Aerosol concentrations in the Southern Hemisphere are largely undersampled. This study presents a chemical and physical description of dust particles collected on board research vessels in the southeast Pacific (SEPS) and the Southern Ocean (SOKS). Concentrations of dust were 6.1 ± 2.4 ng m−3 for SEPS and 13.0 ± 6.3 ng m−3 for SOKS. Dust fluxes, derived from those concentrations, were 9.9 ± 3.7 μg m−2 d−1 for SEPS and 38 ± 14 μg m−2 d−1 for SOKS and are shown to be representative of actual fluxes in those areas. Dust and iron deposition are up to 2 orders of magnitude lower than former predictions. A map of dust deposition on the Southern Hemisphere is proposed by incorporating those in situ measurements into a dust model. This study confirms that dust deposition is not the dominant source of iron to the large high-nutrient low-chlorophyll Southern Ocean.
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 Dust, by affecting marine productivity, the radiative budget of Earth, and precipitation patterns, is a significant and recognized factor in forcing global climate [Jickells et al., 2005]. It has come to be viewed as the main external source of iron for large oceanic areas [Duce and Tindale, 1991; Fung et al., 2000]. Iron limits oceanic productivity in high-nutrient, low-chlorophyll (HNLC) waters [e.g., Martin and Fitzwater, 1988; de Baar et al., 2005; Boyd et al., 2007] and (co)limit nitrogen fixation in some low-nutrient, low-chlorophyll (LNLC) waters [e.g., Mills et al., 2004], thus there has recently been a considerable impetus to understand and estimate dust deposition at the global scale. Dust models [e.g., Luo et al., 2003; Tegen et al., 2002; Ginoux et al., 2004] simulate dust emission, transport, and deposition to calculate dust fluxes on the global scale. Global biogeochemical models have been developed using atmospheric iron derived from those dust models [e.g., Moore et al., 2004; Parekh et al., 2006; Aumont and Bopp, 2006]. To assess the ability of these models in simulating the Earth system, model outputs must be compared against field data. However, collecting aerosols over remote oceanic areas remains a difficult task, mainly because of contamination issues upon sampling [Duce, 1989]. In the Southern Hemisphere, dust deposition is much lower than in the Northern Hemisphere because of the scarcity of continental sources [Mahowald et al., 2005]. For open ocean regions in the southern latitudes, only very limited data are available [Jickells and Spokes, 2001; Witt et al., 2006]. Because of their (micro)nutrient limitation, those areas receiving very low atmospheric deposition are likely to respond strongly to changes in atmospheric deposition [Mahowald et al., 2005].
 Dust deposition is a highly episodic phenomenon, in particular in areas close to important sources [Jickells and Spokes, 2001]. Prospero et al. , using an extensive study of TOMS images, gives a description of global dust sources. Only three important sources are described for the Southern Hemisphere: (1) Australia is the most important source, essentially the Great Artesian basin, although it is noticeably small compared to the aridity of this continent. (2) In southern Africa two small but persistent sources are described close to 20°S, one in Botswana and the other one in Namibia. (3) In South America, two distinct source areas are persistent: the Altiplano in the north and Patagonia in the south.
 This paper focuses on dust deposition in two distinct remote oceanic areas of the Southern Hemisphere that are unexplored regarding in situ aerosols measurements. (1) The Southern Ocean area was sampled south of Kerguelen Island, between 49°S and 54°S. Atmospheric circulation in this area is characterized by persistent and important winds driving air masses from west to east. (2) The southeast Pacific was sampled over a long longitudinal transect. Although aerosols have been extensively sampled/studied in the Pacific during the SEAREX experiment [Duce, 1989], this large province of the South Pacific Ocean has not been explored so far. The main characteristic for southeast Pacific atmospheric circulation is the presence of a permanent anticyclone. The predominate circulation is the anticyclonic winds around this high-pressure system with subtropical easterly winds north of this area and wind fields lying parallel to the South American coast on the eastern side of the basin [Merrill, 1989]. Both studied areas have atmospheric circulation patterns which would tend to preclude them from receiving continental dust.
 The present study aims at (1) describing chemical and physical features of aerosols collected in the southeast Pacific and the Southern Ocean, (2) providing associated dust and iron fluxes, and (3) comparing these fluxes with existing estimations of atmospheric and bottom up iron fluxes within biogeochemical perspectives.
 Aerosol samples were collected during two cruises: (1) The Biogeochemistry and Optics South Pacific Experiment (BIOSOPE) cruise took place along a 8000-km transect through the southeast Pacific from 24 October to 11 December 2004 from Tahiti (French Polynesia) to Concepción (Chile) [Claustre et al., 2008]; during this cruise, seven aerosol samples were collected, labeled from BIO1 to BIO8 (BIO6 missing). (2) The Kerguelen: compared study of the Ocean and the Plateau in Surface water (KEOPS) cruise took place in the Southern Ocean, south of the Kerguelen Island from 10 January to 20 February 2005 [Blain et al., 2007]; during this cruise, six aerosol samples were collected, labeled from K2 to K7. Cruise tracks and sampling areas are presented in Figure 1. Details on sampling schedule are provided as auxiliary material (Table S1).
 Aerosols were collected on four separate 47-mm-diameter filters (two 0.4 μm porosity polycarbonate, Osmonics, and two Teflon 0.5 μm, Zefluor, Pall Corporation) at about 1 m3 h−1 pumping rate. The cumulative amount of pumped air was recorded using volumetric counters. Polycarbonate filters were devoted to particle analyses by transmission electronic microscope (TEM). Teflon filters were devoted to chemical analysis. They were cleaned by filtering 100 mL of a 0.2 mol L–1 dilution of ultrapure hydrochloric acid (Merck Suprapur grade) in Milli-Q water and then rinsed with 200 mL of Milli-Q water. Filters were stored in acid-cleaned Petri dishes.
 Sampling aerosols on board a research vessel obviates contamination from local lithogenic resuspension. However, the main contamination source for aerosol sampling on a ship (in addition to regular activities on board research vessels) is smoke from the engine exhaust stack. Knowing the low dust levels to be encountered in this study, the samples were protected from this possible contamination by (1) collecting only air masses without any mixing with ship exhausts and (2) protecting the samples when collecting was not possible. To do so, a “box” was designed to achieve an integrative sampling during cruise, together with an efficient protection of the samples during intermediary nonsampling periods. The box was attached on the front deck of the ship to a 7-m-high mast during the BIOSOPE campaign and a 2-m-high mast during the KEOPS campaign. Local wind speed and direction were continuously monitored close to the sampling box using a wind vane/anemometer. Depending on the wind conditions, the sampling box operated either in “protection” or “sampling” mode. “Sampling” mode was defined as the period when air was pumped through the filters to collect aerosols. “Protection” mode was defined as the period when pumping through the filters was stopped and clean filtered air (99.99%) was blown with a moderate flow (in order to avoid particle removal) over the filter holders. “Sampling” mode was activated only if wind was oriented in a 120° open angle upwind at a speed higher than 2 m s–1. In addition, the “sampling” mode could not be switched from protected mode before a waiting time of 3 min. The device switched into protected mode or reset waiting time immediately if wind conditions were out of the range defined in sampling mode. Wind conditions were averaged above 1 s. In addition, an optical particle counter (MET-ONE 2400) was continuously recording particle concentrations and numbers were averaged over a 1-min period, whatever the sampling mode conditions. The optical particle counter showed no cut in particulate sizes due to aerodynamic effects when comparing distributions in and out of the sampling device. Particle counts demonstrated the efficiency of the sampling device in the protection mode. Furthermore, during both cruises, a “blank” of the sampler was determined by placing filters for 3 d in the collector switched on “protection” mode.
2.2. Determination of Aluminium Concentration
 A wavelength dispersive X-ray Fluorescence (XRF) spectrometer Phillips PW24004 with a 4kW Rh X-Ray tube was used to perform elemental analyses. XRF is a multielementary method, but only major sea-salt elements and aluminium were above detection limits on the collected samples. Only aluminium (Al) concentrations are presented in this paper. Al was measured on Kα line using a PE002 crystal, 40 kV, and 50 mA electron excitation beam, an angle of 2θ = 144.86° with a background measurement at −1.08° offset. Triplicates (each counting duration = 50 s) were measured and averaged. Calibration filters were performed by depositing 1, 2, and 3–10 μL drops, respectively, of a 1 g L−1 Al solution stock on a polycarbonate membrane. Once dried, the calibration filters were set at the surface of the same type of Teflon Filters as the ones used for the samples to simulate a thin layer deposit. Direct deposition of solution on the Teflon filters gives no reliable results because of the repulsive interactions between Teflon and water. Thin layer measurement conditions have been assumed for both calibration and sample filters. The area of the X-ray beam was smaller than the deposition area of the samples, and the deposition area was different between samples and standards. Therefore a geometric correction had to be performed. The geometric correction factor was inferred from an intercalibration correlation on major sea-salt elements (Na, Ca, and Mg) between XRF measurements and inductively coupled plasma–atomic emission spectrometer (after acid digestion) measurements. The detection limit for the Al analyses was determined by blank dispersion and found to be 5 ng per filter. The relative uncertainty on sample measurements was circa 16%.
2.3. Particle Description and Size Distribution
 The aim of microscopic observations was to describe the collected particles and determine their size distribution, in particular for dust. A transmission electronic microscope (JEOL 100CXII) coupled with a microanalyzer (PGT, dispersion spectrometry of X-Ray Energy, EDX) was used following these analytical conditions: accelerating voltage = 100 kV, tilt angle in the direction of detector = 35°, accumulation time = 60–200 s, and focused beam size = 0.3 μm. The filters were prepared following a protocol adapted from Gaudichet et al. . One-eighth of the sample was cut with a new and clean scalpel. This piece of filter was coated with a carbon layer and directly transferred onto a copper electron microscope grid (diameter: 3.05 mm, 200 mesh of 6400 μm2 each) by dissolving the filter substrate under suction with chloroform. For each grid, 15 squares were observed randomly with TEM. Particles were identified, counted, and analyzed to identify the lithogenic particles. Because of the extremely low numbers of particles detected (often less than five on each sample), observations have been extended to several samples by pooling together the available data. The TEM observations of samples BIO1 to BIO7 were merged together as a representative observation of the southeast Pacific called southeast Pacific sample (SEPS), and the observations of all the samples of the KEOPS cruise were merged together as a representative observation of the Southern Ocean called Southern Ocean–Kerguelen sample (SOKS).
2.4. Other Supporting Data
2.4.1. Ozone Monitoring Instrument Data
 The absorbing aerosol index (A.I.) of the ozone monitoring instrument (OMI) was used as a tool to assess atmospheric dust variability over both sampled areas, in order to better understand how representative the concentration data taken during this cruise was for the seasonal average. A.I. positive values measure absorbing aerosols, such as dust and smoke particles [Herman et al., 1997; Prospero et al., 2002; Ginoux and Torres, 2003]. Inherent problems to the A.I. have been described for the detection of high-latitude or low-altitude aerosols [Herman et al., 1997], which may particularly be a problem for the KEOPS area.
 A.I. values were extracted for each daily gridded data (L3-(NASA/GSFC, Ozone Processing Team, available at http://jwocky.gsfc.nasa.gov/)) during the cruise periods for the corresponding areas (150°W/73°W/37.5°S/8.5°S for SEPS and 68.125°E/78.125°E/53.5°S/48.5°S for SOKS). The A.I. for both investigated areas and period was compared with the complete set of data available from the OMI instrument (September 2004 to September 2006). For SOKS, because of its high-latitude location, wintertime values (April to September) have been eliminated from this study because of probable subpixel cloud problems.
2.4.2. Air Mass Back Trajectories
 Air mass trajectories are commonly used by atmospheric chemists as an approach to determine the potential origin of sampled aerosols. Here, air mass back trajectories have been calculated using the Hybrid Single Particle Lagrangian Integrated trajectory from the NOAA Air Resource Laboratory (HYSPLIT) model [Draxler and Rolph, 2003] with reanalyzed archived meteorological data (FNL).
 Trajectories were calculated at four different heights within the atmospheric boundary layer (10, 100, 500, and 1000 m) up to 120 h back. The trajectory at 10 m was representative of the air at the sampling height during the cruise. The heights of 1000 and 500 m were approximations of the upper limits of the marine boundary layer during the day and at night respectively [Witt et al., 2006]. For SOKS, every 24 h from 10 January 2005 to 20 February 2005, a trajectory was calculated with a finishing point in the center of the area (51.5°S to 73°E). For SEPS cruise (which took place over a broader area), for each sampling day, a trajectory was calculated with a finishing point at the position of the ship at 12 h UTC.
 Moreover, from September 2004 to August 2006, trajectories were calculated up to 240 h back every 24 h for two finishing points at 100 m: (1) in the middle of SOKS area (51.5°S to 73°E) and (2) in the middle of SEPS area (27°S to 263°E). Three simplified dust source areas were defined: Australia (between –15°N/–35°N and 150°E/130°E), South America (between –20°N/–55°N and –55°E/–72°E), and South Africa (between –15°N/–27°N and 15°E/30°E). The frequency of trajectories crossing these three areas was determined at 24-h intervals. It has to be noted that the error on trajectory determination is increasing at each step of the calculation, and thus the error on 10-d trajectories might be important. Nevertheless, they could still give an indication on preferential dust sources to the sampled areas.
2.4.3. Dust Model Data
 Dust model outputs from the model described in detail by Mahowald et al. , Luo et al. , and Mahowald et al.  were used for this study. The dust entrainment and deposition were simulated for four size bins following the Dust Entrainment and Deposition module [Zender et al., 2003]. Transport was simulated by the Model of Atmospheric Transport and Chemistry (MATCH) [Mahowald et al., 1997] using National Center for Environmental Prediction/National Center for Atmospheric Research winds, which are a combination of model and observations [Kistler et al., 2001]. Some systematic discrepancies have been pointed out for this data set in the Southern Hemisphere [Dell' Aquila et al., 2007]. The ability of the model to capture the climatology of dust was examined in detail by Luo et al. , and the interannual and daily variability was examined by Mahowald et al. , Hand et al. , and Luo et al. . The exact same model set up and simulations were extended from those studies into 2005 for comparison to the observations of this paper for the correct days and years. References to the results of the model are referred hereafter as Luo model (Lm).
 Data from global Lm were extracted for our studied areas as follows: (1) for the SEPS area, Lm values were averaged over all pixels corresponding spatially and temporally to the cruise track and (2) for the SOKS area, Lm values were averaged from 49°S/68°W to 54°S/78°W for the months of January and February. For dust concentrations, values were averaged in the first atmospheric layer of the model for the months of the cruises (pressure value: 995 hPa, which corresponds to surface concentration). For dust deposition, climatological values from Lm and from a composite of three dust models [Mahowald et al., 2005] were used.
 In order to provide a new estimate of dust deposition to the open ocean of the Southern Hemisphere, we combined our data with Lm output. Simulations were conducted for the period from March 2004 to March 2005 (with the first month used for spin up) only with the Southern Hemisphere sources (Australia, South Africa, and South America). The minimum of difference between the in situ concentration and the average of the model surface concentration (for SOKS and SEPS) has been optimized using a cost function in order to obtain a correction factor for each source.
3.1. Aluminium Concentrations
 Al concentrations for all collected samples are reported in Table 1. Close to the Chilean coast, Al concentration was 40 times higher than elsewhere in the study region. This value is significantly different from the other concentration values (t test, α = 0.05, υ = 7). The variability (assessed here by the Coefficient of variation, CV) was low between BIO1 to BIO7 (CV = 40%) with regard to the broad area it represents. For KEOPS, the variability between samples was higher (CV = 47%). However, for both areas the variability was low enough to allow to pool together the observations of TEM. Globally, Al concentrations were not significantly different between SEPS (BIO8 not included) and SOKS areas (t test, α = 0.05, υ = 12). Al was under detection limit of the XRF method for the blank filters collected on both cruises.
Table 1. Aluminium Concentrations in the Collected Aerosols for Both Cruises
Southeast Pacific (BIOSOPE-SEPS)
Southern Ocean (KEOPS-SOKS)
Al Concentration, ng m−3
0.30 ± 0.05
1.23 ± 0.19
0.40 ± 0.06
1.75 ± 0.23
0.83 ± 0.12
0.59 ± 0.09
0.45 ± 0.07
0.50 ± 0.08
0.47 ± 0.07
1.23 ± 0.19
0.37 ± 0.06
0.68 ± 0.10
19.0 ± 3.0
Mean (BIO1–BIO7) ± SD
0.47 ± 0.19
Mean ± SD
1.00 ± 0.49
3.2. TEM Observations and Grain Size Distribution of Dust
 For all samples (BIO8 not included), only three types of particles were observed by TEM: (1) the major part of all collected material was “sea-salt” particles, (2) then calcium sulphate (presumably Gypsum), known to originate from marine sources [Andreae et al., 1986], and (3) silicate particles, typical of terrigenous sources, which represented less than 0.1% of the observed particles. Internal mixing of silicate particles with sea salt was observed (Figure 2). Microscopic analysis coupled to microanalysis showed that silicate particles (i.e., dust) contained iron and aluminium (Figure 2). They were the only particles able to transport iron over those remote oceanic areas. No particles were observed with TEM on the “blank” filters.
 Mass size distribution (MSD) for SEPS and SOKS are reported in Figure 3. A monomodal integrated normal distribution was used to fit the data following the method from Dulac et al. . The mass median diameters (MMD) and the geometric standard deviation (σ) were 2.20 μm (σSEPS: 1.36) for SEPS and 2.27 μm (σSOKS: 1.54) for SOKS. Both distributions were not significantly different (t test, α = 0.05, υ = 39).
3.3. Estimated Dust Concentrations and Fluxes
 Dust concentrations (Table 2) were calculated by two independent methods: (1) Al concentration measured by XRF on each aerosol sample was averaged for each cruise; by assuming that Al is only transported by dust (supported by TEM observations) and represents 7.7% in mass of terrigeneous particles [Wedepohl, 1995], a dust concentration was calculated. (2) The size and number of particles transporting iron were determined by TEM observations on a fraction of filter, and those numbers were then extrapolated to the whole filter; by assuming that dust particles had a shape between half-spherical and spherical [Ezat and Dulac, 1995] and a density of 2300 ± 300 kg m−3, a dust concentration was calculated. By using method 1, dust concentrations were 6.1 ± 2.4 ng m−3 for SEPS and 13.0 ± 6.3 ng m−3 for SOKS. By using method 2, dust concentrations were between 3.2 and 7.4 ng m–3 for SEPS and between 6.9 and 15.4 ng m−3 for SOKS.
Table 2. Concentrations of Dust Determined in This Study Compared to Literature Values
 Though only Al concentrations are presented in this manuscript, XRF analysis have clearly pointed out the dominance (>99%) of elements from sea-salt origin on the collected aerosol. Al from sea-salt origin (calculated with a Al/Na ratio in seawater of 9.10−8: Na and Ca concentrations are provided as auxiliary material (Table S2)) represents less than 0.2% of total Al on the filters. This large dominance of sea-salt particles is also supported by TEM observations. However, the estimated dust concentrations from a very small number of particles (less than 0.1% of the observed particles) are reliable because the same numbers were obtained from two independent methods. Such determinations were possible because of the use of this sampling device which excluded local ship contamination and therefore allowed a confidence in the observed particles by TEM.
 Dust fluxes were calculated by summing the dry and wet deposition. Dry deposition was calculated by considering the actual dust concentrations determined by method 1 and a deposition velocity following the 100-step method proposed by [Dulac et al., 1989]. This calculation is based on Slinn and Slinn  deposition model and takes into account the size dispersion of the particles. The mean wind speed used for both cruises was determined from onboard meteorological measurements (BIOSOPE: 6 m s−1; KEOPS: 12 m s−1).
 The daily A.I. given by the Ozone Mapping Instrument (OMI) (NASA/GSFC, Ozone Processing Team, available at http://jwocky.gsfc.nasa.gov/) during the cruises was 0.327 ± 0.075 (n = 35) for SEPS and 0.154 ± 0.080 (n = 38) for SOKS. Those numbers were not significantly different than the mean of available A.I. data from September 2004 to September 2006 presented in Figure 4. No particular “dust event” (A.I. > 0.7) could be identified during both cruises.
3.4.2. Back Trajectories
 Back trajectories at 100-m altitude for both cruises are reported in Figure 5. Only 100-m trajectories are shown as no striking differences were observed between the 10-, 100-, 500-, and 1000-m trajectories. For the KEOPS area, the general east to west circulation is clearly seen (Figure 5a). In the northwestern part of the BIOSOPE area, air masses blowing westward are evident, while in the central part, trajectories are turning around the anticyclone without crossing any continental source; finally, in the southeastern region, close to the Chilean coast, south-north trends are clearly seen (Figure 5b). Only for the last sample (BIO8), trajectories are originating from the South America peninsula (Figure 5b). Frequency of trajectories crossing dust source areas are given in Table 4. For SOKS area, this frequency is extremely low (less than 2%). For SEPS area, no 10-d trajectory is crossing a continental dust source during the 2 years studied.
Table 4. Frequency of Back Trajectories Crossing With Sources in Percent up to 240 h Back Between 1 September 2004 and 31 August 2006 (n = 730)
Back trajectories for an ending point in the middle of SEPS area (−27°N/–107°E).
Back trajectories for an ending point in the middle of SOKS area (−51°N/73°E).
Area of Australian sources defined between −15°N/–35°N and 150°E/130°E.
Area of South American sources defined between −20°N/–55°N and −55°E/–72°E.
Area of South African sources defined between −15°N/–27°N and 15°E/30°E.
4.1. Dust Over Remote Oceanic Areas of the Southern Hemisphere
 Mass size distributions of collected dust particles (Figure 3) show smaller median mass diameters (MMD) compared to other MMD representative of long-range transported dust particles reported in the literature [see, e.g., Maring et al., 2003; Ezat and Dulac, 1995]. According to Tanaka and Chiba , we assume that the Australian desert is the main source of dust for SEPS and the South American desert is the main source for SOKS. Although the source is more distant in the case of SOKS than in the case of SEPS, the grain size distributions of silicates particles collected in both areas are not significantly different. Maring et al.  suggested that, over long-range transport, distance does not significantly play on the size distribution of small mode particles. The MMD reported in this study are the lowest ever reported but, to our knowledge, no study has pointed out a particularly narrow range in the production of dust particles from Southern Hemisphere sources. Therefore, removal of part of small-mode particles over long-range transport cannot be excluded in this study. Although large particles (>10 μm) can be transported over long distances in the North Pacific Ocean [Betzer et al., 1988], none such particles are found in our samples. A plausible explanation is the combination of the paucity of significant sources of particles in the Southern Hemisphere and unfavorable atmospheric circulation for transport to the studied areas.
 No noticeable increase in Al (and dust) is found closer to the Kerguelen Island suggesting that, at least during the KEOPS cruise, the Kerguelen “desert” [as defined by Dulac et al., 2006] is not a significant source of particles for the downwind area. In the southeast Pacific, Al concentrations are rather constant over the whole longitudinal section up to 250 km from the Chilean coast, where an obvious continental imprint is detected. These observations are in agreement with the general atmospheric circulation in that area that precludes the South American continent to be a source of particles to the southeast Pacific. The dust concentrations determined for both areas are in the lowest range among data from the literature (Table 2). The SEPS values are 3 to 20 times lower than dust concentrations determined during the SEAREX experiment on American Samoa and Raratonga Islands (see references in Table 2). Both measurement sites are located west of the SEPS zone and are obviously under a higher influence of the Australian continent. In the Southern Ocean, a clear decreasing latitudinal trend in dust concentrations can be seen as SOKS value is 10 times smaller than levels observed on the Amsterdam Island (situated 15° farther north), but 7 times higher than dust concentration measured on the Antarctic peninsula (see references in Table 2). The dust model (Lm) overestimates concentration values encountered in both studied areas by a factor of 10–50 (Table 2).
 The extremely low dust concentrations presented in this study are in good agreement with the back trajectories calculated. Indeed, the latter demonstrates that the sampled air masses were not prone to enrichment by lithogenic dust as they did not cross a continental area at least during the 5 d preceding the collection. Moreover, the study of back trajectories over 2 years shows that for both sampled areas the frequency of air masses which have crossed a dust source area within 10 d is extremely low, suggesting that both areas receive dust which has been transported over long distances and for more than 10 d. In consequence, the collected dusts are in the lower-scale limit of documented dust particles (regarding both concentration [Jickels and Spokes, 2001] and MSD (C. Zender, Particle size distributions: Theory and application to aerosols, clouds, and soils, 2007, available at http://dust.ess.uci.edu/facts/)).
4.2. Dust/Iron Fluxes to the Southern Hemisphere Ocean
 Dust fluxes calculated in this study are based on samples collected on a small timescale (i.e., duration of the cruises: 1–2 months). This timescale could be too short to integrate sporadic but important inputs of dust. However, several evidences support the representativeness of the calculated dust fluxes. During the 2 years of the OMI data series analyzed, no dust plume is observed over both studied areas, but it has to be pointed out that detection of small dust events could be problematic with OMI in the Southern Ocean [Gasso and Stein, 2007]. However, back trajectories of air masses during the time period of the OMI study also demonstrate that the probability of occurrence of a dust event is extremely low because favorable atmospheric transport does not occur. In the SEPS area, the OMI series illustrate that seasonal variations are very low with a small maximum in austral spring. This trend is confirmed by the in situ time series data collected during the SEAREX program on the Samoa and Rarotonga sites [Prospero et al., 1989]. The frequency of Australian dust storms reaches also a maximum during the austral spring [McTainsh and Lynch, 1996; Mackie et al., 2008]. In the SOKS area, the OMI series is insufficient to assess seasonal variations, because of inherent problems of the A.I. (see section 2). According to the latitude of the SOKS area, this zone receives mainly dust from South American sources which are shown to have their maximum activity during austral summer months [Gaiero et al., 2003]. The precipitation values used to estimate dust deposition are not significantly different from mean values over the period (1979–2005) of the GPCP series. The wet deposition estimates are based on scavenging ratios of dust particles concentration at sea level. A mutual dependence between dry and wet values is inherent to this method and could lead to underestimation of the wet flux because particle concentrations at higher altitudes are not taken into account. Furthermore, seasonal dust deposition variations estimated by climatology from dust models are low in both SEPS and SOKS areas. In consequence, the fluxes proposed here appear to be representative values of longer-term averages. However, for both SEPS and SOKS areas, the sampling was performed during the suspected “high” dust season. Our fluxes could thus tend to slightly overestimate the annual average fluxes.
 In oceanic biogeochemical models which include iron as a micro nutrient, two types of data sets are used for the estimation of dust deposition: (1) fluxes estimated from dust models [see, e.g., Aumont and Bopp, 2006] and (2) fluxes estimated from dust deposition maps (as the one proposed in 1991 by Duce et al. ) and based on the extrapolation of field data.
 Compared to our field data, the dust model overestimates dust deposition by a factor of 10 in the Southern Ocean and by a factor of 30–50 in the southeast Pacific (Table 3). One should bear in mind that there is an important difference in precipitation between the western part and the eastern part of the SEPS area (spatial distribution of precipitation is given in auxiliary material (Figure S1)), which could play on the importance of the wet deposition estimated. However, when using the highest values of precipitation in the western SEPS area from GPCP with a SR of 750, the wet deposition flux would represent 85% of the total flux, which would still be 15 times lower than predicted by the model.
 The fluxes extrapolated from Duce et al.  overestimate from 1 to 12 times our fluxes in the Southern Ocean and from 3 to 30 times in the southeast Pacific (Table 3). This difference between both dust estimations (model and “map”) has been proposed as an important incertitude in former studies of the iron cycle in the Southern Ocean [Ridgwell and Watson, 2002]. The present study shows that for these low dust deposition areas, previously unexplored in regard to atmospheric concentrations, the older estimations based on extrapolation of field data seem to better represent the low-dust areas than dust models. The overestimation of dust fluxes by models in the Southern Hemisphere [Intergovernmental Panel on Climate Change (IPCC), 2001; Luo et al., 2003; Mackie et al., 2008] is clearly confirmed by our calculations in remote oceanic areas of this hemisphere.
Figure 6 shows dust fluxes calculated as the sum of Lm estimated export of dust from the three sources corrected as described in the methods. Australian sources are multiplied by a factor 0.0159, South American sources are multiplied by a factor 0.0400, and South African sources are multiplied by a factor 0.0770. In Table 5, in situ values from the literature are compared with Lm values before and after source correction. A few important points have to be made concerning this new estimation of dust deposition:
Table 5. Comparison Between In Situ Values of the Literature, Model Values (Lm), and Model Values With the Correction (Lm-Cor) Described in This Study (Figure 6)
 1. The Northern Hemisphere sources are not taken into account. Over the largest part of the Southern Hemisphere, these sources are insignificant, but intrusion of northern dust in the Southern Hemisphere has been demonstrated in situ [Krishnamurti et al., 1998] and with models [Luo et al., 2003], which could lead to higher values than estimated in the northern latitudes.
 2. The Australian source has been highly reduced to fit the SEPS data. The new estimation underestimates in situ measurements closer to Australian dust sources than SEPS area (see Tasman Sea, Rarotonga, and American Samoa data in Table 5). This suggests that overestimation of SEPS dust deposition by Lm is not derived from poor estimates of the source but may certainly result from the modeling of dust transport to SEPS area. In fact, SEPS area is not on an important route of dust export from Australia (Table 4), and even if dust would be transported from Australia in direction of SEPS area, the presence of the South Pacific convergence zone, characterized by a belt of precipitation (see auxiliary material (Figure S1)) would play a role of barrier for dust transport.
 3. The South African source is badly constrained with our data, because both studied areas are very slightly impacted by this source.
 4. The new estimation of dust deposition to the Southern Hemisphere presents a good to mitigate agreement with other in situ values in the South Atlantic Ocean (Table 5). As the Lm values are all overestimated for this area, this reinforces the idea that South American sources are overestimated in Lm. Because of the importance of this source for dust deposition on large areas of the Southern Ocean, this correction could have important consequences.
 In summary, even if one should bear in mind that Figure 6 cannot be seen as a “ready to use” product, because of the small data set incorporated, it is a valuable approach to understand global dust deposition over the Southern Hemisphere.
4.3. Consequence upon Biogeochemistry of the Studied Areas
 The respective importance of iron from below (vertical supply from the deep ocean) and above (atmospheric flux) is a key question in order to improve our knowledge of iron biogeochemistry, in particular for HNLC areas [see, e.g., Boyd et al., 2005]. In the estimation of atmospheric dissolved iron (DFe) fluxes, solubility of atmospheric iron in seawater is a major source of uncertainty [Jickells and Spokes, 2001]. Values smaller than 1% have been observed for dust end-members [Bonnet and Guieu, 2004], whereas values of 10% have been suggested more recently for areas remote from dust sources [Baker and Jickells, 2006]. Here, solubility is assumed to range between 1 and 10%. In consequence, the atmospheric fluxes of dissolved iron range between 0.2 and 3.2 nmol m−2 d−1 for SOKS area and between 0.04 and 0.8 nmol m−2 d−1 for SEPS area.
 During the KEOPS cruise, a massive 3 months bloom induced by natural iron fertilization was fueled by “iron from below” [Blain et al., 2007]. Within the area of natural fertilization, the diffusive vertical supply of iron was 31 ± 21 nmol m−2 d−1 (uncertainty estimated from Kz). Outside this area, in the HNLC Southern Ocean, vertical supply of iron was 4 nmol m−2 d−1. This last value is comparable to other estimates in the HNLC Southern Ocean: 6.3 nmol m−2 d−1 [Bowie et al., 2001], 3 nmol m−2 d−1 [Law et al., 2003], 4.1 nmol m−2 d−1 [Croot et al., 2004], and between 10.5 and 21 nmol m−2 d−1 [Croot et al., 2007]. On the basis of all these values, a vertical supply of iron of 5.6 ± 3.0 nmol m−2 d−1 for the HNLC Southern Ocean is assumed. According to our calculation, the atmospheric DFe flux represents only between 0.4% and 16% of the iron input from below in the natural fertilization area and between 3 and 78% outside this area. Thus, atmospheric dust deposition to the Southern Ocean would not have triggered the large Kerguelen bloom observed. Moreover, in the HNLC area, iron from below dominates the iron input. In the modern ocean, the dominance of iron from below by eddy diffusivity has been suggested in sectors of the Southern Ocean [de Baar et al., 1995] and even at the scale of the entire Southern Ocean [Watson, 2001]. A recent study based on remote sensing data analysis in the Atlantic sector of the Southern Ocean argues a control of the biological activity by upwelled iron-rich waters [Meskhidze et al., 2007]. Our data, based on in situ measurements give robust support to this assumption for the HNLC Southern Ocean. The impact of atmospheric deposition on the Southern Ocean productivity is a highly discussed point in particular on the timescale of glacial-interglacial changes [see, e.g., Martin, 1990a; Watson et al., 2000]. Recent studies have investigated the relationship between dust deposition (from models) and marine productivity and some evidences (but not unequivocally) of coupling were pointed out for the whole Southern Ocean [Cassar et al., 2007] and for specific areas close to Australian [Boyd et al., 2004; Gabric et al., 2002] or South American dust sources [Erickson et al., 2003]. For open ocean areas far from dust sources like SOKS area, where dust inputs are not dominating the iron inputs and where the probability of occurrence of a large dust event is low, the demonstration of this coupling is certainly even more difficult.
 One of the main areas of interest of the BIOSOPE cruise was the South Pacific gyre, the most oligotrophic region of the world ocean [Claustre et al., 2008]. South Pacific is largely unexplored and data are scarce. Since the BIOSOPE cruise, vertical distribution of iron has been measured, and profiles show low and uniform dissolved iron concentrations [Blain et al., 2008]. No diffusive supply could thus be inferred from those data to get compared with atmospheric deposition, but the supply of iron from below is likely to be also very low for this area [Blain et al., 2008]. This singularity makes this gyre unique compared to the North Pacific and Atlantic gyres, where atmospheric inputs have been shown to dominate the iron budget [Brown et al., 2005; Jickells, 1999]. In the South Pacific gyre, the primary productivity is primarily controlled by nitrogen and not by DFe availability. Furthermore nitrogen fixation rates measured in this area are extremely reduced and not stimulated by iron additions [Bonnet et al., 2008]. These recent findings are not in agreement with recent oceanic biogeochemical models claiming that nitrogen fixation is driven by iron availability in this area [Moore et al., 2004; Aumont and Bopp, 2006]. This discrepancy could be due to the overestimation of atmospheric iron fluxes by models demonstrated in this study.
 The generally accepted idea that atmospheric deposition is the main source of iron to the open ocean [Duce and Tindale, 1991; Duce et al., 1991; Fung et al., 2000] needs to be critically reevaluated for large areas of the Southern Hemisphere. The overestimation by current dust models raises interesting perspectives for the Southern Hemisphere open ocean:
 According to several models [e.g., Mahowald et al., 1999], dust deposition in the studied areas was 10–50 times higher during the last glacial maximum (LGM) compared to present time. This difference is of the same order of magnitude as the one observed between our in situ observations and current dust models. Furthermore, Latimer and Filippelli  suggest that upwelled iron flux was higher during glacial periods. Dust models should thus be intensely compared with in situ data from a broader range of environments in order to accurately predict differences between present and past dust impact.
 The uncertainty on solubility processes is often proposed as the major source of incertitude in determining atmospheric DFe fluxes [see, e.g., de Baar et al., 2005]. Even if we totally agree on that point, this study shows that the determination of the dust fluxes is the first cause of uncertainty in determining atmospheric DFe fluxes.
 We thank the crew and officers of the French R/Vs Atalante and Marion Dufresnes. We acknowledge Michel Maillé for technical assistance with TEM and Fabrizio D'Ortenzio for his help in data handling. Francois Dulac and Stéphane Blain are acknowledged for their comments. Charlie Zender and one anonymous reviewer are deeply acknowledged for insightful comments on the manuscript. This work was supported by the Institut National des Sciences de l'Univers (INSU) du Centre National de la Recherche Scientifique (CNRS). The NASA-Goddard Space Flight Centre, Ozone Processing Team, provided daily data of OMI Aerosol Index. The NOAA Air Resource Laboratory (ARL) provided the HYSPLIT model. A BDI grant of the Region Provence-Alpes-Cote d'Azur and CNRS supported T.W.