Academic literature on the topic 'Patagonian dust'

Abstract. The supply of bioavailable iron to the high-nitrate low-chlorophyll (HNLC) waters of the Southern Ocean through atmospheric pathways could stimulate phytoplankton blooms and have major implications for the global carbon cycle. In this study, model results and remotely-sensed data are analyzed to examine the horizontal and vertical transport pathways of Patagonian dust and quantify the effect of iron-laden mineral dust deposition on marine biological productivity in the surface waters of the South Atlantic Ocean (SAO). Model simulations for the atmospheric transport and deposition of mineral dust and bioavailable iron are carried out for two large dust outbreaks originated at the source regions of Northern Patagonia during the austral summer of 2009. Model-simulated horizontal and vertical transport pathways of Patagonian dust plumes are in reasonable agreement with remotely-sensed data. Simulations indicate that the synoptic meteorological patterns of high and low pressure systems are largely accountable for dust transport trajectories over the SAO. According to model results and retrievals from the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO), synoptic flows caused by opposing pressure systems (a high pressure system located to the east or north-east of a low pressure system) elevate the South American dust plumes well above the marine boundary layer. Under such conditions, the bulk concentration of mineral dust can quickly be transported around the low pressure system in a clockwise manner, follow the southeasterly advection pathway, and reach the HNLC waters of the SAO and Antarctica in ~3–4 days after emission from the source regions of Northern Patagonia. Two different mechanisms for dust-iron mobilization into a bioavailable form are considered in this study. A global 3-D chemical transport model (GEOS-Chem), implemented with an iron dissolution scheme, is employed to estimate the atmospheric fluxes of soluble iron, while a dust/biota assessment tool (Boyd et al., 2010) is applied to evaluate the amount of bioavailable iron formed through the slow and sustained leaching of dust in the ocean mixed layer. The effect of iron-laden mineral dust supply on surface ocean biomass is investigated by comparing predicted surface chlorophyll-a concentration ([Chl-a]) to remotely-sensed data. As the dust transport episodes examined here represent large summertime outflows of mineral dust from South American continental sources, this study suggests that (1) atmospheric fluxes of mineral dust from Patagonia are not likely to be the major source of bioavailable iron to ocean regions characterized by high primary productivity; (2) even if Patagonian dust plumes may not cause visible algae blooms, they could still influence background [Chl-a] in the South Atlantic sector of the Southern Ocean.

Abstract. The supply of bioavailable iron to the high-nitrate low-chlorophyll (HNLC) waters of the Southern Ocean through atmospheric pathways could stimulate phytoplankton blooms and have major implications for the global carbon cycle. In this study, model results and remotely-sensed data are analyzed to examine the horizontal and vertical transport pathways of Patagonian dust and quantify the effect of iron-laden mineral dust deposition on marine biological productivity in the surface waters of the South Atlantic Ocean (SAO). Model simulations for the atmospheric transport and deposition of mineral dust and bioavailable iron are carried out for two large dust outbreaks originated at the source regions of northern Patagonia during the austral summer of 2009. Model-simulated horizontal and vertical transport pathways of Patagonian dust plumes are in reasonable agreement with remotely-sensed data. Simulations indicate that the synoptic meteorological patterns of high and low pressure systems are largely accountable for dust transport trajectories over the SAO. According to model results and retrievals from the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO), synoptic flows caused by opposing pressure systems (a high pressure system located to the east or north-east of a low pressure system) elevate the South American dust plumes well above the marine boundary layer. Under such conditions, the bulk concentration of mineral dust can quickly be transported around the low pressure system in a clockwise manner, follow the southeasterly advection pathway, and reach the HNLC waters of the SAO and Antarctica in ~3–4 days after emission from the source regions of northern Patagonia. Two different mechanisms for dust-iron mobilization into a bioavailable form are considered in this study. A global 3-D chemical transport model (GEOS-Chem), implemented with an iron dissolution scheme, is employed to estimate the atmospheric fluxes of soluble iron, while a dust/biota assessment tool (Boyd et al., 2010) is applied to evaluate the amount of bioavailable iron formed through the slow and sustained leaching of dust in the ocean mixed layer. The effect of iron-laden mineral dust supply on surface ocean biomass is investigated by comparing predicted surface chlorophyll-a concentration ([Chl-a]) to remotely-sensed data. As the dust transport episodes examined here represent large summertime outflows of mineral dust from South American continental sources, this study suggests that (1) atmospheric fluxes of mineral dust from Patagonia are not likely to be the major source of bioavailable iron to ocean regions characterized by high primary productivity; (2) even if Patagonian dust plumes may not cause visible algae blooms, they could still influence background [Chl-a] in the South Atlantic sector of the Southern Ocean.

Abstract. The effect of Patagonian dust over primary producers in the Southern Ocean has long been disputed. Here we present new remote sensing evidence in favour of dust mediated biological response and postulate a hypothesis to explain the spatial relation observed. A new remote sensing definition of dust source areas based on the Normalized Difference Vegetation Index (NDVI) and Absorbing Aerosol Index (AAI) correlation is presented and interannual variation in AAI is evaluated within the source regions as a proxy for dust activity. Correlation of this data with annual chlorophyll concentration, phytoplankton biomass, and diatom dominance reveals a spatially coherent latitudinal band of positive correlation concentrated between the Polar Front and the Subtropical Front. This pattern is restricted to western areas in the biomass correlation and extends toward Africa for the chlorophyll and diatom correlation. This region is equivalent to the area of the Subantarctic Mode Water formation, characterized by a ratio Si : N ≪ 1 in late summer, an unfavourable condition for diatom development, especially under iron limitation. Therefore, due to Si–Fe co-limitation, the positive correlation could be the consequence of an enhanced sensibility of this area to external iron addition for diatom growth. For the Argentinean shelf-break, is not clear whether direct dust input and/or wind stress driving water masses upwelling could be responsible for the positive correlation.

Abstract. High-resolution records of dust and trace element fluxes were studied in a firn core from the coastal Dronning Maud Land (cDML) in East Antarctica to identify the influence of climate variability on accumulation of these components over the past ~ 50 yr. A doubling of dust deposition was observed since 1985, coinciding with a shift in the Southern Annular Mode (SAM) index to positive values and associated increase in the wind speed. Back-trajectories showed that an increase in dust deposition is associated with the air parcels originating from north-west of the site, possibly indicating its origin from the Patagonian region. Our results suggest that while multiple processes could have influenced the increased dust formation, shift in SAM had a dominant influence on its transport. It is observed that since the 1985s the strength of easterlies increased significantly over the cDML region, which could sink air and dust material to the region that were brought by the westerlies through mass compensation. The correlation between the dust flux and δ18O records further suggest that enhanced dust flux in the firn core occurred during periods of colder atmospheric temperature, which reduced the moisture content and increased dust fall. Interestingly, the timing and amplitude of the insoluble dust peaks matched remarkably well with the fluxes of Ba, Cr, Cu, and Zn confirming that dust was the main carrier/source of atmospheric trace elements to East Antarctica during the recent past.

A travers les époques géologiques, l'océan Austral a joué un rôle majeur dans la régulation du climat à la surface de la Terre et en particulier dans la réduction de la concentration en CO2 atmosphérique. Cette région océanique est la plus importante pompe biologique de carbone et à travers la photosynthèse du phytoplancton permet la séquestration du carbone dans les profondeurs océaniques. Cette diminution aurait été causée par les dépôts de poussières qui par apportant des éléments comme le fer dans les régions limitées en nutriments, fertilise la surface des océans et permet l'activation de la pompe biologique de carbone. Aujourd'hui, l'entrée dans l'ère de l'Anthropocène a été marqué par l'impact que l'activité humaine exerce sur son environnement. L'activité anthropique génère et largue du dioxyde de carbone dans l'atmosphère provoquant un effet de serre sur la Terre altérant l'équilibre environnemental. Cette étude explore l'océan Austral qui est une zone de paradoxe biogéochimique avec de fortes concentrations en macronutriments, mais avec une faible productivité biologique. En 1990, John Martin a élaboré la « Iron Hypothesis » ou le fer (micronutriment) restreint la croissance phytoplanctonique. La poussière est une source majeure de métaux pour l'océan de surface. Dans l'océan Austral, les poussières ont une origine majoritairement d'Amérique du Sud (poussière patagonienne). Les apports d'Amérique du Sud contribuent pour 58% de la poussière totale dans l'océan Austral et seront multipliés par deux avec les futurs changements environnementaux. Pendant le dernier maximum glaciaire dans l'océan Austral, les apports de poussières auraient diminué la concentration en CO2 dans l'atmosphère. A de plus petites échelles de temps, des tests de fertilisation artificielle de fer ont été réalisés dans l'océan Austral et ont montré une forte productivité biologique. L'objectif de ce travail est de mieux caractériser et de quantifier la fraction de métaux qui se solubilise de la poussière patagonienne dans l'eau de mer sous des conditions actuelles et futures (2100) et d'améliorer les prédictions de l'évolution du phytoplancton dans la réponse à l'intensification de l'apport de poussières patagoniennes et des autres changements environnementaux dans l'océan Austral dans le but d'évaluer les impacts sur la production de carbone
Throughout geological time, the Southern Ocean has played a major role in regulating the Earth's surface climate and in particular in the reduction of atmospheric CO2. This oceanic region is the most important biological pump of carbon and through the photosynthesis of phytoplankton allows the sequestration of carbon in the deep ocean. This decrease would have been caused by dust deposits which, by bringing elements such as iron in areas limited in micronutrients, fertilize the ocean surface and allow the activation of the biological carbon pump. Nowadays, the entering into the Anthropocene era has been marked by the impact that human activity has exerted on its environment. Anthropogenic activity that generates the release of carbon dioxide into the atmosphere causes a greenhouse effect on the surface of the Earth and upsets the environmental balance. This study investigates the Southern Ocean which is biogeochemical paradox zone with high concentration of macronutrients but low biological productivity. In 1990 John Martin elaborated the "Iron hypothesis" hence iron (micronutrients) restricts phytoplankton growth. Dust is major source of metals in the surface ocean. In the Southern Ocean, dust have mainly a South America (Patagonian dust) origin. Input from South America contributed to 58% of the total dust into the Southern Ocean and will increase by two fold higher with the future environmental changes. During the last glacial maximal in the Southern Ocean, dust input would have decreased the CO2 concentration in the atmosphere. Moreover, in the small timescale there are tests of artificial iron fertilization performed in Southern Ocean have demonstrated high biological productivity. The overall aim of this work is to better characterize and quantify the fraction of metals that solubilizes from Patagonian dust in seawater under actual and future conditions (2100) and to improve predictions of the phytoplankton evolution in response to intensification of Patagonian dust input and other multi-stressor changes in the Southern Ocean in order to evaluate the impacts on carbon production

Patagonie et la Namibie sont deux sources importantes d'aérosol minéral qui alimente la section Atlantique Sud de l'océan Austral avec les micronutriments.L'objet de ma thèse est d'étudier 1) la concentration atmosphérique et la variation temporel de la poussière en Patagonie, 2) l'hétérogénéité spatiale de composition élémentaire de poussière en Patagonie et en Namibie, et 3) la solubilité élémentaire de poussière en Patagonie et en Namibie. Ces trois aspects sont les principaux enjeux pour modéliser les inventaires des émissions de micronutriments biodisponibles à partir de sources de poussière.La concentration en poussière mesurée en Patagonie montre une variation saisonnière avec un niveau plus bas en hiver. Les données météorologiques suggèrent que cette variation saisonnière est associée à la variation de l'humidité du sol dans les zones source plutôt qu'à la vitesse du vent. Des échantillons d'aérosol minéral ont été générés à partir des sols de Patagonie et de Namibie. La composition élémentaire des poussières diffère de celles des sols parents, en particulier en Namibie en raison de l'effet de dilution par le quartz dans les sols. Des compositions élémentaires varient spatialement aux échelles continentale et régionale en Patagonie et Namibie. Les variations de Ca et Mg sont les principales raisons conduisant à l'hétérogénéité spatiale de la composition élémentaire des poussières. Les solubilités élémentaires des aérosols minéraux de Patagonie et de Namibie augmentent avec l'acidité de la solution altérante. Les poussières riches en calcium présentent une solubilité plus élevée pour les éléments les plus solubles (Ca, etc.) en raison de la présence de carbonate. Le suivi de la concentration en poussières obtenu en Patagonie peut aider à mieux en quantifier les émissions dans la région subantarctique et ainsi à mieux contraindre les modèles. La base de données que nous avons obtenue sur les poussières et leur solubilité contribue également à l'évaluation des émissions d'éléments solubles dans la région Australe
Mineral dust is considered to be an important supplier of micronutrient for the Southern Ocean where the primary production is limited by insufficient supply of micronutrients. Patagonia (South America) and Namibia (Southern Africa) are two main dust sources for the South Atlantic section of the Southern Ocean. Emission inventories of bioavailable micronutrients from these two regions regulate the final biological impact on marine ecosystem in the South Atlantic Ocean. This thesis is mainly focused on the investigation of 1) the atmospheric dust concentration and its temporal pattern in Patagonia, 2) the spatial heterogeneity of dust elemental composition in Patagonia and Namibia, and 3) the pH dependence of elemental solubility in Patagonian and Namibian dust. These three aspects are the key issues to model the emission inventories of bioavailable micronutrients from dust sources. Dust concentration measurements were conducted in Patagonia-Atlantic Coast and revealed a seasonal pattern of dust concentration with lower dust level in winter than the other three seasons. Meteorological records suggest that this seasonal pattern is associated with the variation of soil moisture in source areas rather than the recurrently high wind speed. Dust samples were generated from Patagonian and Namibian soils to investigate the elemental composition and the elemental solubility of source dust. Dust elemental composition differs to different degrees from their parents soils, particularly in Namibia due to the dilution effect of quartz in soil. Spatial variability of dust elemental composition was observed at both continental scale and regional scale in Patagonia and Namibia. Variations in Ca and Mg content are the main reasons for the spatial heterogeneity of dust elemental composition. Elemental solubility of Patagonian and Namibian dust increased with acidity of leaching solution. More soluble elements namely Ca, K, Mg, Mn, Sr and Ba showed much higher solubility in calcium-rich dust due to the presence of carbonate. The dust concentration record obtained in Patagonia may help to better quantify the dust emission in subantarctic region and to constrain dust models. Database of dust elemental composition and elemental solubility in Patagonia and Namibia also contributes to the evaluation of emission inventories of soluble elements from dust sources to the Southern Ocean

Conselho Nacional de Desenvolvimento Científico e Tecnológico
O Oceano Austral é a região oceânica de maior extensão em que os macronutrientes necessários à produção primária permanecem em níveis elevados por todo ano. Essa condição é conhecida como High Nutrient Low Clorophyll (HNLC) e é determinada, em grande parte, pela relativa escassez de micronutrientes, particularmente o ferro. Diversos experimentos comprovaram que a entrada de ferro neste sistema intensifica a produção biológica, aumentando a fixação do carbono e, eventualmente, sua exportação para águas profundas. Este fenômeno recebeu muita atenção nos últimos 20 anos devido a sua possível influencia no clima, via ciclo do carbono. A relação inversa entre concentração de CO2 na atmosfera e o fluxo de poeira mineral observados em registros glaciais da Antártica Central sugere que a deposição atmosférica pode ser uma importante via para o aporte de micronutrientes. Porém, a contribuição da deposição de poeira mineral para a produção primária nesta região permanece para ser demonstrada e seu possível papel no sistema climático ainda não é conclusivo. No caso do setor Atlântico do Oceano Austral, que recebe influência da Patagônia, os baixos fluxos modernos de poeira mineral e a baixa solubilidade do ferro associado à estrutura dos alumíniossilicato levam muitos autores a postular que fontes oceânicas de micronutrientes sejam mais determinantes. Faltam, no entanto, evidências experimentais. Neste trabalho, abordamos o estudo da fertilização do setor Atlântico do Oceano Austral pela poeira da Patagônia utilizando duas ferramentas: (1) o sensoriamento remoto orbital de aerossóis minerais e clorofila-a em escala interanual; e (2) um experimento de fertilização, com poeira da Patagônia, realizado na Passagem de Drake, considerando fluxos estimados para a era moderna e para o último glacial. Após doze dias de bioensaio, os tratamentos de adição de poeira mostraram a elevação da clorofila-a e da abundância de células em níveis acima dos controles. Níveis intermediários e maiores de adição não diferiram entre si na intensidade de resposta biológica, separando-se apenas da menor adição. Esses resultados indicam que a poeira da Patagônia, mesmo nos fluxos atuais, é capaz de prover os micronutrientes escassos na coluna dágua, com potencial para deflagrar aumentos significativos de biomassa. Através da análise por sensoriamento remoto, identificamos uma região de alta correlação entre poeira e clorofila-a, que está localizada entre a Frente Subtropical e a Frente Polar, se estendendo da Argentina ao sul da África. Esta região difere das águas ao sul da Frente Polar pela menor profundidade da camada de mistura, menor concentração de silicatos, baixa biomassa de diatomáceas e, estima-se, maior estresse fisiológico devido à escassez de ferro e menor aporte oceânico deste nutriente. Em conjunto, essas características parecem criar condições que tornam a resposta biológica mais sensível à deposição de poeira mineral. Estes resultados lançam nova luz sobre o controle atual da produção primária na região e sobre a hipótese da regulação climática pelo fitoplâncton no Oceano Austral, mediado pela deposição de poeira da Patagônia.
The Southern Ocean is the larger ocean region where the macronutrients needed for primary production remain in high levels through the year. This condition is known as High Nutrient Low Chlorophyll (HNLC) and is conditioned, largely, by the relative shortage of micronutrients, particularly iron. Several experiments proved that the supply of iron to this system enhances biological production, increasing carbon fixation and, eventually, its exportation to deep waters. This phenomenon received much attention in the last 20 years due to its possible influence in the climate, through carbon cycle. The inverse relationship between the atmospheric CO2 concentration and the mineral dust flux observed on the Central Antarctic glacial records suggest that atmospheric deposition may be an important source for the supply of micronutrients. However, the contribution of mineral dust deposition for the primary production in this region remains to be demonstrated and its possible hole in the climate system its not yet conclusive. In the case of Atlantic Southern Ocean, thats influenced by Patagonia, the low modern flows of mineral dust and the low iron solubility associated with aluminum-silicate structure led many authors to state that oceanic sources of micronutrients are more determinants. However, experimental evidence are lacking. In the present work, we approach the study of fertilization of Atlantic Southern Ocean by Patagonian dust employing two different tools: (1) orbital remote sensing of mineral aerosols and chlorophyll-a on inter-annual scale; and (2) a fertilization experiment with Patagonian dust, carried through in Drake Passage, considering estimated flux for the modern era and for the last glacial. After twelve days of bioassay, the dust addition treatments showed increase on chlorophyll-a and cell abundance beyond controls levels. Intermediary and higher levels of addition didnt differ between each other regarding the intensity of biological response, separating only of the lower addition treatment. These results indicate that even modern Patagonia dust flux is capable of providing micronutrients that are scarce in the water column, with potential to deflagrate a bloom. Through remote sensing analysis we have identified a region with high correlation between dust and chlorophyll-a, thats located between the Subtropical Front and the Polar Front, extending from Argentina to south of Africa. This region differs from waters south of the Polar Front by means of a deeper mixed layer, lower silicate concentrations, low diatom biomass and, is estimated, greater iron physiological stress and lower iron oceanic supply. Together, these properties seem to create conditions to which biological response would be more sensible to dust deposition. These results cast new light over controls on modern primary production in the region and over the phytoplankton climatic regulation in the Southern Ocean, mediated by Patagonian dust deposition.