Stable isotope ratios in rainwater and water vapor act as a tracers of the hydrological cycle. The data on stable isotopic composition in rainwater and water vapor are limited due to the lack of observational studies across the Indian subcontinent and over the ocean. These present day observations are important database to deduce the paleo-climatic condition from geological archives. In majority of the cases, isotopic records are translated into physical factors with the present background knowledge where relationships with physical variables are well established. In case of tropical region, the primary controlling factor identified behind the stable isotopic variations is the amount of rainfall. However recent observations contradict such relationships challenging the role of amount effect and identified source moisture effect on stable isotope ratios in rainwater at Indian stations. The thesis investigated the amount effect relationship of isotopes at seasonal time scales. The long period observation covering 4 years, where daily time interval rainwater samples collected were used for our study. We used two different station locations; Thiruvananthapuram and Bangalore, where monsoonal rainfall is received for Southwest and Northeast periods. The role of mesoscale and synoptic convection and rainout along the transport pathways were found responsible for the isotopic variance. The role of moisture source regions, rainout over the advection pathways, high rainfall producing systems such as depression and cyclones, and continental recycling of water on rainwater and water isotopes ratios were major findings of the thesis work which are detailed in the chapters. Upon knowing the atmospheric and oceanic condition at the moisture source region based on satellite data and reanalysis data set we modeled our observations using the governing equations of isotope fractionation and well accepted Rayliegh’s distillation model. The observations on rainwater and water vapor isotope ratios in oceanic region are extremely limited due to difficulties in conducting sampling. Water vapor and rainwater observations over the Southern Ocean during the expedition of 2013 and estimation of the moisture recycling across the latitudes over the oceanic regions is a novel work in this thesis.

Der Antarktische Krill (Euphausia superba) ist eine Schlüsselart des Ökosystems des Südozeans und möglicherwese die biomassereichste Art der Erde. Klimawandelbedingte Lebensraumänderungen, die Expansion der kommerziellen Krillfischerei, sowie sich erholende Bartenwalpopulationen setzen Krillpopulationen jedoch zunehmend unter Druck. Daher besteht ein großer Bedarf, die Auswirkungen dieser verschiedener Stressoren auf Krillpopulationen zu verstehen und vorherzusagen. Dabei helfen Simulationsmodelle, die das Wachstum und die Entwicklung des Krills vorhersagen. Modelle sind vielseitige Instrumente, mit denen sich die Auswirkungen verschiedener Stressoren auf Krill in unterschiedlichen Szenarien bewerten lässt, was sie für Management- und Projektionsstudien besonders nützlich macht. In dieser Arbeit untersuchen wir Möglichkeiten die Robustheit von Modellen zu verbessern, die das Wachstum von Krillindividuen unter verschiedenen Umweltbedingungen vorhersagen. Zunächst haben wir ein bestehendes Wachstumsmodell erweitert, indem wir es um realistischere physiologische Prozesse ergänzt haben, was zu verbesserten Wachstumsvorhersagen führte. Anschließend haben wir in der Vergangenheit publizierte Wachstumsmodelle verglichen, um zu untersuchen, ob die Mechanismen des Krillwachstums verallgemeinerbar sind, da die Modelle für verschiedene Regionen entwickelt und mit unterschiedlichen Daten kalibriert wurden, regelmäßig aber außerhalb dieser Regionen verwendet werden. Diese Information ist wichtig für künftige Simulationsstudien, da eine regionale Spezifität die Modelle in ihrer großskaligen Anwendbarkeit limitieren würde. Die Wachstumsvorhersagen der verschiedenen Modellen bei identischen Inputdaten zeigte dabei, dass die Mechanismen und Wachstumsvorhersagen zwischen den Modellen erheblich variieren. Durch die Identifizierung der Ursachen dieser Modellspezifität, konnten wir das allgemeine Verständnis der Krill-Wachstumsmechanismen verbessern und zu der Entwicklung robusterer Modellen beitragen. Individuenbasierte Modelle ermöglichen die Einbindung vieler Prozesse, wie z. B. Verhalten, was diese Art von Modellen besonders attraktiv macht. Unser mechanistisches Verständnis des Verhaltens von Krill ist jedoch noch begrenzt, und wir haben versucht, dies durch die Analyse eines achtmonatigen Datensatzes über das vertikale Migrationsverhalten des Krills zu verbessern. Die Analysen zeigten, dass das vertikale Migrationsverhalten von Krillschwärmen sehr flexibel ist und wahrscheinlich von mehreren Faktoren wie dem Stadium, der Jahreszeit, den Nahrungsbedingungen und der Anwesenheit von Krillprädatoren bestimmt wird. Diese Studie dient als Grundlage für die Entwicklung von Modellkomponenten, die es erlauben das Krillverhalten in individualbasierte Modelle zu integrieren. Anschließend haben wir das vorhandene Wissen über das Krillverhalten in einem Reviewartikel zusammengefasst und dabei die möglichen Auswirkungen des Klimawandels auf Krillverteilung und das Schwarmverhalten analysiert. Zuletzt haben wir einen Systematic Literature Review durchgeführt, um eine Übersicht von Daten zu erstellen, die für die Modellentwicklung und -parametrisierung genutzt werden können. Auf diese Weise konnten wir Aspekte der Krillökologie identifizieren, für die aktuell besonders wenige Daten existieren, was wertvoll für zukünftige empirische Forschung sein wird. Da die Schließung dieser Datenlücken Zeit brauchen wird, diskutieren wir zudem auch Möglichkeiten zur Modellierung des Krillwachstums trotz bestehender Unsicherheiten. Mit dieser Arbeit leisten wir einen Beitrag zur Entwicklung realistischerer und robusterer individuenbasierter Krill-Wachstumsmodelle.:1. Introduction 2. Article I - The impact of seasonal regulation of metabolism on the life history of Antarctic krill (Euphausia superba) 3. Article II - An intercomparison of models predicting growth of Antarctic krill (Euphausia superba): the importance of recognizing model specificity 4. Article III - An open and lightweight method to analyze the vertical distribution of pelagic organisms using echogram screenshots 5. Article IV - Plasticity and seasonality of the vertical migratory behaviour of Antarctic krill using acoustic data from fishing vessels 6. Article V - Impacts of climate change on krill behaviour and population dynamics 7. Article VI - Mapping the data landscape for developing and parameterizing Antarctic krill models 8. Supervised Research Projects 9. Discussion 10. Literature cited in Introduction and Discussion 11. Appendices

VILLELA, FRANCO N. J. Análise decadal do fluxo de CO2 entre o oceano e a atmosfera na passagem de Drake, Oceano Austral. 2011. 148 f. Dissertação (mestrado) Programa de Pós-Graduação em Ciência Ambiental (PROCAM), Universidade de São Paulo, São Paulo, 2011. Para a área delimitada pelos paralelos 60ºS e 62,5ºS e pelos meridianos 60ºW e 65ºW, localizada no sul da Passagem de Drake, no Oceano Austral, próximo à Península Antártica, foram calculadas as distribuições médias de 2000 a 2009, sazonais e anual, do fluxo de CO2 na interface oceano-atmosfera e de suas variáveis associadas: a pressão parcial de CO2 na superfície marinha (PCO2sw), a pressão parcial de CO2 na atmosfera (PCO2ar), a diferença da pressão parcial de CO2 entre o oceano e a atmosfera (PCO2) e a taxa de transferência gasosa (TR), que é produto do coeficiente solubilidade do CO2 na água do mar pela velocidade de transferência gasosa. A parametrização utilizada no cálculo dos fluxos foi a de Takahashi et al. (2009) com TR dependente da velocidade do vento ao quadrado multiplicada por um fator de escala 0,26. A área de estudo tem cerca de 75 mil km2 e foi dividida em uma grade espacial de 0,5º x 0,5º, resultando em 50 quadrículas. Foram utilizados mais de 46 mil medições de PCO2sw, que na média espacial variou de 362,7 ±11,2 a 371,9 ±17,5 µatm, no verão e primavera respectivamente. A PCO2 variou de -0,4 a 5,7 µatm no outono e primavera, respectivamente. A TR variou de 0,065 ±0,04 a 0,088 ±0,002 gC.mês-1.m-2.µatm-1, no verão e inverno, respectivamente. O fluxo líquido, se tomando a concentração de gelo como negligenciável, variou de -0,039 ±0,865 a 0,456 ±1,221 gC.m-2.mês-1, no outono e inverno, respectivamente. O fluxo total anual de carbono, estimado através da média espacial por quadrícula, foi de 95 GgC.ano-1. Dessa maneira, na estimativa anual, a superfície do mar se comporta como fonte de CO2 para a atmosfera, principalmente devido à região da plataforma continental com PCO2sw consideravelmente maior que o da atmosfera. Sazonalmente sugere-se que no verão a maior disponibilidade de radiação solar, a temperatura da superfície do mar (TSM) mais elevada e os ventos mais fracos favorecem a produção de biomassa fitoplanctônica, fazendo com que a bomba biológica seja o processo dominante na diminuição da PCO2sw e na absorção de CO2 atmosférico pela superfície marinha. Já no inverno, os ventos se intensificam e, associados com o forte resfriamento da TSM, promovem a mistura com águas profundas ricas em carbono inorgânico dissolvido, levando a superfície marinha a um estado de supersaturação de CO2 em relação à atmosfera. Ventos circumpolares de oeste mais intensos e deslocados para sul tem sido apontados como a causa do aumento da PCO2sw em igual ou maior taxa do que ocorre na atmosfera. Na área de estudo foi levantada uma tendência média da intensidade do vento de 0,23 ±0,03 m.s-1.década-1 e um aumento na freqüência da componente zonal de oeste (positiva) de 1,47 ± 1,13 % .década-1. Sugere-se que estas tendências estejam relacionadas com o Modo Anular Austral (SAM). Entretanto, a tendência decadal estimada para a PCO2sw foi menor que para a atmosfera, apesar de ambas indicarem tendência de aumento. Acredita-se que a grande variabilidade e distribuição esparsa de dados tenham mascarado a magnitude da estimativa da tendência de PCO2sw. / VILLELA, FRANCO N. J. Decadal analysis of the CO2 sea-air flux in the Drake Passage, Southern Ocean 2011. 148 f. Dissertação (mestrado) Programa de Pós-Graduação em Ciência Ambiental (PROCAM), Universidade de São Paulo, São Paulo, 2011. For the area bounded by parallels 60°S and 62.5°S and meridians 60°W and 65°W, located in the southern Drake Passage in the Southern Ocean, near the Antarctic Peninsula, mean seasonal and annual distributions of CO2 flux at the ocean-atmosphere interface, from 2000 to 2009, have been computed, as well as their associated variables: the CO2 partial pressure at sea surface (PCO2sw), the CO2 partial pressure in atmosphere (PCO2ar), the CO2 pressure difference between ocean and atmosphere (PCO2), and the gas transfer rate (TR), which is the product of the CO2 solubility coefficient in sea water by the gas transfer velocity. The parameterization used to calculate fluxes was that of Takahashi et al. (2009) with TR depending on the squared wind speed multiplied by a scale factor 0.26. The study area has about 75,000 km2 and was divided into a grid of 0.5° x 0.5°, resulting in 50 area boxes. Over 46,000 PCO2sw measurements were used, which in the spatial mean varied from 362.7±11.2 to 371.9±17.5 µatm, in summer and spring, respectively. The PCO2 varied from 0.4 to 5.7 µatm in autumn and spring, respectively. TR varied from 0.065±0.04 to 0,088±0.002 gC.month-1.m-2.µatm-1, in summer and winter, respectively. The net flux, taking ice concentration as negligible, varied from 0.039±0.865 to 0.456±1.221 gC.month-1.m-2, in autumn and winter, respectively. The total annual carbon flux, estimated through the spatial mean per square, was 95 GgC.y-1. Thus, in the annual estimate the region acts as a source to the atmosphere, mainly due to the continental shelf having PCO2sw considerably greater than that of the atmosphere. Seasonally, it is suggested that in summer the greater availability of solar radiation, warmer sea surface temperature (SST), and weaker winds favor the production of phytoplanktonic mass, making the biological pump the dominating process in lowering the PCO2sw and the absorption of atmospheric CO2 by the sea surface. On the other hand, in winter winds intensify and, in association with the strong cooling of the SST, promote mixing with deep waters rich in dissolved inorganic carbon, leading the sea surface to a state of supersaturation in CO2 relative to the atmosphere. Stronger circumpolar west winds and displaced to the south have been pointed as the cause for the increase of PCO2sw at a rate equal to or greater than that occurring in the atmosphere. In the study area it has been detected a mean trend of wind intensity 0.23±0.03 m.s-1.decade-1 and an increase in the western zonal component of 1.47±1.3%.decade-1. It is suggested that these trends are related to the Southern Annular Mode (SAM). However, the decadal trend estimated for the PCO2sw was smaller than for the atmosphere, in spite of both indicating increasing tendencies. It is believed that the great variability and scatter distribution of the data have masked the magnitude of the PCO2SW trend estimate.

Lors du projet Kerguelen Ocean and Plateau compared Study (KEOPS), la dynamique des particules (vitesses de chute, temps de résidence) et les interactions entre dissous et particules (" boundary scavenging ") ont été étudiées afin de mieux comprendre les mécanismes responsables de la fertilisation naturelle en fer observée sur le plateau des Kerguelen. <br />Notre étude utilise deux radionucléides le 230Th et le 231Pa - tous deux produits de désintégration de l'uranium et très réactifs vis-à-vis des particules - comme traceurs de la dynamique des particules.<br />L'étude des vitesses de chute des particules, estimées à partir des distributions de 230Th a montré que, paradoxalement à son fort export de C, le plateau avait des vitesses de chute des particules plus faibles (S= 500 m.an-1) que les stations du large dans les eaux HNLC (S=800 m.an-1). Ce résultat, assez surprenant, soulève une question quant à la limitation du modèle de scavenging 1D dans le cadre de l'étude de la dynamique des particules des systèmes côte-large et suggère l'utilisation d'un modèle 2D pour reproduire le scavenging de ces régions.<br />Sur le plateau, les fortes concentrations de 231Pa dissous suggèrent que du 231Pa a été relâché lors de la dégradation bactérienne d'agrégats, riches en opale (phase pour laquelle le Pa a une forte affinité).<br />Sur l'escarpement à l'Est du plateau, la diminution des concentrations de 230Th et de 231Pa dissous, concomitante à l'augmentation de leur concentration dans les particules, a montré un intense boundary scavenging le long de la pente du plateau, sous l'effet de couches néphéloïdes ou de re-suspension depuis les sédiments, riches en opale.

Du fait de l’isolement géographique de l’océan austral et des conditions météorologiques qui y règnent, la collecte de données océanographiques par les moyens conventionnels est particulièrement couteuse dans cette région du globe. Pour pallier à ces difficultés, l’utilisation d’enregistreurs électroniques embarqués sur des prédateurs marins, et notamment sur les éléphants de mer austraux, s’est révélée être une approche intéressante. Les femelles éléphants de mer s’alimentent en grande partie de petits poissons méso-pélagiques bioluminescents, les myctophidés. Leur forte abondance et leur comportement de migration nycthémérale confèrent à ces organismes un rôle écologique de première importance dans l’océan austral. Cependant, la distribution spatiale des proies de l’éléphant de mer, et les processus physiques et biologiques qui influent sur la dynamique de cette distribution sont encore mal connus. Cette thèse se propose d’enquêter sur ces sujets à partir des données à haute fréquence d’échantillonnage collectées par des femelles éléphants de mer. L’analyse du comportement de plongée des femelles éléphants de mer, en relation avec les variations du taux de rencontre de proie dont les données d’accélération permettent d'avoir une estimation, est au cœur des différents travaux développés dans cette thèse. Les résultats obtenus suggèrent notamment, (1) une diminution de l’abondance des proies avec la profondeur ainsi qu’une homogénéisation de leur distribution, (2) une distribution en couches de cette ressource, (3) l’intervention de contraintes verticales délimitant l’étendue verticale de ces couches et ainsi capable de moduler leur densité, (4) au sein des couches, une dispersion relativement importante des proies en comparaison de la portée des capacités de perception du prédateur, et enfin (5) un rôle significatif des tourbillons méso-échelle et de leur bordure sur la structuration de la distribution des ressources alimentaires de l’éléphant de mer durant l’été austral. / Because of the remoteness and harsh meteorological conditions of the southern ocean, data sampling is more costly in this area. Use of electronic devices attached to marine predators (Bio-logging), such as southern elephant seals, has emerged as an interesting approach to cope with this problem. Female southern elephant seals primarily feed on small bioluminescent meso-pelagic fishes called myctophids. Because of their large abundance and of their diel vertical migration behaviour, these organisms have a major ecological importance in the southern ocean. However, the spatial distribution of the elephant seals prey, as well as the bio-physical processes affecting the dynamics of this distribution, are still poorly known. This thesis intends to investigate this issue using high sampling frequency bio-logging data collected by female southern elephant seals. This work is based on the analysis of elephant seals diving behaviour in relation to changes in the occurrence of prey encounter events detected from acceleration data. Our results suggest that (1) prey abundance decreases with depth and that their distribution tend to standardize, (2) prey are distributed into layers, (3) vertical constraints could modulate the prey density by acting on the vertical spread of these layers, (4) prey items are well dispersed in comparison to the perception range of elephant seals, and finally (5) that meso-scale eddies, notably their edges, play a structuring role in the prey distribution during the austral summer.

La calotte polaire Antarctique conditionne un flux d’eau douce dans l’océan Austral par deux voies d’égale importance : une injection immédiate et localisée par fonte des plateformes glaciaires, et une injection « offshore » et différée par production (« vêlage ») puis fonte d’icebergs. On estime ainsi que les icebergs, en fondant, pourraient modifier les caractéristiques hydrologiques et biogéochimiques de la colonne d’eau. Les modèles numériques visant à estimer cet impact présentent des résultats contrastés. Ils sont limités dans leurs stratégies de représentations des icebergs, notamment parce que les connaissances sur la distribution spatiale et de taille des icebergs ou encore leurs mécanismes de perte de masse sont réduites. Une méthode récente exploitant des mesures par altimétrie satellitaire a permis la création d’une base de données cartographiant la distribution des icebergs Antarctiques avec une couverture spatiale et temporelle inédite. Notre analyse conjointe entre ces données et des champs de concentration en glace de mer met en lumière le transport d’eau douce injecté par les icebergs et son impact sur la banquise. On analyse également les liens entre icebergs de différentes tailles : les gros peuvent être vus comme des réservoirs de volume de glace, qu’ils diffusent dans tout l’océan en se fragmentant en petits icebergs de différentes tailles. On étudie alors l’évolution de deux icebergs géants, on propose une première paramétrisation du phénomène de fracturation et analyse la distribution de taille résultante. Ces résultats peuvent permettre une représentation plus réaliste du flux d'eau douce conditionné par les icebergs dans les modèles. / The Antarctic polar ice cap constrains a freshwater flaux into the Austral Ocean through two equally important pathways : a localized and immediate injection through the melting of ice-shelves bases, and a delayed offshore injection through the calving and subsequent melt of icebergs. Some studies reckon that melting icebergs have the capacity to alter the hydrological and biogeo-chemical characteristics of the water column. The numerical models trying to evaluate this impact have shown contrasting results. Yet, they might suffer from a poor representation of the icebergs, namely due to our limited knowledge on both the spatial and size distributions of the icebergs, or even the processes involved in their mass loss. A new method using satellite altimetry measurements has lead to the creation of a database mapping Antarctic icebergs distribution with an unprecedented spatial and temporal coverage. Our joint analysis between these data and sea ice concentration fields highlights a possible transport of the freshwater injected by an iceberg and its impacts on sea ice.We also analyze the links between icebergs of different sizes : the large ones can be seen as ice buffers that diffuse across the whole ocean when breaking into small fragments of various sizes. We finally study the evolution of two giant icebergs, suggest the first parametrization of the fragmentation process and analyze the subsequent size distribution of the fragments. These results can be valuable to account in a more realistic way the fresh water flux constrained by icebergs in models.

The thesis presents observations on the CO2 concentration and carbon isotopes in air CO2 (δ13C) to constrain the inter-annual variability of carbon inventory over the Southern Ocean between the years 2011-2013. Based on the observation, the region of CO2 venting was identified over the Southern Ocean. Further, isotopic characterization allowed inferring about the possible sources of CO2 degassing and contribution from the dissolved inorganic carbon (DIC) that exsolved to generate CO2. It is concluded that the origin CO2 is mainly from the degassing of CO2 available from the dissociation of DIC or organic degradation. Live Foraminiferal samples of Globigerina bulloides from towing were captured, separated and analysed for δ18O and δ13C from various locations across the Southern Ocean between 10°N−60°S. A large similarities in the estimated values (deduced from simultaneous composition of ocean water 18O, δ13C in DIC and temperature i.e. SST under equilibrium condition) and measured δ18O and δ13C values were observed until 40°S from the equator, and hence it was concluded that the calcification depth of G. bulloides is confined to a depth of ~75-200m till 40°S latitude. However, further south (>40oS) disequilibrium from the estimates was detected. A number of possible reasons were cited for the observed disequilibrium such as (1) Deeper depth habitat (2) Partial dissolution (3) Non-equilibrium calcification (4) Oceanic Suess Effect and (5) Genetic Variability. A box model of isotopic mass balance was presented in this study to explain the pattern of enrichment in the 13C values of sea water DIC with latitude (up to about 43°S). The model shows that a steady state of the carbon isotope ratio of water is achieved in a relatively short time of ~5000 days. Rainwater isotope in the open marine condition across the latitudinal transects over Southern Ocean marking zone of precipitation and evaporation is another element of this thesis. A variation with excess lighter isotopes in rainwater was observed in high latitude rain in this study. Observed isotopic depletion is attributed to rainout process over the ocean. The average rainout fraction over the Southern Ocean in the region of zone of precipitation is ~44%, while it drops to ~25% in the zone of evaporation. Second part of the thesis presents a novel method of isotope thermometry which is called “clumped isotope (13C18O16O16O-2 in the calcite structure) thermometry”. A revision in the thermometry equation relating 47 vs T in synthetic carbonates precipitates and otoliths was proposed. The revised calibration was used on fish otoliths from the modern and past environment to estimate the temperatures. Together with the clumped isotope, conventional stable isotopes in the shell carbonates were measured to effectively reconstruct the seasonal fresh water fraction at seasonal time scales.

L'utilisation des isotopes du silicium (δ30Si) comme proxy paléocéanographique nécessite une bonne connaissance de la répartition et du devenir des isotopes du silicium à travers l'océan. Au cours des dernières années, des efforts considérables ont été faits pour cartographier la composition isotopique du silicium dissous (acide silicique, DSi) et de la silice biogénique (BSi) dans l'océan. Les diatomées utilisent le DSi pour construire leur frustule fait d’opale (BSi). Durant ce processus, les diatomées discriminent l'isotope lourd de silicium (30Si) en faveur de l'isotope léger (28Si). Ce fractionnement conduit à une BSi qui a un δ30Si inférieur de 1,1 ‰ à 1,5 ‰ par rapport au DSi source. Cela se traduit dans les eaux de surface par de faibles concentrations en DSi en raison de l'utilisation biologique et par des valeurs de δ30Si élevées en raison de la distillation de Rayleigh. Inversement, lorsque la BSi se dissout, il y a une discrimination contre l’isotope lourd et ainsi produit du silicium dissous avec un δ30Si inférieur de 0,55 ‰. Dans le même temps, la circulation océanique et le mélange vertical contribuent à modifier le δ30Si du pool de silicium dissous dans la couche de surface, ce qui complique l'utilisation du δ30Si des diatomées comme proxy pour l’utilisation du DSi durant la saison de croissance. Cette thèse vise à mieux comprendre les processus qui régissent le cycle du silicium et la signature en δ30Si des masses d'eau dans les différentes régions de l'océan. De nouvelles données de δ30Si de silicium dissous sont présentées et discutées. Ces données proviennent de 6 profiles CTD de la campagne ANTXXIII/9 (Atlantique et secteur indien de l'océan Austral), 7 profiles CTD de la campagne ANTXXIV/3 (secteur Atlantique de l'océan Austral), et 5 profiles CTD de la campagne MSM10/1 (région subtropical et tropical de l’océan Atlantique nord). Les échantillons ont été purifiés par chromatographie échangeuse d'ions après préconcentration par précipitation de Mg(OH)2, et le silicium est extrait en utilisant du triéthylamine molybdate. Les analyses isotopiques ont été réalisées sur Spectromètre de Masse Multi-Collection à source Plasma (MC-ICP-MS, Naptune) à moyenne résolution (Ifremer, Brest). / Use of silicon isotopes (δ30Si) as a paleoceanographic proxy requires sound knowledge of the distribution and behaviour of silicon isotopes throughout the ocean. Over the past few years considerable effort has been made to map the silicon isotope composition (δ30Si) of silicic acid (dissolved silicon, DSi) and biogenic silica (BSi) throughout the ocean. Diatoms uptake DSi to build up their opal frustules (BSi). During this process, diatoms discriminate against the heavier isotope of silicon (30Si) in favor of the light isotope (28Si). This fractionation leads to BSi that has a lower δ30Si than the DSi source by 1.1 ‰ to 1.5 ‰. In turn, this results in surface waters with low DSi concentrations due to biological removal, and high δ30Si values due to Rayleigh distillation. Conversely, when the BSi dissolves it is with discrimination against the heavier isotope producing dissolved silicon with a δ30Si lower by 0.55 ‰. At the same time, episodes of upwelling occurring throughout the growing season, ocean circulation and mixing, contribute to modify the δ30Si of the dissolved silicon pool in the surface mixed layer, which complicate the use of diatom δ30Si as a proxy for DSi removal during the growing season. This dissertation aims to better understand the processes driving the Si cycle and the δ30Si signature of water masses in different regions of the ocean. New data of δ30Si of dissolved Si are presented and discussed. These data come from 6 CTD profiles from ANTXXIII/9 campaign (Atlantic and Indian sector of the Southern Ocean), 7 CTD profiles from ANTXXIV/3 (Atlantic sector of the Southern Ocean), and 5 CTD profiles from the campaign MSM10/1 (north Subtropical and Tropical Atlantic Ocean). Samples were purified by ion-exchange chromatography following preconcentration via Mg(OH)2 precipitation and extraction of silicon using triethylamine molybdate. Isotopic analyses were carried on a Neptune MC-ICP-MS at medium resolution (Ifremer, Brest).

VILLELA, FRANCO N. J. Análise decadal do fluxo de CO2 entre o oceano e a atmosfera na passagem de Drake, Oceano Austral. 2011. 148 f. Dissertação (mestrado) Programa de Pós-Graduação em Ciência Ambiental (PROCAM), Universidade de São Paulo, São Paulo, 2011. Para a área delimitada pelos paralelos 60ºS e 62,5ºS e pelos meridianos 60ºW e 65ºW, localizada no sul da Passagem de Drake, no Oceano Austral, próximo à Península Antártica, foram calculadas as distribuições médias de 2000 a 2009, sazonais e anual, do fluxo de CO2 na interface oceano-atmosfera e de suas variáveis associadas: a pressão parcial de CO2 na superfície marinha (PCO2sw), a pressão parcial de CO2 na atmosfera (PCO2ar), a diferença da pressão parcial de CO2 entre o oceano e a atmosfera (PCO2) e a taxa de transferência gasosa (TR), que é produto do coeficiente solubilidade do CO2 na água do mar pela velocidade de transferência gasosa. A parametrização utilizada no cálculo dos fluxos foi a de Takahashi et al. (2009) com TR dependente da velocidade do vento ao quadrado multiplicada por um fator de escala 0,26. A área de estudo tem cerca de 75 mil km2 e foi dividida em uma grade espacial de 0,5º x 0,5º, resultando em 50 quadrículas. Foram utilizados mais de 46 mil medições de PCO2sw, que na média espacial variou de 362,7 ±11,2 a 371,9 ±17,5 µatm, no verão e primavera respectivamente. A PCO2 variou de -0,4 a 5,7 µatm no outono e primavera, respectivamente. A TR variou de 0,065 ±0,04 a 0,088 ±0,002 gC.mês-1.m-2.µatm-1, no verão e inverno, respectivamente. O fluxo líquido, se tomando a concentração de gelo como negligenciável, variou de -0,039 ±0,865 a 0,456 ±1,221 gC.m-2.mês-1, no outono e inverno, respectivamente. O fluxo total anual de carbono, estimado através da média espacial por quadrícula, foi de 95 GgC.ano-1. Dessa maneira, na estimativa anual, a superfície do mar se comporta como fonte de CO2 para a atmosfera, principalmente devido à região da plataforma continental com PCO2sw consideravelmente maior que o da atmosfera. Sazonalmente sugere-se que no verão a maior disponibilidade de radiação solar, a temperatura da superfície do mar (TSM) mais elevada e os ventos mais fracos favorecem a produção de biomassa fitoplanctônica, fazendo com que a bomba biológica seja o processo dominante na diminuição da PCO2sw e na absorção de CO2 atmosférico pela superfície marinha. Já no inverno, os ventos se intensificam e, associados com o forte resfriamento da TSM, promovem a mistura com águas profundas ricas em carbono inorgânico dissolvido, levando a superfície marinha a um estado de supersaturação de CO2 em relação à atmosfera. Ventos circumpolares de oeste mais intensos e deslocados para sul tem sido apontados como a causa do aumento da PCO2sw em igual ou maior taxa do que ocorre na atmosfera. Na área de estudo foi levantada uma tendência média da intensidade do vento de 0,23 ±0,03 m.s-1.década-1 e um aumento na freqüência da componente zonal de oeste (positiva) de 1,47 ± 1,13 % .década-1. Sugere-se que estas tendências estejam relacionadas com o Modo Anular Austral (SAM). Entretanto, a tendência decadal estimada para a PCO2sw foi menor que para a atmosfera, apesar de ambas indicarem tendência de aumento. Acredita-se que a grande variabilidade e distribuição esparsa de dados tenham mascarado a magnitude da estimativa da tendência de PCO2sw. / VILLELA, FRANCO N. J. Decadal analysis of the CO2 sea-air flux in the Drake Passage, Southern Ocean 2011. 148 f. Dissertação (mestrado) Programa de Pós-Graduação em Ciência Ambiental (PROCAM), Universidade de São Paulo, São Paulo, 2011. For the area bounded by parallels 60°S and 62.5°S and meridians 60°W and 65°W, located in the southern Drake Passage in the Southern Ocean, near the Antarctic Peninsula, mean seasonal and annual distributions of CO2 flux at the ocean-atmosphere interface, from 2000 to 2009, have been computed, as well as their associated variables: the CO2 partial pressure at sea surface (PCO2sw), the CO2 partial pressure in atmosphere (PCO2ar), the CO2 pressure difference between ocean and atmosphere (PCO2), and the gas transfer rate (TR), which is the product of the CO2 solubility coefficient in sea water by the gas transfer velocity. The parameterization used to calculate fluxes was that of Takahashi et al. (2009) with TR depending on the squared wind speed multiplied by a scale factor 0.26. The study area has about 75,000 km2 and was divided into a grid of 0.5° x 0.5°, resulting in 50 area boxes. Over 46,000 PCO2sw measurements were used, which in the spatial mean varied from 362.7±11.2 to 371.9±17.5 µatm, in summer and spring, respectively. The PCO2 varied from 0.4 to 5.7 µatm in autumn and spring, respectively. TR varied from 0.065±0.04 to 0,088±0.002 gC.month-1.m-2.µatm-1, in summer and winter, respectively. The net flux, taking ice concentration as negligible, varied from 0.039±0.865 to 0.456±1.221 gC.month-1.m-2, in autumn and winter, respectively. The total annual carbon flux, estimated through the spatial mean per square, was 95 GgC.y-1. Thus, in the annual estimate the region acts as a source to the atmosphere, mainly due to the continental shelf having PCO2sw considerably greater than that of the atmosphere. Seasonally, it is suggested that in summer the greater availability of solar radiation, warmer sea surface temperature (SST), and weaker winds favor the production of phytoplanktonic mass, making the biological pump the dominating process in lowering the PCO2sw and the absorption of atmospheric CO2 by the sea surface. On the other hand, in winter winds intensify and, in association with the strong cooling of the SST, promote mixing with deep waters rich in dissolved inorganic carbon, leading the sea surface to a state of supersaturation in CO2 relative to the atmosphere. Stronger circumpolar west winds and displaced to the south have been pointed as the cause for the increase of PCO2sw at a rate equal to or greater than that occurring in the atmosphere. In the study area it has been detected a mean trend of wind intensity 0.23±0.03 m.s-1.decade-1 and an increase in the western zonal component of 1.47±1.3%.decade-1. It is suggested that these trends are related to the Southern Annular Mode (SAM). However, the decadal trend estimated for the PCO2sw was smaller than for the atmosphere, in spite of both indicating increasing tendencies. It is believed that the great variability and scatter distribution of the data have masked the magnitude of the PCO2SW trend estimate.

Killer whales are the oceans’ apex predator and are known to have important effects on ecosystems. At Subantarctic Marion Island, southern Indian Ocean, they have only been studied opportunistically, resulting in limited knowledge of their ecosystem impact here. This dissertation describes the prey and seasonal abundance, estimates the population size and assesses the predatory impact of killer whales on seals and penguins at Marion Island, using dedicated and opportunistic shore-based observations and photographic identification, from 2006 to 2009. During 823 sightings of killer whales at Marion Island (2006 to 2009) 48 predation events were recorded; in only 10 cases could prey be identified. Killer whales fed on fur seals, elephant seals and penguins. Constant effort (dedicated) observations (259 hours, 2008 to 2009) showed that killer whale abundance, which peaked in September to December with a secondary peak in April to May, is linked to the abundance of seals and penguins. Mark-recapture analyses were performed using nearly 10 000 photographs taken from 2006 to 2009. Following careful quality control criteria 37 individuals were identified and a population size of 42 (95% CI = 35-50) individuals estimated using the open population POPAN parameterization in the software program MARK. The analytical approach is more rigorous than that used in any previous population size assessment at Marion Island. Finally, the above data were integrated to assess whether top-down control of seal and penguin populations at Marion Island is generally plausible using a simple process of elimination. Based on published data I predicted the energetic ingestion requirements of adult male and female killer whales as 1 394 MJ.day-1 and 1 028 MJ.day-1, respectively. Expanding these requirements to the 37 killer whales photographically identified at Marion Island, the population requires 40 600MJ.day-1. Based on available energy density and mass data, I predicted the energy content of available seal and penguin prey and calculated the rates at which killer whales would consume these prey in various scenarios. Penguins and Subantarctic fur seals are relatively insensitive to killer whale predation owing to their large population sizes (10 000s to 100 000s), conversely, the smaller populations (100s to 1 000s) of Antarctic fur seals and southern elephant seals are sensitive to predation, particularly the latter as they have a high energy content (approximately 2 000 to 9 000 MJ). Populations of these seals are currently increasing or stable and I conclude that presently killer whale predation is not driving population declines, although they clearly have the potential for regulation of these smaller populations. Thus, if population sizes were reduced by bottom-up processes, if killer whale diet shifted, or if prey availability changed, top-down control by killer whales could become significant. This study provides baseline information for the informed management and conservation of killer whales at Marion Island, identifies avenues for further research, and provides a foundation for the continuation of structured and dedicated killer whale research at Marion Island. / Dissertation (MSc)--University of Pretoria, 2011. / Zoology and Entomology / unrestricted