydraulic-jump unit bars</em> formed a <em>hydraulic-jump bar complex</em>. In another, the same sediment was supplied more quickly and only two unit bars formed. In the third run with the same sediment supply rate, but different grain size, only one large unit bar formed. All unit bars developed in a similar way but their size and internal architecture differed; they all resulted from a reduction in sediment transport capacity at the transition from supercritical flow to subcritical flow in the hydraulic jump. After initial onset of sedimentation and unit bar formation, generation of subsequent unit bars may be: (i) related to small changes in sediment flux; and (ii) independent of changes in the hydraulic jump. Continued sedimentation caused changes from oscillating to weak hydraulic jumps and <em>hydraulic-jump unit bars</em> formed in both circumstances. The flow of water and suspended sediment becomes shallower over the lee of the bar complex. This leads to flow acceleration and a return to supercritical flow conditions. In turn, a chain of such features can form and generate a chute and pool bed morphology. There is an inherent upper size limit to a <em>hydraulic-jump bar complex</em> due to the changing flow conditions over the growing deposit as the water above it becomes shallower. There is also an amplitude minimum for the development of foresets and subsequent unit bar growth. <em>Hydraulic-jump unit bars</em> have architectures that should be recognizable in the rock record and because their size is constrained by the flow conditions, their identification should be useful for interpreting palaeoenvironment.</p></div>
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Sediment accumulation downstream of hydraulic jumps can occur in many settings but the architectures of such deposits are poorly documented. Here, three flume runs were used to examine the influence of sediment grain size and transport rate on the characteristics of hydraulic-jump unit bars. In one of these runs six hydraulic-jump unit bars formed a hydraulic-jump bar complex. In another, the same sediment was supplied more quickly and only two unit bars formed. In the third run with the same sediment supply rate, but different grain size, only one large unit bar formed. All unit bars developed in a similar way but their size and internal architecture differed; they all resulted from a reduction in sediment transport capacity at the transition from supercritical flow to subcritical flow in the hydraulic jump. After initial onset of sedimentation and unit bar formation, generation of subsequent unit bars may be: (i) related to small changes in sediment flux; and (ii) independent of changes in the hydraulic jump. Continued sedimentation caused changes from oscillating to weak hydraulic jumps and hydraulic-jump unit bars formed in both circumstances. The flow of water and suspended sediment becomes shallower over the lee of the bar complex. This leads to flow acceleration and a return to supercritical flow conditions. In turn, a chain of such features can form and generate a chute and pool bed morphology. There is an inherent upper size limit to a hydraulic-jump bar complex due to the changing flow conditions over the growing deposit as the water above it becomes shallower. There is also an amplitude minimum for the development of foresets and subsequent unit bar growth. Hydraulic-jump unit bars have architectures that should be recognizable in the rock record and because their size is constrained by the flow conditions, their identification should be useful for interpreting palaeoenvironment.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12028" xmlns="http://purl.org/rss/1.0/"><title>Environmental controls on the Late Holocene carbonate sedimentation of a karstic lake in the Middle-Atlas Mountains (Lake Afourgagh, Morocco)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12028</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Environmental controls on the Late Holocene carbonate sedimentation of a karstic lake in the Middle-Atlas Mountains (Lake Afourgagh, Morocco)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sébastien Détriché, Jean-Gabriel Bréhéret, L'houcine Karrat, Florent Hinschberger, Jean-Jacques Macaire</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-09T05:19:51.637404-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12028</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/">10.1111/sed.12028</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12028</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 Lake Afourgagh sediment record and facies successions provide an outstanding example of environmentally controlled carbonate sedimentation. Afourgagh is a small, shallow permanent lake located in the Middle-Atlas Mountains in Morocco in a karstic context. It is fed by ground waters that are relatively enriched in Mg resulting from the leaching of the Jurassic dolomitic bedrock of the catchment. This eutrophic lake is episodically restricted and characterized by alkaline waters with a fluctuating high Mg/Ca ratio. The maximum extension of the Holocene shoreline coincides with evidence of a lake stabilization level corresponding to the outflow of the lake through a wadi. Lakeshore terrace sediments deposited on an alluvial fan siltstone during the past <em>ca</em> 2500 cal yr <span class="smallCaps">bp</span> comprise four main facies: a littoral crust, palaeosols, palustrine silts and charophyte tufas, which reflect different environments from the shoreline toward the deeper water. In the more distal parts, the charophyte tufas display a well-expressed lamination punctuated by the development of microstromatolites on algae thalli. The mineralogical composition of the carbonates is linked to the facies. While the charophyte tufas are characterized by a relatively high content in aragonite, in addition to low-Mg calcite, the littoral crust is mainly composed of magnesite. This pattern is related to the evolving chemistry of water due to the influence of charophyte proliferation during dry summers. Calcium-carbonate precipitation on algae thalli (both bioinduced and microbially mediated) progressively induces an increase in the Mg/Ca ratio of the lake water, while the capillary evaporation of shallow ground waters causes precipitation of a magnesite precursor on the shoreline, producing magnesite during early diagenesis. This effect is characteristic of two episodes: part of the Roman Warm Period and the beginning of the Dark Age Cold Period. The carbonate mineralogy of the different depositional sequences at Afourgagh indicates lake-level and water-chemistry fluctuations under a climatic influence. Therefore, among other regional records, the Lake Afourgagh sedimentary record provides useful evidence for reconstructing these environmental changes.</p></div>
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The Lake Afourgagh sediment record and facies successions provide an outstanding example of environmentally controlled carbonate sedimentation. Afourgagh is a small, shallow permanent lake located in the Middle-Atlas Mountains in Morocco in a karstic context. It is fed by ground waters that are relatively enriched in Mg resulting from the leaching of the Jurassic dolomitic bedrock of the catchment. This eutrophic lake is episodically restricted and characterized by alkaline waters with a fluctuating high Mg/Ca ratio. The maximum extension of the Holocene shoreline coincides with evidence of a lake stabilization level corresponding to the outflow of the lake through a wadi. Lakeshore terrace sediments deposited on an alluvial fan siltstone during the past ca 2500 cal yr bp comprise four main facies: a littoral crust, palaeosols, palustrine silts and charophyte tufas, which reflect different environments from the shoreline toward the deeper water. In the more distal parts, the charophyte tufas display a well-expressed lamination punctuated by the development of microstromatolites on algae thalli. The mineralogical composition of the carbonates is linked to the facies. While the charophyte tufas are characterized by a relatively high content in aragonite, in addition to low-Mg calcite, the littoral crust is mainly composed of magnesite. This pattern is related to the evolving chemistry of water due to the influence of charophyte proliferation during dry summers. Calcium-carbonate precipitation on algae thalli (both bioinduced and microbially mediated) progressively induces an increase in the Mg/Ca ratio of the lake water, while the capillary evaporation of shallow ground waters causes precipitation of a magnesite precursor on the shoreline, producing magnesite during early diagenesis. This effect is characteristic of two episodes: part of the Roman Warm Period and the beginning of the Dark Age Cold Period. The carbonate mineralogy of the different depositional sequences at Afourgagh indicates lake-level and water-chemistry fluctuations under a climatic influence. Therefore, among other regional records, the Lake Afourgagh sedimentary record provides useful evidence for reconstructing these environmental changes.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12036" xmlns="http://purl.org/rss/1.0/"><title>Microfacies and diagenesis of older Pleistocene (pre-last glacial maximum) reef deposits, Great Barrier Reef, Australia (IODP Expedition 325): A quantitative approach</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12036</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Microfacies and diagenesis of older Pleistocene (pre-last glacial maximum) reef deposits, Great Barrier Reef, Australia (IODP Expedition 325): A quantitative approach</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Eberhard Gischler, Alex L. Thomas, André W. Droxler, Jody M. Webster, Yusuke Yokoyama, Bernd R. Schöne</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-08T04:16:58.748713-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12036</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/">10.1111/sed.12036</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12036</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>During Integrated Ocean Drilling Program Expedition 325, 34 holes were drilled along five transects in front of the Great Barrier Reef of Australia, penetrating some 700 m of late Pleistocene reef deposits (post-glacial; largely 20 to 10 kyr <span class="smallCaps">bp</span>) in water depths of 42 to 127 m. In seven holes, drilled in water depths of 42 to 92 m on three transects, older Pleistocene (older than last glacial maximum, &gt;20 kyr <span class="smallCaps">bp</span>) reef deposits were recovered from lower core sections. In this study, facies, diagenetic features, mineralogy and stable isotope geochemistry of 100 samples from six of the latter holes were investigated and quantified. Lithologies are dominated by grain-supported textures, and were to a large part deposited in high-energy, reef or reef slope environments. Quantitative analyses allow 11 microfacies to be defined, including mixed skeletal packstone and grainstone, mudstone-wackestone, coral packstone, coral grainstone, coralline algal grainstone, coral-algal packstone, coralline algal packstone, <em>Halimeda</em> grainstone, microbialite and caliche. Microbialites, that are common in cavities of younger, post-glacial deposits, are rare in pre-last glacial maximum core sections, possibly due to a lack of open framework suitable for colonization by microbes. In pre-last glacial maximum deposits of holes M0032A and M0033A (&gt;20 kyr <span class="smallCaps">bp</span>), marine diagenetic features are dominant; samples consist largely of aragonite and high-magnesium calcite. Holes M0042A and M0057A, which contain the oldest rocks (&gt;169 kyr <span class="smallCaps">bp</span>), are characterized by meteoric diagenesis and samples mostly consist of low-magnesium calcite. Holes M0042A, M0055A and M0056A (&gt;30 kyr <span class="smallCaps">bp</span>), and a horizon in the upper part of hole M0057A, contain both marine and meteoric diagenetic features. However, only one change from marine to meteoric pore water is recorded in contrast with the changes in diagenetic environment that might be inferred from the sea-level history. Values of stable isotopes of oxygen and carbon are consistent with these findings. Samples from holes M0032A and M0033A reflect largely positive values (δ<sup>18</sup>O: −1 to +1‰ and δ<sup>13</sup>C: +1 to +4‰), whereas those from holes M0042A and M0057A are negative (δ<sup>18</sup>O: −4 to +2‰ and δ<sup>13</sup>C: −8 to +2‰). Holes M0055A and M0056A provide intermediate values, with slightly positive δ<sup>13</sup>C, and negative δ<sup>18</sup>O values. The type and intensity of meteroric diagenesis appears to have been controlled both by age and depth, i.e. the time available for diagenetic alteration, and reflects the relation between reef deposition and sea-level change.</p></div>
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During Integrated Ocean Drilling Program Expedition 325, 34 holes were drilled along five transects in front of the Great Barrier Reef of Australia, penetrating some 700 m of late Pleistocene reef deposits (post-glacial; largely 20 to 10 kyr bp) in water depths of 42 to 127 m. In seven holes, drilled in water depths of 42 to 92 m on three transects, older Pleistocene (older than last glacial maximum, &gt;20 kyr bp) reef deposits were recovered from lower core sections. In this study, facies, diagenetic features, mineralogy and stable isotope geochemistry of 100 samples from six of the latter holes were investigated and quantified. Lithologies are dominated by grain-supported textures, and were to a large part deposited in high-energy, reef or reef slope environments. Quantitative analyses allow 11 microfacies to be defined, including mixed skeletal packstone and grainstone, mudstone-wackestone, coral packstone, coral grainstone, coralline algal grainstone, coral-algal packstone, coralline algal packstone, Halimeda grainstone, microbialite and caliche. Microbialites, that are common in cavities of younger, post-glacial deposits, are rare in pre-last glacial maximum core sections, possibly due to a lack of open framework suitable for colonization by microbes. In pre-last glacial maximum deposits of holes M0032A and M0033A (&gt;20 kyr bp), marine diagenetic features are dominant; samples consist largely of aragonite and high-magnesium calcite. Holes M0042A and M0057A, which contain the oldest rocks (&gt;169 kyr bp), are characterized by meteoric diagenesis and samples mostly consist of low-magnesium calcite. Holes M0042A, M0055A and M0056A (&gt;30 kyr bp), and a horizon in the upper part of hole M0057A, contain both marine and meteoric diagenetic features. However, only one change from marine to meteoric pore water is recorded in contrast with the changes in diagenetic environment that might be inferred from the sea-level history. Values of stable isotopes of oxygen and carbon are consistent with these findings. Samples from holes M0032A and M0033A reflect largely positive values (δ18O: −1 to +1‰ and δ13C: +1 to +4‰), whereas those from holes M0042A and M0057A are negative (δ18O: −4 to +2‰ and δ13C: −8 to +2‰). Holes M0055A and M0056A provide intermediate values, with slightly positive δ13C, and negative δ18O values. The type and intensity of meteroric diagenesis appears to have been controlled both by age and depth, i.e. the time available for diagenetic alteration, and reflects the relation between reef deposition and sea-level change.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12040" xmlns="http://purl.org/rss/1.0/"><title>Influence of sieving time on the efficiency and accuracy of grain-size analysis of beach and dune sands</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12040</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Influence of sieving time on the efficiency and accuracy of grain-size analysis of beach and dune sands</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Jorge Román-Sierra, Juan j. Muñoz-perez, Marina Navarro-Pons</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-05-08T04:15:29.203849-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12040</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/">10.1111/sed.12040</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12040</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Grain size is a fundamental property of sediments and is commonly used to describe sedimentary facies and classify sedimentary environments. Among the various conventional techniques utilized to determine grain-size frequency distributions, sieving is the most widely applied procedure. The accuracy of such analyses is, among other factors, strongly dependent on the sieving time. However, despite a substantial amount of research in this field, optimal sieving times for different types of sediments have, to date, not been established. In this article, the influence of sieving time on grain-size analyses of medium-grained microtidal and mesotidal beach and dune sands has been determined. To assess the precision of important textural parameters, such as median grain size, sorting, skewness and kurtosis, an error analysis was carried out for different sieving times (2, 5, 10, 15 and 20 minutes). After calibrating the analytical and sampling methodologies, significant deviations were registered when sieving time was less than 10 minutes. However, such deviations were very small and grain-size distributions remained almost identical for sieving times of 10 minutes and longer, relative errors being as low as 0% in some cases.</p></div>
]]></content:encoded><description>

Grain size is a fundamental property of sediments and is commonly used to describe sedimentary facies and classify sedimentary environments. Among the various conventional techniques utilized to determine grain-size frequency distributions, sieving is the most widely applied procedure. The accuracy of such analyses is, among other factors, strongly dependent on the sieving time. However, despite a substantial amount of research in this field, optimal sieving times for different types of sediments have, to date, not been established. In this article, the influence of sieving time on grain-size analyses of medium-grained microtidal and mesotidal beach and dune sands has been determined. To assess the precision of important textural parameters, such as median grain size, sorting, skewness and kurtosis, an error analysis was carried out for different sieving times (2, 5, 10, 15 and 20 minutes). After calibrating the analytical and sampling methodologies, significant deviations were registered when sieving time was less than 10 minutes. However, such deviations were very small and grain-size distributions remained almost identical for sieving times of 10 minutes and longer, relative errors being as low as 0% in some cases.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12042" xmlns="http://purl.org/rss/1.0/"><title>The morphology and function of thrombolitic calcite precipitating biofilms: A universal model derived from freshwater mesocosm experiments</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12042</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">The morphology and function of thrombolitic calcite precipitating biofilms: A universal model derived from freshwater mesocosm experiments</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Martyn Pedley</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-29T07:08:59.372812-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12042</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/">10.1111/sed.12042</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12042</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Processes and products in freshwater carbonates</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>Microbialites with laminar (stromatolite) and thrombolitic (thrombolite) fabrics are ubiquitous within the Cenozoic freshwater sedimentary record. However, the biology and physiology of the living prokaryote–microphyte biofilms which produced them is only now becoming understood. The present contribution describes a flowing water experimental mesocosm study spanning over 2·5 years and run under near-natural conditions. This work focussed on microbial biofilm precipitation mechanisms which produce thrombolitic carbonate micro-fabrics capable of preservation in the geological record. In particular, the roles of microbial guilds and carbonate precipitation processes were examined and recorded at all stages of thrombolite development. The mesocosm experiments convincingly demonstrated that the biofilm community actively encouraged calcium ion precipitation derived from flowing waters. This precipitation took the form of amorphous calcium carbonate nanosphere clusters. These clusters were not randomly distributed within the biofilm extracellular polymeric substances but were focussed in the close vicinity of living filament and coccoid bacterial clusters within individual living biofilm layers. Significantly, the precipitates never replaced microbial cell walls and never buried the living microbes. During nanosphere precipitation extracellular polymeric substances were progressively occluded from between the developing nanosphere clusters. However, extracellular polymeric substances were never totally removed from within the amorphous calcium carbonate clusters until they had neomorphosed into microspar crystals. The orientation of precipitating microspar crystals within the biofilm appeared to be controlled by the host extracellular polymeric substance fabric (cf. typical crystal growth from solid substrates). Precipitates were organized around the margins of a cancellate microfabric developed by a range of microbial guilds within each biofilm layer. This produced a distinct thrombolitic fabric within the biofilm which was quite distinct from laminar stromatolite fabrics. It is concluded that the mesocosm grown freshwater biofilms and their associated microbialite calcite micro-fabrics present a universally applicable model. Importantly, they provide a mechanism for thrombolite micro-fabric developments throughout the geological record.</p></div>
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Microbialites with laminar (stromatolite) and thrombolitic (thrombolite) fabrics are ubiquitous within the Cenozoic freshwater sedimentary record. However, the biology and physiology of the living prokaryote–microphyte biofilms which produced them is only now becoming understood. The present contribution describes a flowing water experimental mesocosm study spanning over 2·5 years and run under near-natural conditions. This work focussed on microbial biofilm precipitation mechanisms which produce thrombolitic carbonate micro-fabrics capable of preservation in the geological record. In particular, the roles of microbial guilds and carbonate precipitation processes were examined and recorded at all stages of thrombolite development. The mesocosm experiments convincingly demonstrated that the biofilm community actively encouraged calcium ion precipitation derived from flowing waters. This precipitation took the form of amorphous calcium carbonate nanosphere clusters. These clusters were not randomly distributed within the biofilm extracellular polymeric substances but were focussed in the close vicinity of living filament and coccoid bacterial clusters within individual living biofilm layers. Significantly, the precipitates never replaced microbial cell walls and never buried the living microbes. During nanosphere precipitation extracellular polymeric substances were progressively occluded from between the developing nanosphere clusters. However, extracellular polymeric substances were never totally removed from within the amorphous calcium carbonate clusters until they had neomorphosed into microspar crystals. The orientation of precipitating microspar crystals within the biofilm appeared to be controlled by the host extracellular polymeric substance fabric (cf. typical crystal growth from solid substrates). Precipitates were organized around the margins of a cancellate microfabric developed by a range of microbial guilds within each biofilm layer. This produced a distinct thrombolitic fabric within the biofilm which was quite distinct from laminar stromatolite fabrics. It is concluded that the mesocosm grown freshwater biofilms and their associated microbialite calcite micro-fabrics present a universally applicable model. Importantly, they provide a mechanism for thrombolite micro-fabric developments throughout the geological record.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12043" xmlns="http://purl.org/rss/1.0/"><title>Signatures of biologically influenced CaCo3 and Mg–Fe silicate precipitation in hot springs: Case study from the Ruidian geothermal area, western Yunnan Province, China</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12043</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Signatures of biologically influenced CaCo3 and Mg–Fe silicate precipitation in hot springs: Case study from the Ruidian geothermal area, western Yunnan Province, China</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Brian Jones, Xiaotong Peng</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-25T04:11:23.437302-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12043</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/">10.1111/sed.12043</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12043</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Processes and Products in Freshwater Carbonates</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>Hot springs at Gongxiaoshe and Zhuyuan (maximum temperatures of 73 to 84°C, respectively) are characterized by deposits formed of calcite, aragonite, non-crystalline Si–Mg–Fe deposits, and minor amounts of barite and gypsum. The deposits at Gongxiaoshe are formed largely of alternating calcite and aragonite laminae, whereas those at Zhuyuan are formed largely of calcite. The calcite is in the form of: (i) pseudodendrites that grew as sub-crystals stacked upon each other; and (ii) unattached euhedral and incompletely formed dodecahedral and rhombohedral crystals. Amorphous CaCO<sub>3</sub>, formed of nanoparticles &lt;1 μm long, is common in some of the Zhuyuan deposits, but minor in the Gongxiaoshe deposits. The morphologically diverse arrays of aragonite crystals that lie parallel to bedding were not nucleated on a growth surface. Many substrates in these deposits are covered with reticulate coatings that are formed largely of Si and Mg with minor Fe and micro-granular coatings that are formed largely of Si and Fe. Biofilms, with their extracellular polymeric substances, and microbes are common at both springs. The compositionally and crystallographically diverse precipitates at these two springs are attributed to a biologically influenced model with precipitation taking place in micro-domains that developed in the extracellular polymeric substances. According to this model, precipitation varied at the micron-scale influenced by the elemental concentrations that developed in the hydrogel of extracellular polymeric substances. Critically, the very low preservation potential of the extracellular polymeric substance and its formative microbes means that the precipitates will rapidly lose evidence of their biotic origin. The compositional diversity of the precipitates, the crystallographic diversity of the calcite and aragonite with numerous incompletely formed crystals, and local concentrations of Si, Mg and Fe may, however, serve as proxies of that biologically influenced precipitation.</p></div>
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Hot springs at Gongxiaoshe and Zhuyuan (maximum temperatures of 73 to 84°C, respectively) are characterized by deposits formed of calcite, aragonite, non-crystalline Si–Mg–Fe deposits, and minor amounts of barite and gypsum. The deposits at Gongxiaoshe are formed largely of alternating calcite and aragonite laminae, whereas those at Zhuyuan are formed largely of calcite. The calcite is in the form of: (i) pseudodendrites that grew as sub-crystals stacked upon each other; and (ii) unattached euhedral and incompletely formed dodecahedral and rhombohedral crystals. Amorphous CaCO3, formed of nanoparticles &lt;1 μm long, is common in some of the Zhuyuan deposits, but minor in the Gongxiaoshe deposits. The morphologically diverse arrays of aragonite crystals that lie parallel to bedding were not nucleated on a growth surface. Many substrates in these deposits are covered with reticulate coatings that are formed largely of Si and Mg with minor Fe and micro-granular coatings that are formed largely of Si and Fe. Biofilms, with their extracellular polymeric substances, and microbes are common at both springs. The compositionally and crystallographically diverse precipitates at these two springs are attributed to a biologically influenced model with precipitation taking place in micro-domains that developed in the extracellular polymeric substances. According to this model, precipitation varied at the micron-scale influenced by the elemental concentrations that developed in the hydrogel of extracellular polymeric substances. Critically, the very low preservation potential of the extracellular polymeric substance and its formative microbes means that the precipitates will rapidly lose evidence of their biotic origin. The compositional diversity of the precipitates, the crystallographic diversity of the calcite and aragonite with numerous incompletely formed crystals, and local concentrations of Si, Mg and Fe may, however, serve as proxies of that biologically influenced precipitation.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12029" xmlns="http://purl.org/rss/1.0/"><title>Colluvial sedimentation in a hyperarid setting (Atacama Desert, northern Chile): Geomorphic controls and stratigraphic facies variability</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12029</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Colluvial sedimentation in a hyperarid setting (Atacama Desert, northern Chile): Geomorphic controls and stratigraphic facies variability</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Dario Ventra, Guillermo Chong Dìaz, Poppe l. boer</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-22T12:56:15.782612-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12029</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/">10.1111/sed.12029</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12029</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original Manuscript</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>Research on colluvial depositional systems has recently emphasized periglacial and high-altitude settings, and the relations between Quaternary slope stratigraphy and climate change. This article examines the role of variable slope morphology, surface hydrology and microclimate in controlling colluvial sedimentation along a coastal tract of the hyperarid Atacama Desert in northern Chile. Direct accessibility of active surfaces is accompanied by uninterrupted stratigraphic exposures along the base of slopes, allowing direct comparisons between surface processes and the resulting sedimentary record. Four slope sectors are identified, based on differences in morphology and processes over active surfaces. Colluvial sedimentation is controlled by complex interactions of slope gradients and profiles, exposure to dominant winds, and potential runoff pathways, which vary considerably between different sectors. Major differences are evident between these hyperarid deposits and slope sedimentation in periglacial and temperate settings, including the complete absence of pedogenic activity and clay minerals; the volume of aeolian deposits and their role in controlling processes which redistribute sediment downslope, extending colluvial aprons; and the occurrence of runoff processes only where favoured by particular topographic configurations. Depositional surfaces range from steep talus cones, to debris-flow-dominated and aeolian-dominated colluvial aprons, to an aeolian ramp subject to reworking by mass flows and flash floods. Consequently, facies associations and architectures at outcrop are highly variable and highlight the importance of spatial variations in slope morphology and processes in producing distinct, coeval colluvial stratigraphies within a single environmental context. Discrepancies between active processes and the corresponding stratigraphic signatures are also evident in some sectors; for example, preservation of alluvial and aeolian facies in stratigraphic sections does not always reflect the dominant processes over active slopes. Together with the spatial variability in processes and deposits along these slopes, this suggests that caution is required when extracting palaeoenvironmental information from analyses of colluvial successions.</p></div>
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Research on colluvial depositional systems has recently emphasized periglacial and high-altitude settings, and the relations between Quaternary slope stratigraphy and climate change. This article examines the role of variable slope morphology, surface hydrology and microclimate in controlling colluvial sedimentation along a coastal tract of the hyperarid Atacama Desert in northern Chile. Direct accessibility of active surfaces is accompanied by uninterrupted stratigraphic exposures along the base of slopes, allowing direct comparisons between surface processes and the resulting sedimentary record. Four slope sectors are identified, based on differences in morphology and processes over active surfaces. Colluvial sedimentation is controlled by complex interactions of slope gradients and profiles, exposure to dominant winds, and potential runoff pathways, which vary considerably between different sectors. Major differences are evident between these hyperarid deposits and slope sedimentation in periglacial and temperate settings, including the complete absence of pedogenic activity and clay minerals; the volume of aeolian deposits and their role in controlling processes which redistribute sediment downslope, extending colluvial aprons; and the occurrence of runoff processes only where favoured by particular topographic configurations. Depositional surfaces range from steep talus cones, to debris-flow-dominated and aeolian-dominated colluvial aprons, to an aeolian ramp subject to reworking by mass flows and flash floods. Consequently, facies associations and architectures at outcrop are highly variable and highlight the importance of spatial variations in slope morphology and processes in producing distinct, coeval colluvial stratigraphies within a single environmental context. Discrepancies between active processes and the corresponding stratigraphic signatures are also evident in some sectors; for example, preservation of alluvial and aeolian facies in stratigraphic sections does not always reflect the dominant processes over active slopes. Together with the spatial variability in processes and deposits along these slopes, this suggests that caution is required when extracting palaeoenvironmental information from analyses of colluvial successions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12030" xmlns="http://purl.org/rss/1.0/"><title>Impact of environmental parameters on coral reef development and drowning: Forward modelling of the last deglacial reefs from Tahiti (French Polynesia; IODP Expedition #310)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12030</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Impact of environmental parameters on coral reef development and drowning: Forward modelling of the last deglacial reefs from Tahiti (French Polynesia; IODP Expedition #310)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Claire Seard, Jean Borgomano, Didier Granjeon, Gilbert Camoin</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-20T02:01:36.905024-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12030</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/">10.1111/sed.12030</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12030</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 sedimentological and chronological analysis of the last deglacial reef sequences of Tahiti (French Polynesia), drilled during the Integrated Ocean Drilling Program Expedition 310, provide a high-resolution data set allowing a well-constrained forward modelling study. This study represents the first attempt to model in three dimensions the coral reef development of Tahiti during the last deglacial sea-level rise (23 000 to 6000 cal yr <span class="smallCaps">bp</span>) using the software <span class="smallCaps">dionisos</span> developed by IFP Energies nouvelles. It allows the testing of the reconstructed last deglacial sea-level curve and the different environmental parameters (for example, wave energy and sediment fluxes) that could have influenced the reef development. These last deglacial reef sequences form two prominent ridges occurring seaward of the living barrier reef that consist of successive submerged reefs. These reefs have been prone to drowning because the window of maximum carbonate production rate is inhibited by high water turbidity (sediment supply from a nearby river), shallow depth of wave action and substrate availability. These factors, combined with rapid sea-level rise, have driven the growth of retrograding reef pinnacles. Local factors (substratum nature, sediment supply and wave energy) were the main processes that induced the drowning of the inner ridge, whereas interplay of local and global factors (acceleration of the sea-level rise) was responsible for the drowning of the outer ridge. This particular acceleration of sea-level rise of 16 m between 14·6 ka and 14 ka <span class="smallCaps">bp</span> corresponds to meltwater pulse 1A.</p></div>
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The sedimentological and chronological analysis of the last deglacial reef sequences of Tahiti (French Polynesia), drilled during the Integrated Ocean Drilling Program Expedition 310, provide a high-resolution data set allowing a well-constrained forward modelling study. This study represents the first attempt to model in three dimensions the coral reef development of Tahiti during the last deglacial sea-level rise (23 000 to 6000 cal yr bp) using the software dionisos developed by IFP Energies nouvelles. It allows the testing of the reconstructed last deglacial sea-level curve and the different environmental parameters (for example, wave energy and sediment fluxes) that could have influenced the reef development. These last deglacial reef sequences form two prominent ridges occurring seaward of the living barrier reef that consist of successive submerged reefs. These reefs have been prone to drowning because the window of maximum carbonate production rate is inhibited by high water turbidity (sediment supply from a nearby river), shallow depth of wave action and substrate availability. These factors, combined with rapid sea-level rise, have driven the growth of retrograding reef pinnacles. Local factors (substratum nature, sediment supply and wave energy) were the main processes that induced the drowning of the inner ridge, whereas interplay of local and global factors (acceleration of the sea-level rise) was responsible for the drowning of the outer ridge. This particular acceleration of sea-level rise of 16 m between 14·6 ka and 14 ka bp corresponds to meltwater pulse 1A.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12039" xmlns="http://purl.org/rss/1.0/"><title>Precession-scale cyclicity in the fluvial lower Eocene Willwood Formation of the Bighorn Basin, Wyoming (USA)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12039</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Precession-scale cyclicity in the fluvial lower Eocene Willwood Formation of the Bighorn Basin, Wyoming (USA)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Hemmo A. Abels, Mary J. Kraus, Philip D. Gingerich</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-19T11:31:29.986834-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12039</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/">10.1111/sed.12039</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12039</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Little is known about controls on river avulsion at geological time scales longer than 10<sup>4</sup> years, primarily because it is difficult to link observed changes in alluvial architecture to well-defined allogenic mechanisms and to disentangle allogenic from autogenic processes. Recognition of Milankovitch-sale orbital forcing in alluvial stratigraphy would provide unprecedented age control in terrestrial deposits, and also exploit models of allogenic forcing enabling more rigorous testing of allocyclic and autocyclic controls. The Willwood Formation of the Bighorn Basin is a lower Eocene fluvial unit distinctive for its thick sequence of laterally extensive lithological cycles on a scale of 4 to 10 m. Intervals of red palaeosols that formed on overbank mudstones are related to periods of relative channel stability when gradients between channel belts and floodplains were low. The intervening drab, heterolithic intervals with weak palaeosol development are attributed to episodes of channel avulsion that occurred when channels became super-elevated above the floodplain. In the Deer Creek Amphitheater section in the McCullough Peaks area, these overbank and avulsion deposits alternate with a dominant cycle thickness of <em>ca</em> 7·1 m. Using integrated stratigraphic age constraints, this cyclicity has an estimated period of <em>ca</em> 21·6 kyr, which is in the range of the period of precession climate cycles in the early Eocene. Previous analyses of three older and younger sections in the Bighorn Basin showed a similar 7 to 8 m spacing of red palaeosol clusters with an estimated duration close to the precession period. Intervals of floodplain stability alternating with episodes of large-scale reorganization of the fluvial system could be entirely autogenic; however, the remarkable regularity and the match in time scales documented here indicate that these alternations were probably paced by allogenic, astronomically forced climate change.</p></div>
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Little is known about controls on river avulsion at geological time scales longer than 104 years, primarily because it is difficult to link observed changes in alluvial architecture to well-defined allogenic mechanisms and to disentangle allogenic from autogenic processes. Recognition of Milankovitch-sale orbital forcing in alluvial stratigraphy would provide unprecedented age control in terrestrial deposits, and also exploit models of allogenic forcing enabling more rigorous testing of allocyclic and autocyclic controls. The Willwood Formation of the Bighorn Basin is a lower Eocene fluvial unit distinctive for its thick sequence of laterally extensive lithological cycles on a scale of 4 to 10 m. Intervals of red palaeosols that formed on overbank mudstones are related to periods of relative channel stability when gradients between channel belts and floodplains were low. The intervening drab, heterolithic intervals with weak palaeosol development are attributed to episodes of channel avulsion that occurred when channels became super-elevated above the floodplain. In the Deer Creek Amphitheater section in the McCullough Peaks area, these overbank and avulsion deposits alternate with a dominant cycle thickness of ca 7·1 m. Using integrated stratigraphic age constraints, this cyclicity has an estimated period of ca 21·6 kyr, which is in the range of the period of precession climate cycles in the early Eocene. Previous analyses of three older and younger sections in the Bighorn Basin showed a similar 7 to 8 m spacing of red palaeosol clusters with an estimated duration close to the precession period. Intervals of floodplain stability alternating with episodes of large-scale reorganization of the fluvial system could be entirely autogenic; however, the remarkable regularity and the match in time scales documented here indicate that these alternations were probably paced by allogenic, astronomically forced climate change.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12032" xmlns="http://purl.org/rss/1.0/"><title>Secular changes in colony-forms and bryozoan carbonate sediments through geological history</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12032</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Secular changes in colony-forms and bryozoan carbonate sediments through geological history</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Paul D. Taylor, Noel P. James</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-19T10:00:19.447788-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12032</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/">10.1111/sed.12032</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12032</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Ever since their first radiation in the Ordovician, bryozoans have contributed significantly to carbonate sedimentation. Most of the numerous colony-forms developed by bryozoans have evolved repeatedly in different taxonomic groups and vary in their sediment-producing potential. There are nine basic bryozoan colony-forms: encrusting, dome-shaped, palmate, foliose, fenestrate, robust branching, delicate branching, articulated and free-living. The proportion of these morphotypes in bryozoan faunas period by period is shown to change significantly through the Phanerozoic. Notable patterns include: (i) steady increase in the number and proportion of encrusting species through time, interrupted by a transient drop in the Late Palaeozoic; (ii) post-Triassic decrease in robust branching colonies; (iii) rise in the proportion of fenestrate colonies through the Palaeozoic, followed by their absence in the Triassic and Jurassic, rarity in the Cretaceous and reappearance in smaller proportions in the Cenozoic; and (iv) scarcity of articulated colonies and absence of free-living colonies until the Cretaceous. Most Palaeozoic bryozoan sediments come from two architecturally distinct groups of colonies: (i) domal, delicate branching, robust branching and palmate; and (ii) fenestrate. The former generate coarse particles both as sediment and components of stromatoporoid-coral reefs in the Early and mid Palaeozoic, whereas the delicate lacy fans of the latter create both prolific coarse sediment and form the cores of Late Palaeozoic deep-water, sub-photic biogenic mounds. Nearly all post-Palaeozoic bryozoan sediments comprise cyclostomes and cheilostomes with many of the same growth forms but with the addition of free-living colonies and significant numbers of articulated colonies. The latter produced sand and mud-sized bryozoan sediment via disarticulation for the first time. In contrast to the Palaeozoic, post-Palaeozoic bryozoans generated sediment varying more widely across the grain-size spectrum, from mud to sand to gravel. This article highlights the need to consider evolutionary changes in carbonate-producing organisms when interpreting facies changes through time.</p></div>
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Ever since their first radiation in the Ordovician, bryozoans have contributed significantly to carbonate sedimentation. Most of the numerous colony-forms developed by bryozoans have evolved repeatedly in different taxonomic groups and vary in their sediment-producing potential. There are nine basic bryozoan colony-forms: encrusting, dome-shaped, palmate, foliose, fenestrate, robust branching, delicate branching, articulated and free-living. The proportion of these morphotypes in bryozoan faunas period by period is shown to change significantly through the Phanerozoic. Notable patterns include: (i) steady increase in the number and proportion of encrusting species through time, interrupted by a transient drop in the Late Palaeozoic; (ii) post-Triassic decrease in robust branching colonies; (iii) rise in the proportion of fenestrate colonies through the Palaeozoic, followed by their absence in the Triassic and Jurassic, rarity in the Cretaceous and reappearance in smaller proportions in the Cenozoic; and (iv) scarcity of articulated colonies and absence of free-living colonies until the Cretaceous. Most Palaeozoic bryozoan sediments come from two architecturally distinct groups of colonies: (i) domal, delicate branching, robust branching and palmate; and (ii) fenestrate. The former generate coarse particles both as sediment and components of stromatoporoid-coral reefs in the Early and mid Palaeozoic, whereas the delicate lacy fans of the latter create both prolific coarse sediment and form the cores of Late Palaeozoic deep-water, sub-photic biogenic mounds. Nearly all post-Palaeozoic bryozoan sediments comprise cyclostomes and cheilostomes with many of the same growth forms but with the addition of free-living colonies and significant numbers of articulated colonies. The latter produced sand and mud-sized bryozoan sediment via disarticulation for the first time. In contrast to the Palaeozoic, post-Palaeozoic bryozoans generated sediment varying more widely across the grain-size spectrum, from mud to sand to gravel. This article highlights the need to consider evolutionary changes in carbonate-producing organisms when interpreting facies changes through time.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12031" xmlns="http://purl.org/rss/1.0/"><title>Arsenic in framboidal pyrite from recent sediments of a shallow water lagoon of the Baltic Sea</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12031</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Arsenic in framboidal pyrite from recent sediments of a shallow water lagoon of the Baltic Sea</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Thomas Neumann, Florian Scholz, Utz Kramar, Michael Ostermaier, Nicole Rausch, Zsolt Berner</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-19T09:20:29.534902-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12031</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/">10.1111/sed.12031</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12031</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Arsenic is a redox-sensitive element of environmental relevance and often enriched in iron sulphides. Because sediments from the Achterwasser lagoon, a part of the estuarine system of the river Oder, south-west Baltic Sea, show unexpectedly high pyrite concentrations of up to 7·5 wt% they were used to investigate the influence of authigenic pyrite on the mobility and burial of As in the coastal environment. Micro-X-ray-fluorescence measurements of 106 micrometre-sized pyrite framboids from the anoxic sediments show highly variable As concentrations ranging from 6 to 1142 μg g<sup>−1</sup>. Even within a 1 cm thick layer, the As concentration of different framboids varies greatly and no clear depth trend is visible throughout the 50 cm long sediment core. Pyrite can account for 9 to 55% (average 22%) of the total As budget of the sediments and the degree of trace metalloid pyritization for As ranges from 26 to 61%, indicating that authigenic pyrite formation is an important process in the geochemical cycling of As in coastal sediments. High-resolution micro-X-ray fluorescence mapping of single pyrite grains shows that As is distributed inhomogeneously within larger framboids, suggesting changing pore water composition during pyrite growth. X-ray absorption near edge structure spectra indicate that As is usually present as As(-I) substituting S in the pyrite lattice. However, in samples close to the sediment/water interface a considerable part of As is in higher valence states (+III/+V). This can be explained by frequent re-suspension of the surficial sediments to the oxic water column due to wave action and subsequent re-deposition, leading to the adsorption of As oxyanions onto pyrite. Although reduced As(-I) becomes more important in the deeper samples, reflecting decreasing redox potential and a longer time since deposition, the occurrence of oxidized As species (AsIII/AsV) in pyrite in the anoxic part of the sediment suggests formation under dysoxic conditions.</p></div>
]]></content:encoded><description>

Arsenic is a redox-sensitive element of environmental relevance and often enriched in iron sulphides. Because sediments from the Achterwasser lagoon, a part of the estuarine system of the river Oder, south-west Baltic Sea, show unexpectedly high pyrite concentrations of up to 7·5 wt% they were used to investigate the influence of authigenic pyrite on the mobility and burial of As in the coastal environment. Micro-X-ray-fluorescence measurements of 106 micrometre-sized pyrite framboids from the anoxic sediments show highly variable As concentrations ranging from 6 to 1142 μg g−1. Even within a 1 cm thick layer, the As concentration of different framboids varies greatly and no clear depth trend is visible throughout the 50 cm long sediment core. Pyrite can account for 9 to 55% (average 22%) of the total As budget of the sediments and the degree of trace metalloid pyritization for As ranges from 26 to 61%, indicating that authigenic pyrite formation is an important process in the geochemical cycling of As in coastal sediments. High-resolution micro-X-ray fluorescence mapping of single pyrite grains shows that As is distributed inhomogeneously within larger framboids, suggesting changing pore water composition during pyrite growth. X-ray absorption near edge structure spectra indicate that As is usually present as As(-I) substituting S in the pyrite lattice. However, in samples close to the sediment/water interface a considerable part of As is in higher valence states (+III/+V). This can be explained by frequent re-suspension of the surficial sediments to the oxic water column due to wave action and subsequent re-deposition, leading to the adsorption of As oxyanions onto pyrite. Although reduced As(-I) becomes more important in the deeper samples, reflecting decreasing redox potential and a longer time since deposition, the occurrence of oxidized As species (AsIII/AsV) in pyrite in the anoxic part of the sediment suggests formation under dysoxic conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12033" xmlns="http://purl.org/rss/1.0/"><title>Techniques for assessing spatial heterogeneity of carbonate δ13C values: Implications for craton-wide isotope gradients</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12033</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Techniques for assessing spatial heterogeneity of carbonate δ13C values: Implications for craton-wide isotope gradients</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">J. Garrecht Metzger, David A. Fike</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-13T00:27:08.748495-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12033</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/">10.1111/sed.12033</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12033</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 sedimentary record of carbonate carbon isotopes (δ<sup>13</sup>C<sub>carb</sub>) provides one of the best methods for correlating marine strata and understanding the long-term evolution of the global carbon cycle. This work focuses on the Late Ordovician Guttenberg isotopic carbon excursion, a <em>ca</em> 2·5‰ positive δ<sup>13</sup>C<sub>carb</sub> excursion that is found in strata globally. Substantial variability in the apparent magnitude and stratigraphic morphology of the Guttenberg excursion at different localities has hampered high-resolution correlations and led to divergent reconstructions of ocean chemistry and the biogeochemical carbon cycle. This work investigates the magnitude, spatial scale and sources of isotopic variability of the Guttenberg excursion in two sections from Missouri, USA. Centimetre-scale isotope transects revealed variations in δ<sup>13</sup>C<sub>carb</sub> and δ<sup>18</sup>O<sub>carb</sub> greater than 2‰ across individual beds. Linear δ<sup>13</sup>C<sub>carb</sub> to δ<sup>18</sup>O<sub>carb</sub> mixing lines, together with petrographic and elemental abundance data, demonstrate that much of the isotopic scatter in single beds is due to mixing of isotopically distinct components. These patterns facilitated objective sample screening to determine the ‘least-altered’ data. A δ<sup>18</sup>O<sub>carb</sub> filter based on empirical δ<sup>18</sup>O<sub>carb</sub> values of well-preserved carbonate mudstones allowed further sample discrimination. The resulting ‘least-altered’ δ<sup>13</sup>C<sub>carb</sub> profile improves the understanding of regional as well as continental-scale stratigraphic relations in this interval. Correlations with other Laurentian sections strongly suggest that: (i) small-scale variability in Guttenberg excursion δ<sup>13</sup>C<sub>carb</sub> values may result in part from local diagenetic overprinting; (ii) peak-Guttenberg excursion δ<sup>13</sup>C<sub>carb</sub> values of the Midcontinent are not distinct from their Taconic equivalents; and (iii) no primary continental-scale spatial gradient in δ<sup>13</sup>C<sub>carb</sub> (for example, arising from chemically distinct ‘aquafacies’) is required during Guttenberg excursion-time. This study demonstrates the importance of detailed petrographic and geochemical screening of samples to be used for δ<sup>13</sup>C<sub>carb</sub> chemostratigraphy and for enhancing understanding of epeiric ocean chemistry.</p></div>
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The sedimentary record of carbonate carbon isotopes (δ13Ccarb) provides one of the best methods for correlating marine strata and understanding the long-term evolution of the global carbon cycle. This work focuses on the Late Ordovician Guttenberg isotopic carbon excursion, a ca 2·5‰ positive δ13Ccarb excursion that is found in strata globally. Substantial variability in the apparent magnitude and stratigraphic morphology of the Guttenberg excursion at different localities has hampered high-resolution correlations and led to divergent reconstructions of ocean chemistry and the biogeochemical carbon cycle. This work investigates the magnitude, spatial scale and sources of isotopic variability of the Guttenberg excursion in two sections from Missouri, USA. Centimetre-scale isotope transects revealed variations in δ13Ccarb and δ18Ocarb greater than 2‰ across individual beds. Linear δ13Ccarb to δ18Ocarb mixing lines, together with petrographic and elemental abundance data, demonstrate that much of the isotopic scatter in single beds is due to mixing of isotopically distinct components. These patterns facilitated objective sample screening to determine the ‘least-altered’ data. A δ18Ocarb filter based on empirical δ18Ocarb values of well-preserved carbonate mudstones allowed further sample discrimination. The resulting ‘least-altered’ δ13Ccarb profile improves the understanding of regional as well as continental-scale stratigraphic relations in this interval. Correlations with other Laurentian sections strongly suggest that: (i) small-scale variability in Guttenberg excursion δ13Ccarb values may result in part from local diagenetic overprinting; (ii) peak-Guttenberg excursion δ13Ccarb values of the Midcontinent are not distinct from their Taconic equivalents; and (iii) no primary continental-scale spatial gradient in δ13Ccarb (for example, arising from chemically distinct ‘aquafacies’) is required during Guttenberg excursion-time. This study demonstrates the importance of detailed petrographic and geochemical screening of samples to be used for δ13Ccarb chemostratigraphy and for enhancing understanding of epeiric ocean chemistry.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12038" xmlns="http://purl.org/rss/1.0/"><title>Oxygenation of shallow marine environments and chemical sedimentation in Palaeoproterozoic peritidal settings: Frere Formation, Western Australia</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12038</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Oxygenation of shallow marine environments and chemical sedimentation in Palaeoproterozoic peritidal settings: Frere Formation, Western Australia</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Sara J. Akin, Peir K. Pufahl, Eric E. Hiatt, Franco Pirajno</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-04-08T01:49:38.731553-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12038</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/">10.1111/sed.12038</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12038</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original Manuscript</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 Palaeoproterozoic Frere Formation (<em>ca</em> 1.89 Gyr old) of the Earaheedy Basin, Western Australia, is a <em>ca</em> 600 m thick succession of iron formation and fine-grained, clastic sedimentary rocks that accumulated on an unrimmed continental margin with oceanic upwelling. Lithofacies stacking patterns suggest that deposition occurred during a marine transgression punctuated by higher frequency relative sea-level fluctuations that produced five parasequences. Decametre-scale parasequences are defined by flooding surfaces overlain by either laminated magnetite or magnetite-bearing, hummocky cross-stratified sandstone that grades upward into interbedded hematite-rich mudstone and trough cross-stratified granular iron formation. Each aggradational cycle is interpreted to record progradation of intertidal and tidal channel sediments over shallow subtidal and storm-generated deposits of the middle shelf. The presence of aeolian deposits, mud cracks and absence of coarse clastics indicate deposition along an arid coastline with significant wind-blown sediment input. Iron formation in the Frere Formation, in contrast to most other Palaeoproterozoic examples, was deposited almost exclusively in peritidal environments. These other continental margin iron formations also reflect upwelling of anoxic, Fe-rich sea water, but accumulated in the full spectrum of shelf environments. Dilution by fine-grained, windblown terrigenous clastic sediment probably prevented the Frere iron formation from forming in deeper settings. Lithofacies associations and interpreted paragenetic pathways of Fe-rich lithofacies further suggest precipitation in sea water with a prominent oxygen chemocline. Although essentially unmetamorphosed, the complex diagenetic history of the Frere Formation demonstrates that understanding the alteration of iron formation is a prerequisite for any investigation seeking to interpret ocean-atmosphere evolution. Unlike studies that focus exclusively on their chemistry, an approach that also considers palaeoenvironment and oceanography, as well the effects of post-depositional fluid flow and alteration, mitigates the potential for incorrectly interpreting geochemical data.</p></div>
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The Palaeoproterozoic Frere Formation (ca 1.89 Gyr old) of the Earaheedy Basin, Western Australia, is a ca 600 m thick succession of iron formation and fine-grained, clastic sedimentary rocks that accumulated on an unrimmed continental margin with oceanic upwelling. Lithofacies stacking patterns suggest that deposition occurred during a marine transgression punctuated by higher frequency relative sea-level fluctuations that produced five parasequences. Decametre-scale parasequences are defined by flooding surfaces overlain by either laminated magnetite or magnetite-bearing, hummocky cross-stratified sandstone that grades upward into interbedded hematite-rich mudstone and trough cross-stratified granular iron formation. Each aggradational cycle is interpreted to record progradation of intertidal and tidal channel sediments over shallow subtidal and storm-generated deposits of the middle shelf. The presence of aeolian deposits, mud cracks and absence of coarse clastics indicate deposition along an arid coastline with significant wind-blown sediment input. Iron formation in the Frere Formation, in contrast to most other Palaeoproterozoic examples, was deposited almost exclusively in peritidal environments. These other continental margin iron formations also reflect upwelling of anoxic, Fe-rich sea water, but accumulated in the full spectrum of shelf environments. Dilution by fine-grained, windblown terrigenous clastic sediment probably prevented the Frere iron formation from forming in deeper settings. Lithofacies associations and interpreted paragenetic pathways of Fe-rich lithofacies further suggest precipitation in sea water with a prominent oxygen chemocline. Although essentially unmetamorphosed, the complex diagenetic history of the Frere Formation demonstrates that understanding the alteration of iron formation is a prerequisite for any investigation seeking to interpret ocean-atmosphere evolution. Unlike studies that focus exclusively on their chemistry, an approach that also considers palaeoenvironment and oceanography, as well the effects of post-depositional fluid flow and alteration, mitigates the potential for incorrectly interpreting geochemical data.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12026" xmlns="http://purl.org/rss/1.0/"><title>Impact of dynamic sedimentation on facies heterogeneities in Lower Cretaceous peritidal deposits of central east Oman</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12026</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Impact of dynamic sedimentation on facies heterogeneities in Lower Cretaceous peritidal deposits of central east Oman</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Claire M. Sena, Cédric M. John</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-30T00:43:37.803142-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12026</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/">10.1111/sed.12026</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12026</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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, based in the Haushi-Huqf area of central east Oman, aims to characterize the controls on facies distribution and geometries of some of the best preserved examples of Lower Cretaceous tidal flat facies within the Tethyan epeiric platform. Field, petrographic and geochemical data were acquired from the Barremian–Aptian Jurf and Qishn formations that crop out in a 500 × 1000 m<sup>2</sup> butte, thus allowing for pseudo three-dimensional quantitative data acquisition of the dimensions and spatial distributions of discontinuity surfaces and sedimentary bodies. The interpretation presented here suggests that the main processes impacting sedimentation in the Lower Cretaceous peritidal environment of the Haushi-Huqf were transport and erosion processes related to storm waves and currents. The vertical evolution of the carbonate system is organized into six types of metre-scale depositional sequences, from subtidal dominated sequences to supratidal-capped sequences, which are bounded by regional discontinuity surfaces. At subaerial exposure and submarine erosion surfaces associated with a base level shift, sedimentary horizons along the entire depositional profile are cut by scours possibly created by storm events. Chemostratigraphy allows correlation between the Haushi-Huqf and the age-equivalent sections logged in the interior of the platform in Oman. The correlation suggests that the change from subtidal to intertidal depositional sequences during the late highstand is coeval with the development of rudist dominated shoals on the shelf. This study is the first to discuss the controls on Lower Cretaceous peritidal carbonate cyclicity of the Arabian epeiric platform. The results presented here also offer a unique quantitative dataset of the distribution and dimensions of peritidal carbonate shoals and storm scours in a regional sequence stratigraphic context.</p></div>
]]></content:encoded><description>

This study, based in the Haushi-Huqf area of central east Oman, aims to characterize the controls on facies distribution and geometries of some of the best preserved examples of Lower Cretaceous tidal flat facies within the Tethyan epeiric platform. Field, petrographic and geochemical data were acquired from the Barremian–Aptian Jurf and Qishn formations that crop out in a 500 × 1000 m2 butte, thus allowing for pseudo three-dimensional quantitative data acquisition of the dimensions and spatial distributions of discontinuity surfaces and sedimentary bodies. The interpretation presented here suggests that the main processes impacting sedimentation in the Lower Cretaceous peritidal environment of the Haushi-Huqf were transport and erosion processes related to storm waves and currents. The vertical evolution of the carbonate system is organized into six types of metre-scale depositional sequences, from subtidal dominated sequences to supratidal-capped sequences, which are bounded by regional discontinuity surfaces. At subaerial exposure and submarine erosion surfaces associated with a base level shift, sedimentary horizons along the entire depositional profile are cut by scours possibly created by storm events. Chemostratigraphy allows correlation between the Haushi-Huqf and the age-equivalent sections logged in the interior of the platform in Oman. The correlation suggests that the change from subtidal to intertidal depositional sequences during the late highstand is coeval with the development of rudist dominated shoals on the shelf. This study is the first to discuss the controls on Lower Cretaceous peritidal carbonate cyclicity of the Arabian epeiric platform. The results presented here also offer a unique quantitative dataset of the distribution and dimensions of peritidal carbonate shoals and storm scours in a regional sequence stratigraphic context.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12025" xmlns="http://purl.org/rss/1.0/"><title>Aragonite stromatolitic buildups from Santorini (Aegean Sea, Greece): Geochemical and palaeontological constraints of the caldera palaeoenvironment prior to the Minoan eruption (ca 3600 yr bp)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12025</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Aragonite stromatolitic buildups from Santorini (Aegean Sea, Greece): Geochemical and palaeontological constraints of the caldera palaeoenvironment prior to the Minoan eruption (ca 3600 yr bp)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Pere Anadón, Carles Canet, Walter L. Friedrich</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-14T06:50:16.667233-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12025</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/">10.1111/sed.12025</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12025</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 pyroclastic deposits of the Minoan eruption (<em>ca</em> 3600 yr <span class="smallCaps">bp</span>) in Santorini contain abundant xenoliths. Most of these deposits are calcareous blocks of laminated-botryoidal, stromatolite-like buildups that formed in the shallow waters of the flooded pre-Minoan caldera; they consist of (i) light laminae, of fibrous aragonite arranged perpendicular to layering, and (ii) dark laminae, with calcified filaments of probable biological origin. These microstructures are absent in the light laminae, suggesting a predominant inorganic precipitation of aragonite on substrates probably colonized by microbes. Internal cavities contain loose skeletal grains (molluscs, ostracods, foraminifera and diatoms) that comprise taxa typical of shallow marine and/or lagoon environments. Most of these forms are typical of warm water environments, although no typical taxa from hydrothermal vents have been observed. Past gasohydrothermal venting is recorded by the occurrence of barite, pyrolusite and pyrite traces. The most striking features of the stable isotopic data set are: (i) an overall wide range in δ<sup>13</sup>C<sub>PDB</sub> (0·16 to 12·97‰) with a narrower variation for δ<sup>18</sup>O<sub>PDB</sub> (−0·23 to 4·33‰); and (ii) a relatively uniform isotopic composition for the fibrous aragonite (δ<sup>13</sup>C = 12·40 ± 0·43‰ and δ<sup>18</sup>O = 2·42 ± 0·77‰, <em>n </em>= 21). The δ<sup>13</sup>C and δ<sup>18</sup>O values from molluscs and ostracods display a covariant trend, which reflects a mixing between sea water and a fluid influenced by volcano-hydrothermal activity. Accordingly, <sup>87</sup>Sr/<sup>86</sup>Sr from the studied carbonates (0·708758 to 0·709011 in fibrous aragonite and 0·708920 to 0·708991 in molluscs) suggests that the aragonite buildups developed in sea water under the influence of a hydrothermal/volcanic source. Significant differences in trace elements have been detected between the fibrous aragonite and modern marine aragonite cements. The caldera water from which the fibrous aragonite crusts formed received an input from a volcano-hydrothermal system, probably producing diffuse venting of volcanogenic CO<sub>2</sub> gas and of a fluid enriched in Ca, Mn and Ba, and depleted in Mg and probably in Sr.</p></div>
]]></content:encoded><description>

The pyroclastic deposits of the Minoan eruption (ca 3600 yr bp) in Santorini contain abundant xenoliths. Most of these deposits are calcareous blocks of laminated-botryoidal, stromatolite-like buildups that formed in the shallow waters of the flooded pre-Minoan caldera; they consist of (i) light laminae, of fibrous aragonite arranged perpendicular to layering, and (ii) dark laminae, with calcified filaments of probable biological origin. These microstructures are absent in the light laminae, suggesting a predominant inorganic precipitation of aragonite on substrates probably colonized by microbes. Internal cavities contain loose skeletal grains (molluscs, ostracods, foraminifera and diatoms) that comprise taxa typical of shallow marine and/or lagoon environments. Most of these forms are typical of warm water environments, although no typical taxa from hydrothermal vents have been observed. Past gasohydrothermal venting is recorded by the occurrence of barite, pyrolusite and pyrite traces. The most striking features of the stable isotopic data set are: (i) an overall wide range in δ13CPDB (0·16 to 12·97‰) with a narrower variation for δ18OPDB (−0·23 to 4·33‰); and (ii) a relatively uniform isotopic composition for the fibrous aragonite (δ13C = 12·40 ± 0·43‰ and δ18O = 2·42 ± 0·77‰, n = 21). The δ13C and δ18O values from molluscs and ostracods display a covariant trend, which reflects a mixing between sea water and a fluid influenced by volcano-hydrothermal activity. Accordingly, 87Sr/86Sr from the studied carbonates (0·708758 to 0·709011 in fibrous aragonite and 0·708920 to 0·708991 in molluscs) suggests that the aragonite buildups developed in sea water under the influence of a hydrothermal/volcanic source. Significant differences in trace elements have been detected between the fibrous aragonite and modern marine aragonite cements. The caldera water from which the fibrous aragonite crusts formed received an input from a volcano-hydrothermal system, probably producing diffuse venting of volcanogenic CO2 gas and of a fluid enriched in Ca, Mn and Ba, and depleted in Mg and probably in Sr.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12027" xmlns="http://purl.org/rss/1.0/"><title>Internal architecture and evolution of bioclastic beach ridges in a megatidal chenier plain: Field data and wave flume experiment</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12027</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Internal architecture and evolution of bioclastic beach ridges in a megatidal chenier plain: Field data and wave flume experiment</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Pierre Weill, Dominique Mouazé, Bernadette Tessier</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-03-14T01:29:36.436235-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12027</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/">10.1111/sed.12027</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12027</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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>Beach ridges in macrotidal environments experience strong multi-annual to multi-decennial fluctuations of tidal inundation. The duration of tide flooding directly controls the duration of sediment reworking by waves, and thus the ridge dynamics. Flume modelling was used to investigate the impact of low-frequency tidal cycles on beach ridge evolution and internal architecture. The experiment was performed using natural bioclastic sediment, constant wave parameters and low-frequency variations of the mean water level. The morphological response of the beach ridge to water level fluctuations and the preservation of sedimentary structures were monitored by using side-view and plan-view photographs. Results were compared with the internal architecture of modern bioclastic beach ridges in a macrotidal chenier plain (Mont St. Michel Bay, France) surveyed with ground-penetrating radar. The experimentally obtained morphologies and internal structures matched those observed in the field, and the three ridge development stages identified in ground-penetrating radar profiles (early transgressive, late transgressive and progradational) were modelled successfully. Flume experiments indicate that flat bioclastic shapes play a key role in sediment sorting in the breaker zone, and in sediment layering in the beach and washover fans. Water level controls washover geometry, beach ridge evolution and internal structure. Low water levels allow beach ridge stabilization and sediment accumulation lower on tidal flats. During subsequent water level rise, accumulated sediment becomes available for deposition of new washover units and for bayward extension of the beach ridges. In the field, low-frequency water level fluctuations are related to the 4·4 year and 18·6 year tidal cycles. Experimental results suggest that these cycles may represent the underlying factor in the evolution of the macrotidal chenier coast at the multi-decadal to centennial time scale.</p></div>
]]></content:encoded><description>

Beach ridges in macrotidal environments experience strong multi-annual to multi-decennial fluctuations of tidal inundation. The duration of tide flooding directly controls the duration of sediment reworking by waves, and thus the ridge dynamics. Flume modelling was used to investigate the impact of low-frequency tidal cycles on beach ridge evolution and internal architecture. The experiment was performed using natural bioclastic sediment, constant wave parameters and low-frequency variations of the mean water level. The morphological response of the beach ridge to water level fluctuations and the preservation of sedimentary structures were monitored by using side-view and plan-view photographs. Results were compared with the internal architecture of modern bioclastic beach ridges in a macrotidal chenier plain (Mont St. Michel Bay, France) surveyed with ground-penetrating radar. The experimentally obtained morphologies and internal structures matched those observed in the field, and the three ridge development stages identified in ground-penetrating radar profiles (early transgressive, late transgressive and progradational) were modelled successfully. Flume experiments indicate that flat bioclastic shapes play a key role in sediment sorting in the breaker zone, and in sediment layering in the beach and washover fans. Water level controls washover geometry, beach ridge evolution and internal structure. Low water levels allow beach ridge stabilization and sediment accumulation lower on tidal flats. During subsequent water level rise, accumulated sediment becomes available for deposition of new washover units and for bayward extension of the beach ridges. In the field, low-frequency water level fluctuations are related to the 4·4 year and 18·6 year tidal cycles. Experimental results suggest that these cycles may represent the underlying factor in the evolution of the macrotidal chenier coast at the multi-decadal to centennial time scale.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12024" xmlns="http://purl.org/rss/1.0/"><title>Implications of trace element composition of syntaxial quartz cements for the geochemical conditions during quartz precipitation in sandstones</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12024</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Implications of trace element composition of syntaxial quartz cements for the geochemical conditions during quartz precipitation in sandstones</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">Thomas Götte, Karl Ramseyer, Thomas Pettke, Monika Koch-Müller</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-02-25T03:22:07.52729-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12024</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/">10.1111/sed.12024</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12024</prism:url><prism:section xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">Original 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 petrographic investigation revealed polyphase quartz cementation in the Finefrau Sandstone (Upper Carboniferous, Western Germany) and the Solling Sandstone (Lower Triassic, Central Germany). Three different cements could be distinguished in each sandstone based on their cathodoluminescence and trace element composition. The first quartz generation is suggested to have been formed during eogenesis due to dissolution and replacement of feldspar. The mesogenetic paragenesis comprises two generations of quartz and illite, which are accompanied by albite in the Solling Sandstone. Sharp luminescence zoning in quartz overgrowths points to distinct episodes of cementation in both sandstones. Significant amounts of Al, Li and H and traces of Ge and B have been detected in the quartz overgrowths. The Al-content of the quartz cements in the Finefrau Sandstones exceeds that in the quartz cements in the Solling Sandstone by a factor of five. It is suggested that this compositional variation reflects the conditions in the pore-water, such as temperature and pH. The Al-concentration is generally correlated to the Li-content with the exception of the latest quartz generation in the Finefrau Sandstones which is also most enriched in trace elements. The ratio of Li/Al varies between 0·11 and 0·25 in the two sandstones. The Li/H-ratio, which ranges from 0·12 to 0·3, is controlled by the activity ratio of Li and H in the pore fluid. Clay minerals are the most important source for Li and high salinities favour the mobilization of Li during diagenesis. Thus, a relatively low salinity and low pH are responsible for the low Li/H-ratio in the Finefrau Sandstone, while high salinity and neutral to alkaline pH results in a high Li/H-ratio for the Solling Sandstone. The Ge-contents are generally near the average of detrital quartz and indicate that pressure dissolution is a major source for quartz cementation. Different chemical compositions of distinct quartz generations indicate changes in the physico-chemical conditions and point to mobilization of silica from different sources (for example, pressure solution and clay mineral transformations).</p></div>
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A petrographic investigation revealed polyphase quartz cementation in the Finefrau Sandstone (Upper Carboniferous, Western Germany) and the Solling Sandstone (Lower Triassic, Central Germany). Three different cements could be distinguished in each sandstone based on their cathodoluminescence and trace element composition. The first quartz generation is suggested to have been formed during eogenesis due to dissolution and replacement of feldspar. The mesogenetic paragenesis comprises two generations of quartz and illite, which are accompanied by albite in the Solling Sandstone. Sharp luminescence zoning in quartz overgrowths points to distinct episodes of cementation in both sandstones. Significant amounts of Al, Li and H and traces of Ge and B have been detected in the quartz overgrowths. The Al-content of the quartz cements in the Finefrau Sandstones exceeds that in the quartz cements in the Solling Sandstone by a factor of five. It is suggested that this compositional variation reflects the conditions in the pore-water, such as temperature and pH. The Al-concentration is generally correlated to the Li-content with the exception of the latest quartz generation in the Finefrau Sandstones which is also most enriched in trace elements. The ratio of Li/Al varies between 0·11 and 0·25 in the two sandstones. The Li/H-ratio, which ranges from 0·12 to 0·3, is controlled by the activity ratio of Li and H in the pore fluid. Clay minerals are the most important source for Li and high salinities favour the mobilization of Li during diagenesis. Thus, a relatively low salinity and low pH are responsible for the low Li/H-ratio in the Finefrau Sandstone, while high salinity and neutral to alkaline pH results in a high Li/H-ratio for the Solling Sandstone. The Ge-contents are generally near the average of detrital quartz and indicate that pressure dissolution is a major source for quartz cementation. Different chemical compositions of distinct quartz generations indicate changes in the physico-chemical conditions and point to mobilization of silica from different sources (for example, pressure solution and clay mineral transformations).
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01344.x" xmlns="http://purl.org/rss/1.0/"><title>Spatial variability of watermass conditions within the European Epicontinental Seaway during the Early Jurassic (Pliensbachian–Toarcian)</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01344.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Spatial variability of watermass conditions within the European Epicontinental Seaway during the Early Jurassic (Pliensbachian–Toarcian)</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">DARIO HARAZIM, BAS VAN DE SCHOOTBRUGGE, KATRIN SORICHTER, JENS FIEBIG, ANDRIES WEUG, GUILLAUME SUAN, WOLFGANG OSCHMANN</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-08-21T10:59:55.166329-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01344.x</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/">10.1111/j.1365-3091.2012.01344.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01344.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">359</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">390</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 order to constrain spatial variability in watermass conditions within the European Epicontinental Seaway prior to, during and after the Toarcian Oceanic Anoxic Event, carbon (δ<sup>13</sup>C<sub>bel</sub>, δ<sup>13</sup>C<sub>carb</sub>) and oxygen (δ<sup>18</sup>O<sub>bel</sub>, δ<sup>18</sup>O<sub>carb</sub>) isotope records were obtained from three sections in the Grands Causses Basin (southern France). These data were then compared with similar records along a north–south transect across the European Epicontinental Seaway. As the conclusions reached here strongly depend on the reliability of belemnite calcites as archives of palaeoceanographic changes, an attempt was made to improve the understanding of isotope signals recorded in belemnite calcite. Intra-rostral carbon and oxygen-isotope data from six belemnite specimens belonging to the genus <em>Passaloteuthis</em> were collected. Intra-rostral carbon-isotopes are influenced by vital effects, whereas oxygen-isotopes reflect relative changes in temperature and salinity. Palaeotemperatures calculated from δ<sup>18</sup>O<sub>bel</sub>-isotope records from the Grands Causses Basin confirm relatively low temperatures throughout the Late Pliensbachian. Similar cool water conditions have previously been shown in Germany, England, Spain and Portugal. A temperature increase of up to 6 °C is observed across the Pliensbachian–Toarcian boundary. A pronounced negative shift of at least −3‰ (Vienna-Pee Dee Belemnite) is recorded in bulk carbonate carbon during the lower <em>Harpoceras serpentinum</em> zone, typical of the Toarcian Oceanic Anoxic Event. Before and after the Toarcian Oceanic Anoxic Event, a good correlation between δ<sup>13</sup>C<sub>carb</sub> and δ<sup>13</sup>C<sub>bel</sub> exists, indicating well-ventilated bottom-waters and normal marine conditions. Instead, data for the Toarcian Oceanic Anoxic Event indicate the development of a strong north–south gradient in salinity stratification and surface-water productivity for the Western Tethyan realm. This study thus lends further support to a pronounced regional overprint on carbon and oxygen-isotope records in epicontinental seaways.</p></div>
]]></content:encoded><description>

In order to constrain spatial variability in watermass conditions within the European Epicontinental Seaway prior to, during and after the Toarcian Oceanic Anoxic Event, carbon (δ13Cbel, δ13Ccarb) and oxygen (δ18Obel, δ18Ocarb) isotope records were obtained from three sections in the Grands Causses Basin (southern France). These data were then compared with similar records along a north–south transect across the European Epicontinental Seaway. As the conclusions reached here strongly depend on the reliability of belemnite calcites as archives of palaeoceanographic changes, an attempt was made to improve the understanding of isotope signals recorded in belemnite calcite. Intra-rostral carbon and oxygen-isotope data from six belemnite specimens belonging to the genus Passaloteuthis were collected. Intra-rostral carbon-isotopes are influenced by vital effects, whereas oxygen-isotopes reflect relative changes in temperature and salinity. Palaeotemperatures calculated from δ18Obel-isotope records from the Grands Causses Basin confirm relatively low temperatures throughout the Late Pliensbachian. Similar cool water conditions have previously been shown in Germany, England, Spain and Portugal. A temperature increase of up to 6 °C is observed across the Pliensbachian–Toarcian boundary. A pronounced negative shift of at least −3‰ (Vienna-Pee Dee Belemnite) is recorded in bulk carbonate carbon during the lower Harpoceras serpentinum zone, typical of the Toarcian Oceanic Anoxic Event. Before and after the Toarcian Oceanic Anoxic Event, a good correlation between δ13Ccarb and δ13Cbel exists, indicating well-ventilated bottom-waters and normal marine conditions. Instead, data for the Toarcian Oceanic Anoxic Event indicate the development of a strong north–south gradient in salinity stratification and surface-water productivity for the Western Tethyan realm. This study thus lends further support to a pronounced regional overprint on carbon and oxygen-isotope records in epicontinental seaways.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01345.x" xmlns="http://purl.org/rss/1.0/"><title>Depositional processes beneath coastal multi-year sea ice</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01345.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Depositional processes beneath coastal multi-year sea ice</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">KATHERINE T. MURRAY, MOLLY F. MILLER, SAMUEL S. BOWSER</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-07-27T07:00:53.007762-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01345.x</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/">10.1111/j.1365-3091.2012.01345.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01345.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">391</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">410</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 extent of multi-year sea ice impacts climate processes worldwide, such as ocean–atmosphere carbon dioxide exchange and deep ocean current formation. Reconstructing these processes in the past, and assessing the distribution of ecologically and climatically significant features, such as polynas, requires recognition of sediments deposited under multi-year sea ice, but little is known about their characteristics. Textural analysis of subaerial and sea floor sediment in Explorers Cove, McMurdo Sound, at the mouth of Taylor Valley, Antarctica, augmented with observations of sedimentary structures and faunal components, elucidates how sediment is transported to the sea floor and allows characterization of the deposits. Comparison of grain-size characteristics of subaerial (moraine, delta and sea-ice surface) sediment and sea floor sediment from short cores taken at depths of 7 to 25 m indicates that the likely source of the moderately to poorly sorted sea floor sand is deltaic sediment; small glacial meltwater streams have built deltas since Taylor Valley became ice-free <em>ca</em> 7000 years ago. Windblown sediment accumulating on the multi-year sea ice close to the coast typically is coarser grained than sediment on the sea floor; this suggests that the transport of sediment through the ice to the sea floor is not the predominant mode of sediment transfer. However, supra-sea-ice sediment does move to the sea floor through local fractures. The rate of sedimentation under multi-year sea ice is low because of limited stream flow and biogenic sedimentation; the ice cover inhibits primary productivity and dampens waves, precluding physical re-suspension. The upper centimetres of sea floor sediment are churned by epifaunal scallops and brittle stars that leave no telltale biogenic structures and whose calcite ossicles and shells may be poorly preserved. The resulting deposits under multi-year sea ice are poorly sorted, massive sand that provides little evidence of the bioturbators that have masked the indicators of the original physical depositional processes.</p></div>
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The extent of multi-year sea ice impacts climate processes worldwide, such as ocean–atmosphere carbon dioxide exchange and deep ocean current formation. Reconstructing these processes in the past, and assessing the distribution of ecologically and climatically significant features, such as polynas, requires recognition of sediments deposited under multi-year sea ice, but little is known about their characteristics. Textural analysis of subaerial and sea floor sediment in Explorers Cove, McMurdo Sound, at the mouth of Taylor Valley, Antarctica, augmented with observations of sedimentary structures and faunal components, elucidates how sediment is transported to the sea floor and allows characterization of the deposits. Comparison of grain-size characteristics of subaerial (moraine, delta and sea-ice surface) sediment and sea floor sediment from short cores taken at depths of 7 to 25 m indicates that the likely source of the moderately to poorly sorted sea floor sand is deltaic sediment; small glacial meltwater streams have built deltas since Taylor Valley became ice-free ca 7000 years ago. Windblown sediment accumulating on the multi-year sea ice close to the coast typically is coarser grained than sediment on the sea floor; this suggests that the transport of sediment through the ice to the sea floor is not the predominant mode of sediment transfer. However, supra-sea-ice sediment does move to the sea floor through local fractures. The rate of sedimentation under multi-year sea ice is low because of limited stream flow and biogenic sedimentation; the ice cover inhibits primary productivity and dampens waves, precluding physical re-suspension. The upper centimetres of sea floor sediment are churned by epifaunal scallops and brittle stars that leave no telltale biogenic structures and whose calcite ossicles and shells may be poorly preserved. The resulting deposits under multi-year sea ice are poorly sorted, massive sand that provides little evidence of the bioturbators that have masked the indicators of the original physical depositional processes.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01346.x" xmlns="http://purl.org/rss/1.0/"><title>An interglacial on snowball Earth? Dynamic ice behaviour revealed in the Chuos Formation, Namibia</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01346.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">An interglacial on snowball Earth? Dynamic ice behaviour revealed in the Chuos Formation, Namibia</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">DANIEL P. LE HERON, MARIE E. BUSFIELD, FRED KAMONA</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-08-02T11:51:16.357998-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01346.x</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/">10.1111/j.1365-3091.2012.01346.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01346.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">411</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">427</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 Sturtian is the oldest (<em>ca</em> 716 Ma) of three pan-global glaciations in the Cryogenian. At Omutirapo, in northern Namibia, a 2 km wide, 400 m deep palaeovalley is filled by glaciogenic strata of the Chuos Formation, which represents the Sturtian glacial record. Sedimentary logging of an exceptionally high-quality exposure permits detailed stratigraphic descriptions and interpretations, allowing two glacial cycles to be identified. At the base of the exposed succession, strong evidence supporting glaciation includes diamictites, ice-rafted dropstones and intensely sheared zones of interpreted subglacial origin. These facies collectively represent ice-proximal to ice-rafted deposits. Upsection, dropstone-free mudstones in the middle of the succession, and the absence of diamictites, imply sedimentation free from glacial influence. However, the reappearance of glacial deposits above indicates a phase of Sturtian glacial re-advance. Comparison with age-equivalent strata in South Australia, where evidence for sea-ice free sedimentation has been established previously, suggests that a Sturtian interglacial may have been extensive, implying global-scale waxing and waning of ice sheets during a Cryogenian glacial event.</p></div>
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The Sturtian is the oldest (ca 716 Ma) of three pan-global glaciations in the Cryogenian. At Omutirapo, in northern Namibia, a 2 km wide, 400 m deep palaeovalley is filled by glaciogenic strata of the Chuos Formation, which represents the Sturtian glacial record. Sedimentary logging of an exceptionally high-quality exposure permits detailed stratigraphic descriptions and interpretations, allowing two glacial cycles to be identified. At the base of the exposed succession, strong evidence supporting glaciation includes diamictites, ice-rafted dropstones and intensely sheared zones of interpreted subglacial origin. These facies collectively represent ice-proximal to ice-rafted deposits. Upsection, dropstone-free mudstones in the middle of the succession, and the absence of diamictites, imply sedimentation free from glacial influence. However, the reappearance of glacial deposits above indicates a phase of Sturtian glacial re-advance. Comparison with age-equivalent strata in South Australia, where evidence for sea-ice free sedimentation has been established previously, suggests that a Sturtian interglacial may have been extensive, implying global-scale waxing and waning of ice sheets during a Cryogenian glacial event.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01347.x" xmlns="http://purl.org/rss/1.0/"><title>Impact of lake-level changes on the formation of thermogene travertine in continental rifts: Evidence from Lake Bogoria, Kenya Rift Valley</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01347.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Impact of lake-level changes on the formation of thermogene travertine in continental rifts: Evidence from Lake Bogoria, Kenya Rift Valley</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">ROBIN W. RENAUT, R. BERNHART OWEN, BRIAN JONES, JEAN-JACQUES TIERCELIN, CORINNE TARITS, JOHN K. EGO, KURT O. KONHAUSER</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-08-28T11:20:38.450818-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01347.x</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/">10.1111/j.1365-3091.2012.01347.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01347.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">428</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">468</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>Travertine is present at 20% of the <em>ca</em> 60 hot springs that discharge on Loburu delta plain on the western margin of saline, alkaline Lake Bogoria in the Kenya Rift. Much of the travertine, which forms mounds, low terraces and pool-rim dams, is sub-fossil (relict) and undergoing erosion, but calcite-encrusted artefacts show that carbonate is actively precipitating at several springs. Most of the springs discharge alkaline (pH: 8·3 to 8·9), Na-HCO<sub>3</sub> waters containing little Ca (&lt;2 mg l<sup>−1</sup>) at temperatures of 94 to 97·5°C. These travertines are unusual because most probably precipitated at temperatures of &gt;80°C. The travertines are composed mainly of dendritic and platy calcite, with minor Mg-silicates, aragonite, fluorite and opaline silica. Calcite precipitation is attributed mainly to rapid CO<sub>2</sub> degassing, which led to high-disequilibrium crystal morphologies. Stratigraphic evidence shows that the travertine formed during several stages separated by intervals of non-deposition. Radiometric ages imply that the main phase of travertine formation occurred during the late Pleistocene (<em>ca</em> 32 to 35 ka). Periods of precipitation were influenced strongly by fluctuations in lake level, mostly under climate control, and by related changes in the depth of boiling. During relatively arid phases, meteoric recharge of ground water declines, the lake is low and becomes hypersaline, and the reduced hydrostatic pressure lowers the level of boiling in the plumbing system of the hot springs. Any carbonate precipitation then occurs below the land surface. During humid phases, the dilute meteoric recharge increases, enhancing geothermal circulation, but the rising lake waters, which become relatively dilute, flood most spring vents. Much of the aqueous Ca<sup>2+</sup> then precipitates as lacustrine stromatolites on shallow firm substrates, including submerged older travertines. Optimal conditions for subaerial travertine precipitation at Loburu occur when the lake is at intermediate levels, and may be favoured during transitions from humid to drier conditions.</p></div>
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Travertine is present at 20% of the ca 60 hot springs that discharge on Loburu delta plain on the western margin of saline, alkaline Lake Bogoria in the Kenya Rift. Much of the travertine, which forms mounds, low terraces and pool-rim dams, is sub-fossil (relict) and undergoing erosion, but calcite-encrusted artefacts show that carbonate is actively precipitating at several springs. Most of the springs discharge alkaline (pH: 8·3 to 8·9), Na-HCO3 waters containing little Ca (&lt;2 mg l−1) at temperatures of 94 to 97·5°C. These travertines are unusual because most probably precipitated at temperatures of &gt;80°C. The travertines are composed mainly of dendritic and platy calcite, with minor Mg-silicates, aragonite, fluorite and opaline silica. Calcite precipitation is attributed mainly to rapid CO2 degassing, which led to high-disequilibrium crystal morphologies. Stratigraphic evidence shows that the travertine formed during several stages separated by intervals of non-deposition. Radiometric ages imply that the main phase of travertine formation occurred during the late Pleistocene (ca 32 to 35 ka). Periods of precipitation were influenced strongly by fluctuations in lake level, mostly under climate control, and by related changes in the depth of boiling. During relatively arid phases, meteoric recharge of ground water declines, the lake is low and becomes hypersaline, and the reduced hydrostatic pressure lowers the level of boiling in the plumbing system of the hot springs. Any carbonate precipitation then occurs below the land surface. During humid phases, the dilute meteoric recharge increases, enhancing geothermal circulation, but the rising lake waters, which become relatively dilute, flood most spring vents. Much of the aqueous Ca2+ then precipitates as lacustrine stromatolites on shallow firm substrates, including submerged older travertines. Optimal conditions for subaerial travertine precipitation at Loburu occur when the lake is at intermediate levels, and may be favoured during transitions from humid to drier conditions.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01348.x" xmlns="http://purl.org/rss/1.0/"><title>Evidence for a transgressive barrier within a regressive strandplain system: Implications for complex coastal response to environmental change</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01348.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Evidence for a transgressive barrier within a regressive strandplain system: Implications for complex coastal response to environmental change</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">CHRISTOPHER J. HEIN, DUNCAN M. FitzGERALD, WILLIAM J. CLEARY, MARCIO B. ALBERNAZ, JOAO THADEU 
            De MENEZES, ANTONIO H. da F. KLEIN</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-09-03T10:43:33.34985-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01348.x</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/">10.1111/j.1365-3091.2012.01348.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01348.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">469</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">502</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>Clastic, depositional strandplain systems have the potential to record changes in the primary drivers of coastal evolution: climate, sea-level, and the frequency of major meteorological and oceanographic events. This study seeks to use one such record from a southern Brazilian strandplain to highlight the potentially-complex nature of coastal sedimentological response to small changes in these drivers. Following a 2 to 4 m highstand at <em>ca</em> 5·8 ka in southern Brazil, falling sea-level reworked shelf sediment onshore, forcing coastal progradation, smoothing the irregular coastline and forming the 5 km wide Pinheira Strandplain, composed of <em>ca</em> 500 successive beach and dune ridges. Sediment cores, grab samples and &gt;11 km of ground-penetrating radar profiles reveal that the strandplain sequence is composed of well-sorted, fine to very-fine quartz sand. Since the mid-Holocene highstand, the shoreline prograded at a rate of <em>ca</em> 1 to 2 m yr<sup>−1</sup> through the deposition of a 4 to 6 m thick shoreface unit; a 1 to 3 m thick foreshore unit containing ubiquitous ridge and runnel facies; and an uppermost beach and foredune unit. However, the discovery of a linear, 100 m wide barrier ridge with associated washover units, a 3 to 4 m deep lagoon and 250 m wide tidal inlet within the strandplain sequence reveals a period of shoreline transgression at 3·3 to 2·8 ka during the otherwise regressive developmental history of the plain. The protected nature of Pinheira largely buffered it from changes in precipitation patterns, wave energy and fluvial sediment supply during the time of its formation. However, multiple lines of evidence indicate that a change in the rate of relative sea-level fall, probably due to either steric or ice-volume effects, may have affected this coastline. Thus, whereas these other potential drivers cannot be fully discounted, this study provides insights into the complexity of decadal-scale to millennial-scale coastal response to likely variability in sea-level change rates.</p></div>
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Clastic, depositional strandplain systems have the potential to record changes in the primary drivers of coastal evolution: climate, sea-level, and the frequency of major meteorological and oceanographic events. This study seeks to use one such record from a southern Brazilian strandplain to highlight the potentially-complex nature of coastal sedimentological response to small changes in these drivers. Following a 2 to 4 m highstand at ca 5·8 ka in southern Brazil, falling sea-level reworked shelf sediment onshore, forcing coastal progradation, smoothing the irregular coastline and forming the 5 km wide Pinheira Strandplain, composed of ca 500 successive beach and dune ridges. Sediment cores, grab samples and &gt;11 km of ground-penetrating radar profiles reveal that the strandplain sequence is composed of well-sorted, fine to very-fine quartz sand. Since the mid-Holocene highstand, the shoreline prograded at a rate of ca 1 to 2 m yr−1 through the deposition of a 4 to 6 m thick shoreface unit; a 1 to 3 m thick foreshore unit containing ubiquitous ridge and runnel facies; and an uppermost beach and foredune unit. However, the discovery of a linear, 100 m wide barrier ridge with associated washover units, a 3 to 4 m deep lagoon and 250 m wide tidal inlet within the strandplain sequence reveals a period of shoreline transgression at 3·3 to 2·8 ka during the otherwise regressive developmental history of the plain. The protected nature of Pinheira largely buffered it from changes in precipitation patterns, wave energy and fluvial sediment supply during the time of its formation. However, multiple lines of evidence indicate that a change in the rate of relative sea-level fall, probably due to either steric or ice-volume effects, may have affected this coastline. Thus, whereas these other potential drivers cannot be fully discounted, this study provides insights into the complexity of decadal-scale to millennial-scale coastal response to likely variability in sea-level change rates.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01349.x" xmlns="http://purl.org/rss/1.0/"><title>Quaternary coastal lithofacies, sequence development and stratigraphy in a passive margin setting, North Carolina and Virginia, USA</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01349.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Quaternary coastal lithofacies, sequence development and stratigraphy in a passive margin setting, North Carolina and Virginia, USA</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">PETER R. PARHAM, STANLEY R. RIGGS, STEPHEN J. CULVER, DAVID J. MALLINSON, W. JACK RINK, KEVIN BURDETTE</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-11-05T07:08:32.015687-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01349.x</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/">10.1111/j.1365-3091.2012.01349.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01349.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">503</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">547</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>Lithofacies analysis is fundamental to unravelling the succession of depositional environments associated with sea-level fluctuations. These successions and their timing are often poorly understood. This report defines lithofacies encountered within the north-eastern North Carolina and south-eastern Virginia Quaternary section, interprets their depositional environments, presents a model for coastal depositional sequence development in a passive margin setting and uses this understanding to develop the stratigraphy and Quaternary evolutionary history of the region. Data were obtained from numerous drill cores and outcrops. Chronology was based on age estimates acquired using optically stimulated luminescence, amino acid racemization, Uranium series and radiocarbon dating techniques. Geomorphic patterns were identified and interpreted using light detection and ranging imagery. Since lithofacies occurrence, distribution and stratigraphic patterns are different on interfluves than in palaeo-valleys, this study focused on interfluves to obtain a record of highstand sea-level cycles with minimal alteration by fluvial processes during subsequent lowstands. Nine primary lithofacies and four diagenetic facies were identified in outcrops and cores. The uppermost depositional sequence on interfluves exhibits an upward succession from shelly marine lithofacies to tidal estuarine lithofacies and is bounded below by a marine ravinement surface and above by the modern land surface. Older depositional sequences in the subsurface are typically bounded above and below by marine ravinement surfaces. Portions of seven depositional sequences were recognized and interpreted to represent deposition from late middle Pleistocene to present. Erosional processes associated with each successive depositional sequence removed portions of older depositional sequences. The stratigraphic record of the most recent sea-level highstands (Marine Isotope Stage 5a and Marine Isotope Stage 3) is best preserved. Glacio-isostatic adjustment has influenced depositional patterns so that deposits associated with late Quaternary sea-level highstands (Marine Isotope Stages 5c, 5a and 3), which did not reach as high as present sea-level according to equatorial eustatic records, are uplifted and emergent within the study area.</p></div>
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Lithofacies analysis is fundamental to unravelling the succession of depositional environments associated with sea-level fluctuations. These successions and their timing are often poorly understood. This report defines lithofacies encountered within the north-eastern North Carolina and south-eastern Virginia Quaternary section, interprets their depositional environments, presents a model for coastal depositional sequence development in a passive margin setting and uses this understanding to develop the stratigraphy and Quaternary evolutionary history of the region. Data were obtained from numerous drill cores and outcrops. Chronology was based on age estimates acquired using optically stimulated luminescence, amino acid racemization, Uranium series and radiocarbon dating techniques. Geomorphic patterns were identified and interpreted using light detection and ranging imagery. Since lithofacies occurrence, distribution and stratigraphic patterns are different on interfluves than in palaeo-valleys, this study focused on interfluves to obtain a record of highstand sea-level cycles with minimal alteration by fluvial processes during subsequent lowstands. Nine primary lithofacies and four diagenetic facies were identified in outcrops and cores. The uppermost depositional sequence on interfluves exhibits an upward succession from shelly marine lithofacies to tidal estuarine lithofacies and is bounded below by a marine ravinement surface and above by the modern land surface. Older depositional sequences in the subsurface are typically bounded above and below by marine ravinement surfaces. Portions of seven depositional sequences were recognized and interpreted to represent deposition from late middle Pleistocene to present. Erosional processes associated with each successive depositional sequence removed portions of older depositional sequences. The stratigraphic record of the most recent sea-level highstands (Marine Isotope Stage 5a and Marine Isotope Stage 3) is best preserved. Glacio-isostatic adjustment has influenced depositional patterns so that deposits associated with late Quaternary sea-level highstands (Marine Isotope Stages 5c, 5a and 3), which did not reach as high as present sea-level according to equatorial eustatic records, are uplifted and emergent within the study area.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01350.x" xmlns="http://purl.org/rss/1.0/"><title>Pyrite geochemistry in the Toarcian Posidonia Shale of south-west Germany: Evidence for contrasting trace-element patterns of diagenetic and syngenetic pyrites</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01350.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Pyrite geochemistry in the Toarcian Posidonia Shale of south-west Germany: Evidence for contrasting trace-element patterns of diagenetic and syngenetic pyrites</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">ZSOLT A. BERNER, HARALD PUCHELT, THOMAS NÖLTNER, UTZ KRAMAR</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-09-03T10:42:10.268345-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01350.x</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/">10.1111/j.1365-3091.2012.01350.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01350.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">548</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">573</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>Authigenic pyrite grains from a section of the Lower Toarcian Posidonia Shale were analysed for their trace-element contents and sulphur-isotope compositions. The resulting data are used to evaluate the relationship between depositional conditions and pyrite trace-element composition. By using factor analysis, trace-elements in pyrite may be assigned to four groups: (i) heavy metals (including Cu, Ni, Co, Pb, Bi and Tl); (ii) oxyanionic elements (As, Mo and Sb); (iii) elements partitioned in sub-microscopic sphalerite inclusions (Zn and Cd); and (iv) elements related to organic or silicate impurities (Ga and V). Results indicate that trace-element contents in pyrite depend on the site and mechanism of pyrite formation, with characteristic features being observed for diagenetic and syngenetic pyrites. Diagenetic pyrite formed within anoxic sediments generally has a high heavy metals content, and the degree of pyritization of these elements increases with increasing oxygen deficiency, similar to the degree of pyritization of reactive Fe. The highest gradient in the increase of the degree of trace element pyritization with bottom-water oxygenation was found for the elements Ni &lt; Cu &lt; Mo = As &lt; Tl. In contrast, syngenetic pyrite formed within a euxinic water column typically is enriched in As, Mo and Sb, but is low in heavy metals, and the geochemical variation reflects changes in sea water composition.</p></div>
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Authigenic pyrite grains from a section of the Lower Toarcian Posidonia Shale were analysed for their trace-element contents and sulphur-isotope compositions. The resulting data are used to evaluate the relationship between depositional conditions and pyrite trace-element composition. By using factor analysis, trace-elements in pyrite may be assigned to four groups: (i) heavy metals (including Cu, Ni, Co, Pb, Bi and Tl); (ii) oxyanionic elements (As, Mo and Sb); (iii) elements partitioned in sub-microscopic sphalerite inclusions (Zn and Cd); and (iv) elements related to organic or silicate impurities (Ga and V). Results indicate that trace-element contents in pyrite depend on the site and mechanism of pyrite formation, with characteristic features being observed for diagenetic and syngenetic pyrites. Diagenetic pyrite formed within anoxic sediments generally has a high heavy metals content, and the degree of pyritization of these elements increases with increasing oxygen deficiency, similar to the degree of pyritization of reactive Fe. The highest gradient in the increase of the degree of trace element pyritization with bottom-water oxygenation was found for the elements Ni &lt; Cu &lt; Mo = As &lt; Tl. In contrast, syngenetic pyrite formed within a euxinic water column typically is enriched in As, Mo and Sb, but is low in heavy metals, and the geochemical variation reflects changes in sea water composition.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01351.x" xmlns="http://purl.org/rss/1.0/"><title>Deciphering condensed sequences: A case study from the Oxfordian (Upper Jurassic) Dhosa Oolite member of the Kachchh Basin, western India</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01351.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Deciphering condensed sequences: A case study from the Oxfordian (Upper Jurassic) Dhosa Oolite member of the Kachchh Basin, western India</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">MATTHIAS ALBERTI, FRANZ T. FÜRSICH, DHIRENDRA K. PANDEY</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-09-07T06:57:32.225717-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01351.x</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/">10.1111/j.1365-3091.2012.01351.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01351.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">574</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">598</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 large parts of the Kachchh Basin, a Mesozoic rift basin situated in western India, the Oxfordian succession is characterized by strong condensation and several depositional gaps. The top layer of the Early to Middle Oxfordian Dhosa Oolite member, for which the term ‘Dhosa Conglomerate Bed’ is proposed, is an excellent marker horizon. Despite being mostly less than 1 m thick, this unit can be followed for more than 100 km throughout the Kachchh Mainland. A detailed sedimentological analysis has led to a complex model for its formation. Signs of subaerial weathering, including palaeokarst features, suggest at least two phases of emersion of the area. Metre-sized concretionary slabs floating in a fine-grained matrix, together with signs of synsedimentary tectonics, point to a highly active fault system causing recurrent earthquakes in the basin. The model takes into account information from outcrops outside the Kachchh Mainland and thereby considerably refines the current understanding of the basin history during the Late Jurassic. Large fault systems and possibly the so-called Median High uplift separated the basin into several sub-basins. The main reason for condensation in the Oxfordian succession is an inversion that affected large parts of the basin by cutting them off from the sediment supply. The Dhosa Conglomerate Bed is an excellent example, demonstrating the potential of condensed units in reconstructing depositional environments and events that took place during phases of non-deposition. Although condensed sequences occur frequently throughout the sedimentary record, they are particularly common around the Callovian to Oxfordian transition. A series of models has been proposed to explain these almost worldwide occurrences, ranging from eustatic sea-level highstands to glacial phases connected with regressions. The succession of the Kachchh Basin shows almost stable conditions across this boundary with only a slight fall in relative sea-level, reaching its minimum not before the late Early Oxfordian.</p></div>
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In large parts of the Kachchh Basin, a Mesozoic rift basin situated in western India, the Oxfordian succession is characterized by strong condensation and several depositional gaps. The top layer of the Early to Middle Oxfordian Dhosa Oolite member, for which the term ‘Dhosa Conglomerate Bed’ is proposed, is an excellent marker horizon. Despite being mostly less than 1 m thick, this unit can be followed for more than 100 km throughout the Kachchh Mainland. A detailed sedimentological analysis has led to a complex model for its formation. Signs of subaerial weathering, including palaeokarst features, suggest at least two phases of emersion of the area. Metre-sized concretionary slabs floating in a fine-grained matrix, together with signs of synsedimentary tectonics, point to a highly active fault system causing recurrent earthquakes in the basin. The model takes into account information from outcrops outside the Kachchh Mainland and thereby considerably refines the current understanding of the basin history during the Late Jurassic. Large fault systems and possibly the so-called Median High uplift separated the basin into several sub-basins. The main reason for condensation in the Oxfordian succession is an inversion that affected large parts of the basin by cutting them off from the sediment supply. The Dhosa Conglomerate Bed is an excellent example, demonstrating the potential of condensed units in reconstructing depositional environments and events that took place during phases of non-deposition. Although condensed sequences occur frequently throughout the sedimentary record, they are particularly common around the Callovian to Oxfordian transition. A series of models has been proposed to explain these almost worldwide occurrences, ranging from eustatic sea-level highstands to glacial phases connected with regressions. The succession of the Kachchh Basin shows almost stable conditions across this boundary with only a slight fall in relative sea-level, reaching its minimum not before the late Early Oxfordian.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01352.x" xmlns="http://purl.org/rss/1.0/"><title>From non-tidal shelf to tide-dominated strait: The Miocene Bonifacio Basin, Southern Corsica</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01352.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">From non-tidal shelf to tide-dominated strait: The Miocene Bonifacio Basin, Southern Corsica</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">JEAN-YVES REYNAUD, MICHELLE FERRANDINI, JEAN FERRANDINI, MIGUEL SANTIAGO, ISABELLE THINON, JEAN-PIERRE ANDRÉ, YVES BARTHET, POL GUENNOC, BERNADETTE TESSIER</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-10-01T06:29:22.696083-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01352.x</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/">10.1111/j.1365-3091.2012.01352.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01352.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">599</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">623</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 documents a change from a non-tidal to tide-dominated shelf system that occurred between Corsica and Sardinia (the Bonifacio Basin, Western Mediterranean) during the early to middle Miocene. The non-tidal deposits formed on a low-energy siliciclastic shelf surrounded by progradational coralline algal ramps at full highstand. The tidal deposits consist of an up to 200 m thick succession of siliciclastic to coralline-rich cross-beds formed by large sub-tidal dunes. Based on outcrop and sub-surface data, it is possible to conclude that the tidal currents were amplified as a consequence of the rapid subsidence of the basin centre due to tectonic activity. It is suggested that this tectonic event initiated the strait between Corsica and Sardinia. The strait was deep enough to allow the tidal flux to be significantly increased, generating a localized strong tidal current at the junction between the Western Mediterranean and the East Corsica Basin.</p></div>
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This study documents a change from a non-tidal to tide-dominated shelf system that occurred between Corsica and Sardinia (the Bonifacio Basin, Western Mediterranean) during the early to middle Miocene. The non-tidal deposits formed on a low-energy siliciclastic shelf surrounded by progradational coralline algal ramps at full highstand. The tidal deposits consist of an up to 200 m thick succession of siliciclastic to coralline-rich cross-beds formed by large sub-tidal dunes. Based on outcrop and sub-surface data, it is possible to conclude that the tidal currents were amplified as a consequence of the rapid subsidence of the basin centre due to tectonic activity. It is suggested that this tectonic event initiated the strait between Corsica and Sardinia. The strait was deep enough to allow the tidal flux to be significantly increased, generating a localized strong tidal current at the junction between the Western Mediterranean and the East Corsica Basin.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01363.x" xmlns="http://purl.org/rss/1.0/"><title>Discussion: “Were the Ediacaran siliciclastics of South Australia coastal or deep marine?” by Retallack et al., Sedimentology, 59, 1208–1236</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01363.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Discussion: “Were the Ediacaran siliciclastics of South Australia coastal or deep marine?” by Retallack et al., Sedimentology, 59, 1208–1236</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">RICHARD H. T. CALLOW, MARTIN D. BRASIER, DUNCAN MCILROY</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-10-01T06:56:22.391068-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01363.x</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/">10.1111/j.1365-3091.2012.01363.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01363.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">624</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">627</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=10.1111%2Fj.1365-3091.2012.01362.x" xmlns="http://purl.org/rss/1.0/"><title>Reply to the Discussion by Callow et al. on “Were the Ediacaran siliciclastics of South Australia coastal or deep marine?” by Gregory J. Retallack, Sedimentology, 59, 1208–1236</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01362.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Reply to the Discussion by Callow et al. on “Were the Ediacaran siliciclastics of South Australia coastal or deep marine?” by Gregory J. Retallack, Sedimentology, 59, 1208–1236</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">GREGORY J. RETALLACK</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-10-01T06:56:18.891843-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01362.x</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/">10.1111/j.1365-3091.2012.01362.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01362.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">628</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">630</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=10.1111%2Fj.1365-3091.2012.01360.x" xmlns="http://purl.org/rss/1.0/"><title> Corrigendum: Strange bedfellows: glacial diamictite and cap carbonate from the Marinoan (635 Ma) glaciation in Namibia</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01360.x</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/"> Corrigendum: Strange bedfellows: glacial diamictite and cap carbonate from the Marinoan (635 Ma) glaciation in Namibia</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/">PAUL F. HOFFMAN</dc:creator><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2012-10-22T08:10:29.4727-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/j.1365-3091.2012.01360.x</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/">10.1111/j.1365-3091.2012.01360.x</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fj.1365-3091.2012.01360.x</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">631</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">634</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>Tectonic fold tests conducted in Namibia demonstrate that the inclination with respect to bedding of geoplumb (palaeovertical) tubular structures in the Marinoan (635 Ma) syndeglacial cap dolostone is mainly the result of tectonic strain. Therefore, tubestone inclination data cannot be used to estimate the gradient of the sea floor on the foreslope of the Otavi carbonate platform during the Marinoan glaciation. A gradient steeper than 0·1 (slope angle <em>ca</em> 5·7°), implying a glacial base-level fall ≥0·5 km, is nevertheless supported by boulder-size intraclast debrite in the falling-stand wedge directly beneath the glacigenic sequence. Cryogenian oceans lacked skeletal carbonate production, raising the carbonate saturation state and persistent deep water anoxia excluded acid-producing aerobic respiration, facilitating early diagenetic carbonate precipitation, lithification and steep submarine slopes.</p></div>
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Tectonic fold tests conducted in Namibia demonstrate that the inclination with respect to bedding of geoplumb (palaeovertical) tubular structures in the Marinoan (635 Ma) syndeglacial cap dolostone is mainly the result of tectonic strain. Therefore, tubestone inclination data cannot be used to estimate the gradient of the sea floor on the foreslope of the Otavi carbonate platform during the Marinoan glaciation. A gradient steeper than 0·1 (slope angle ca 5·7°), implying a glacial base-level fall ≥0·5 km, is nevertheless supported by boulder-size intraclast debrite in the falling-stand wedge directly beneath the glacigenic sequence. Cryogenian oceans lacked skeletal carbonate production, raising the carbonate saturation state and persistent deep water anoxia excluded acid-producing aerobic respiration, facilitating early diagenetic carbonate precipitation, lithification and steep submarine slopes.
</description></item><item rdf:about="http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12034" xmlns="http://purl.org/rss/1.0/"><title>Erratum</title><link>http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12034</link><dc:title xmlns:dc="http://purl.org/dc/elements/1.1/">Erratum</dc:title><dc:creator xmlns:dc="http://purl.org/dc/elements/1.1/"/><dc:date xmlns:dc="http://purl.org/dc/elements/1.1/">2013-01-30T09:03:17.759975-05:00</dc:date><dc:identifier xmlns:dc="http://purl.org/dc/elements/1.1/">doi:10.1111/sed.12034</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/">10.1111/sed.12034</prism:doi><prism:url xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1111%2Fsed.12034</prism:url><prism:startingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">635</prism:startingPage><prism:endingPage xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/">636</prism:endingPage><content:encoded xmlns:content="http://purl.org/rss/1.0/modules/content/"><![CDATA[]]></content:encoded><description/></item></rdf:RDF>