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O oceano desempenha papel fundamental na configuração e manutenção do clima da Terra, sendo considerado um dos componentes principais do sistema climático.Diversos estudo foram conduzidos para avaliar as mudanças nos processos climáticos e como o clima, em contrapartida, é afetado por tais mudanças. O presente trabalho visa investigar o impacto das mudanças climáticas na formação de massas de água do oceano austral. Foram analisados resultados de simulação numérica para os séculos XX e XXI pelo modelo CCSM3 para os cenários 20c3m e SRESA1B do IPCC. Através da técnica de separação de mássas de água Análise Otimizada de Parâmetros Múltiplos (OMP) foram identificadas 3 massas de água no Mar de Ross: Água Profunda Circumpolar (CDW); Água da Plataforma de Gelo (ISW); Água de Plataforma de Baixa Salinidade (LSSW). A ISW, precursora da Água de Fundo Antártica (AABW), apresenta maior variação espacial tornando-se mais rasa no século XX e assumindo camadas mais profundas no século XXI. A variação da ISW está relacionada à variação do Modo Anular Sul (SAM) e à variação do gelo marinho. / It has been known for a long time that the ocean plays the most important role on Earth\'s heat budget, what turns it into a major component of the global climate system. Therefore, many studies have been made to assess whether features of climate processes are changing and how may climate itself be affected by these changes. This work aims to look at the impact of climate changes on water masses formation in the Southern Ocean. Results from the 20th century and SRESA1b CCSM3/NCAR simulation (1870 to 2100) were analyzed using the Optimum Multiparameter Analysis (OMP) to separate water masses. Three water masses were identified in the Ross Sea: Circumpolar Deep Water (CDW); Ice Shelf Water (ISW); Low Salinity Shelf Water (LSSW). Simulation results have shown that the ISW gets shallower during the 20th century and then, during the 21stcentury, it gets deeper and occupies the deepest layer by 2100 while it flows towards higher latitudes as AABW. Much closely to what has been shown by observational studies, water masses formation in the Southern Ocean is intrinsically linked to atmospheric vaiability modes, such as the southern annular mode--SAM, and to sea ice variation.

A desintegração da plataforma de gelo da enseada Larsen A, em 1995, possibilitou uma oportunidade para estudar a comunidade bêntica da região. Foram analisadas a densidade da macrofauna e a densidade e biomassa da meiofauna. Duas estações na região de mar aberto, no Mar de Weddell, também foram coletadas, para comparações entre diferentes ambientes. Parâmetros ambientais também foram analisados, e serviram para tentar explicar a variação da fauna bêntica. Na região do Mar de Weddell as porcentagens de matéria orgânica foram maiores que na enseada Larsen A, provavelmente um reflexo da maior produtividade primária da área, enquanto as porcentagens de carbonato foram mais altas na enseada do que em mar aberto. A granulometria variou entre silte arenoso a areia síltica, sendo as estações no Mar de Weddell tiveram maiores porcentagens de areia. Em relação à fauna, Nematoda foi o táxon mais abundante, seguido por Copepoda e Nauplii dentro da meiofauna, enquanto Bivalvia e Polychaeta foram os mais abundantes dentro da macrofauna. As maiores densidades de meio- e macrofauna foram encontradas nas estações de mar aberto, e apresentaram correlação com as concentrações de pigmentos. A biomassa total dos nemátodes se correlacionou à biomassa individual do grupo, enquanto a biomassa dos copépodes se correlacionou com a densidade do grupo. Através dos resultados obtidos no presente trabalho foi possível observar que as comunidades bênticas das duas regiões estudadas diferem entre si, em termos de densidade e número de grandes grupos encontrados. E que a disponibilidade de alimento é o principal fator estruturados da fauna na região. / The collapse of the Larsen A ice shelf, in 1995, allowed an opportunity to study the benthic community in the region. The density of macrofauna and the density and biomass of meiofauna were analyzed. Two open water stations in the Weddell Sea were also collected for comparisons between different environments. Environmental parameters were analyzed to look for possible relations with benthic fauna distribution, abundance and biomass. In the Weddell Sea region the percentage of organic matter were higher than in the Larsen A, which was probably a reflection of the higher primary productivity of the area, while the carbonate percentages were higher in the bay than in open water. Particle size ranged from sandy silt to siltic sand, with Weddell Sea stations presenting higher sand content. Nematoda was the most abundant meiofauna taxon, followed by copepods and Nauplii, while Bivalvia and Polychaeta were the most abundant macrofauna. The highest densities of meio- and macrofauna were found in the open sea stations, and were correlated with pigment concentrations. The total nematode biomass was correlated with nematode individual biomass of the group, while copepod biomass correlated with its density. We observed that the benthic communities differed between studied areas in terms of density and taxon richness. Food availability appears to be the main factor structuring fauna in the region.

A desintegração da plataforma de gelo da enseada Larsen A, em 1995, possibilitou uma oportunidade para estudar a comunidade bêntica da região. Foram analisadas a densidade da macrofauna e a densidade e biomassa da meiofauna. Duas estações na região de mar aberto, no Mar de Weddell, também foram coletadas, para comparações entre diferentes ambientes. Parâmetros ambientais também foram analisados, e serviram para tentar explicar a variação da fauna bêntica. Na região do Mar de Weddell as porcentagens de matéria orgânica foram maiores que na enseada Larsen A, provavelmente um reflexo da maior produtividade primária da área, enquanto as porcentagens de carbonato foram mais altas na enseada do que em mar aberto. A granulometria variou entre silte arenoso a areia síltica, sendo as estações no Mar de Weddell tiveram maiores porcentagens de areia. Em relação à fauna, Nematoda foi o táxon mais abundante, seguido por Copepoda e Nauplii dentro da meiofauna, enquanto Bivalvia e Polychaeta foram os mais abundantes dentro da macrofauna. As maiores densidades de meio- e macrofauna foram encontradas nas estações de mar aberto, e apresentaram correlação com as concentrações de pigmentos. A biomassa total dos nemátodes se correlacionou à biomassa individual do grupo, enquanto a biomassa dos copépodes se correlacionou com a densidade do grupo. Através dos resultados obtidos no presente trabalho foi possível observar que as comunidades bênticas das duas regiões estudadas diferem entre si, em termos de densidade e número de grandes grupos encontrados. E que a disponibilidade de alimento é o principal fator estruturados da fauna na região. / The collapse of the Larsen A ice shelf, in 1995, allowed an opportunity to study the benthic community in the region. The density of macrofauna and the density and biomass of meiofauna were analyzed. Two open water stations in the Weddell Sea were also collected for comparisons between different environments. Environmental parameters were analyzed to look for possible relations with benthic fauna distribution, abundance and biomass. In the Weddell Sea region the percentage of organic matter were higher than in the Larsen A, which was probably a reflection of the higher primary productivity of the area, while the carbonate percentages were higher in the bay than in open water. Particle size ranged from sandy silt to siltic sand, with Weddell Sea stations presenting higher sand content. Nematoda was the most abundant meiofauna taxon, followed by copepods and Nauplii, while Bivalvia and Polychaeta were the most abundant macrofauna. The highest densities of meio- and macrofauna were found in the open sea stations, and were correlated with pigment concentrations. The total nematode biomass was correlated with nematode individual biomass of the group, while copepod biomass correlated with its density. We observed that the benthic communities differed between studied areas in terms of density and taxon richness. Food availability appears to be the main factor structuring fauna in the region.

O oceano desempenha papel fundamental na configuração e manutenção do clima da Terra, sendo considerado um dos componentes principais do sistema climático.Diversos estudo foram conduzidos para avaliar as mudanças nos processos climáticos e como o clima, em contrapartida, é afetado por tais mudanças. O presente trabalho visa investigar o impacto das mudanças climáticas na formação de massas de água do oceano austral. Foram analisados resultados de simulação numérica para os séculos XX e XXI pelo modelo CCSM3 para os cenários 20c3m e SRESA1B do IPCC. Através da técnica de separação de mássas de água Análise Otimizada de Parâmetros Múltiplos (OMP) foram identificadas 3 massas de água no Mar de Ross: Água Profunda Circumpolar (CDW); Água da Plataforma de Gelo (ISW); Água de Plataforma de Baixa Salinidade (LSSW). A ISW, precursora da Água de Fundo Antártica (AABW), apresenta maior variação espacial tornando-se mais rasa no século XX e assumindo camadas mais profundas no século XXI. A variação da ISW está relacionada à variação do Modo Anular Sul (SAM) e à variação do gelo marinho. / It has been known for a long time that the ocean plays the most important role on Earth\'s heat budget, what turns it into a major component of the global climate system. Therefore, many studies have been made to assess whether features of climate processes are changing and how may climate itself be affected by these changes. This work aims to look at the impact of climate changes on water masses formation in the Southern Ocean. Results from the 20th century and SRESA1b CCSM3/NCAR simulation (1870 to 2100) were analyzed using the Optimum Multiparameter Analysis (OMP) to separate water masses. Three water masses were identified in the Ross Sea: Circumpolar Deep Water (CDW); Ice Shelf Water (ISW); Low Salinity Shelf Water (LSSW). Simulation results have shown that the ISW gets shallower during the 20th century and then, during the 21stcentury, it gets deeper and occupies the deepest layer by 2100 while it flows towards higher latitudes as AABW. Much closely to what has been shown by observational studies, water masses formation in the Southern Ocean is intrinsically linked to atmospheric vaiability modes, such as the southern annular mode--SAM, and to sea ice variation.

The West Antarctic Ice Sheet is drained primarily by five major ice streams, which together control the volume of ice discharged into the ocean across the grounding line. The grounding line of Kamb Ice Stream (KIS) is unusual because the ice stream upstream of it is stagnant. Here, a set of surface features--shore-parallel, long wavelength, low amplitude undulations--found only at that grounding line are examined and found to be "pinch and swell" features formed by an instability in the viscous deformation of the ice. When a relatively competent layer is surrounded by lower strength materials, particular wavelength features within the layer may be amplified under certain layer thickness and strain rate conditions. The undulations at KIS grounding line are possible due to the relatively large strain rates and particular ice thickness at that location. Several data sets are used to characterize the surface features. High resolution surface profiles are created using kinematic GPS carried on board a sled that was used to tow ice penetrating radar equipment. The radar data are used to examine the relationship between surface shape and basal crevasses. Additional surface profiles are created using ICESat laser altimeter observations. Repeat GPS surveys of a strain grid across the grounding line yields strain rate information. Analysis of repeat observations over tidal cycles and multi-day intervals shows that the features are not standing or traveling waves. Together, these observations are then used to evaluate the contributions of elastic and viscous deformation of the ice in creating the grounding line undulations.

Les questions que se pose le glaciologue peuvent souvent être identifiées à des problèmes inverses. C'est ce qui est illustré dans ce travail à travers trois exemples: * Reconstruction des températures du passé : nous essayons de combiner l'information donnée par la composition isotopique de la glace et le profil de température mesuré à Vostok (Antarctique). Cette approche suggère que le profil de température ne permet pas de donner de meilleure estimation de la température du dernier stade glaciaire à Vostok que le thermomètre isotopique classique. * Reconstruction de la composition de l'atmosphère du passé: lors de la transformation de la neige en glace, des bulles d'air de composition voisine de celle de l'atmosphère sont emprisonnées dans la porosité de la glace. Différents processus naturels peuvent altérer la composition de la bulle et l'interprétation des mesures n'est pas immédiate. Nous proposons ici une méthode de déconvolution du signal atmosphérique prenant en compte les phénomènes de diffusion et de gravitation dans le névé polaire. Nous appliquons ensuite cette méthode à l'interprétation des mesures de méthane, CFCs et rapport isotopique du méthane dans le névé et la glace. * Reconstruction des propriétés rhéologiques de la glace à grande échelle : les iceshelves (plates-formes de glace flottantes) constituent avec les ice-streams (fleuves de glace) les éléments dynamiques de la calotte Antarctique. Leur rhéologie est un paramètre important à prendre en compte pour prédire l'évolution de la géométrie de la calotte Antarctique. Nous montrons comment retrouver ce paramètre critique à partir d'un modèle d'écoulement et de mesures de terrain, puis nous fournissons une carte de viscosité apparente du Ross Ice Shelf (Antarctique de l'Ouest). Les techniques d'inversion décrites dans ce travail sont classiques dans de nombreux domaines de la géophysique, mais elles sont peu connues en glaciologie. En les appliquant sous une forme simplifiée, nous nous sommes efforcés de montrer ce qu'elles peuvent apporter à la glaciologie et quelles sont leurs limites.

Un modèle d'écoulement de la glace est développé en tenant compte du couplage vitesse-température. Ce modèle permet l'étude des réactions d'une calotte polaire aux variations du climat et est appliqués à la ligne de courant "Ridge B - Vostok - Glacier Byrd". (Antarctique de l'Est). Les processus à prendre en compte, les équations de base ainsi qu'une étude bibliographique sont présentés au chapitre (1). Au chapitre (II) dans le but d'interpréter les forages glaciaires, nous développons un outil dans lequel les vitesses d'écoulement sont déduites de la géométrie de la nappe de glace et de l'alimentation par précipitation. A partir du champ de vitesse ainsi calculé, le champ de température est obtenu en résolvant l'équation de la chaleur dépendant du temps avec des conditions aux limites qui tiennent compte de la fusion éventuelle à la base de la calotte de glace ainsi que de la température dans le socle rocheux. Cet outil est utilisé (chapitre III) pour calculer l'âge de la glace dans le carottage de Vostok. Il apparait que la principale incertitude sur la chronologie vient de la mauvaise connaissance de l'accumulation de glace en amont du forage. Le modèle de température permet également d'interpréter le profil de température mesuré à Vostok et d'en tirer des informations sur le flux géothermique et sur l'accumulation. Le modèle thermo-mécanique (chapitre IV) simule l'évolution de l'épaisseur de glace au cours du temps. Les vitesses d'écoulement sont intégrées numériquement et couplées aux température à chaque pas de temps. Un modèle d'ice-shelf est également développé et les déplacements de la ligne d'échouage sont calculés en fonction de la dynamique de la calotte glaciaire et de celle de l'ice-shelf. Des études de sensibilité sont effectuées pour les divers paramètres du modèle. Les variations d'altitude à Vostok pour le dernier cycle climatique sont obtenues et ne dépassent pas 100 m.

The Antarctic ice sheet is increasingly contributing to sea-level rise because of accelerated mass losses at its floating extensions -- its ice shelves. By floating while remaining attached to the grounded ice sheet, ice shelves buttress (i.e. restrain) the inland ice in such a way that ice-shelf losses lead to accelerated ice discharge in the ocean. This thesis investigates the stability of Antarctic ice shelves -- so crucial for the stability of the entire ice sheet -- using the Roi Baudouin Ice Shelf (RBIS), Dronning Maud Land, East Antarctica, as a case study. The RBIS has remained relatively stable over the last millennia and presents various kilometre-scale features (pinning point, ice-shelf channels and englacial lakes) with potential impact on its present and future stability.We first derive a horizontal velocity field, combining interferometry and speckle tracking with Synthetic Aperture Radar images from ERS 1/2 and ALOS-PALSAR, respectively. The resulting velocities and associated shear-strain rates represent the most detailed fields, currently available for the RBIS and clearly resolve small-scale features of the RBIS: significant slow-down and shearing are observed upstream of a small pinning point and ice converges at ice-shelf channels. We then combine our flow field with high-resolution elevations from TanDEM-X to infer the Basal Mass Balance (BMB) of the RBIS. This method relies on mass conservation in a Lagrangian frame and enables us to finely detect spatial variability in the BMB. We show that the BMB of the RBIS varies substantially on sub-kilometre scales. Our technique is promising and could easily be applied more widely.Additionally, the flow field is used to investigate how considering/ignoring small pinning points in observations (geometry and velocities) impacts data initialisation of poorly known parameters (e.g. basal friction, ice viscosity) and subsequent ice-sheet modelling with BISICLES. We find that overlooking the pinning point in the bathymetry leads to erroneous ice-shelf properties whereas accurately capturing the pinning point in velocities is of secondary importance. Finally, before concluding the thesis, we discuss the stability of the RBIS and its neighbouring ice shelves. Most studies agree that the ice shelf has remained stable over the last decades to millennia and would likely remain so in the absence of external forcing. We however point out to three potential triggers of instabilities: (i) large quantities of surface meltwater are formed in the grounding zone and subsequently stored on the ice shelf, thereby providing fuel for hydrofracturing; (ii) ice-shelf channels are found to significantly incise the ice inland and (iii) a bathymetric trough beneath the RBIS forms a potential gateway for warm water intrusions the ice-shelf cavity, which could destabilise the ice shelf from below. We close with a short essay on the importance of outreach, where we argue that public engagement as a scientist should be considered as being part of science and should be valued for its worth. This chapter gives us the opportunity to present outreach activities undertaken in the frame of this thesis. We conclude that, just like ice shelves control Antarctic ice losses, science communication determines transfers of scientific expertise to public knowledge. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Neste trabalho é apresentado um estudo sobre a estrutura vertical e massas d\'água presentes na região oeste e norte da Península Antártica. Foram utilizados dados de temperatura, salinidade e pressão (profundidade) coletados por plataformas de coleta de dados (PCDs) fixadas em elefantes-marinhos do sul (EMS) pelo Projeto MEOP-BR, coordenado pela Profª Dra Mônica M. C. Muelbert, no período de fevereiro a novembro de 2008. Estes dados são transmitidos via sistema de satélites ARGOS a uma taxa de 2.91+/-0.25 vezes ao dia, distância média entre cada perfil coletado é de 14.43 +/- 12.28 km resultando em uma resolução espacial de 41.61 km/dia. Estes dados permitiram uma descrição detalhada da estrutura vertical e identificação de massas d\'água durante diferentes meses do ano de 2008. São comparados perfis verticais em diferentes estações do ano em regiões de plataformas de gelo marinho, do Estreito de Bransfield (EB) e norte da Península Antártica (PA), comparados transectos da porção oeste da PA coletados durante o verão e inverno de 2008 e são apresentados transectos através do Mar da Escócia (ME) nos meses de Setembro a Outubro de 2008. Os valores de temperatura potencial coletados estiveram na faixa entre -1.89ºC e 2.32ºC, os valores mínimos estão relacionados a áreas de formação de gelo marinho e os máximos a investidas através da Corrente Circumpolar Antártica (CCA) em mar aberto e em direção as Ilhas Georgia (IGS). Os valores de salinidade possuem variações entre 32.36 e 35.03 psu, estes valores resultam de diferentes processos, sendo os extremos relacionados a regiões de derretimento e formação de gelo marinho, respectivamente. Graças à grande área utilizada pelos EMS para forrageio durante o x período analisado, diversas massas d\'água são identificadas através de diagramas -S, são elas: Água Profunda Circumpolar (CDW), Água de Inverno (WW), Água de Plataforma de Baixa Salinidade (LSSW), Água Superficial Antártica (AASW), Água de Plataforma de Alta Salinidade (HSSW), Água Profunda Circumpolar Superior e Inferior (UCDW e LCDW), Água de Plataforma (SW), Água de Plataforma de Gelo (ISW), Água Profunda Cálida (WDW) e Água Profunda Cálida Modificada (MWDW). / To study the termohaline structure and water masses in the north and west sides of Antarctic Peninsula, 10 southern elephant seals (EMS) were equipped with highaccuracy conductivity-temperature-depth satellite-relayed data loggers (CTDSRDLs) by the MEOP-BR Project in beginning of 2008 at Elephant Island. Here, we show that measurements collected by these long-ranging, deep-diving predators allow oceanic vertical structure and water masses of the Southern Ocean to be mapped in regions and at times of year not sampled by other oceanographic instruments. These data are transmitted by the ARGOS satellite system at a rate of 2.91+/-0.25 times per day, mean distance between each profile collected is 14.43+/- 12.28 km, resulting in a spatial resolution of 41.61km/day. Vertical profiles are compared at different seasons in sea ice platforms regions, Bransfield Strait (EB) and northern tip of Antarctic Peninsula (PA). Are compared transects at the western side of the PA collected during summer and winter of 2008 and are presented transects across the Scotia Sea (ME) in the months of September and October of 2008. The collected potential temperature values were in the range from -1.89º C to 2.32ºC, the minimum values are related to areas of sea ice formation and the maximum amounts to dives through the Antarctic Circumpolar Current (ACC) in the open sea and towards the South Georgia Islands. The salinity values have variations between 32.36 and 35.03 psu, these values result from different processes, being related to melting and formation of sea ice. The large region sampled allowed us to identify during the study period several water masses from -S diagrams, they are: Circumpolar Deep Water (CDW), Winter Water (WW), Low Salinity Shelf Water xii (LSSW), Antarctic Surface Water (AASW), High Salinity Shelf Water (HSSW), Upper and Bottom Circumpolar Deep Water (UCDW and LCDW), Shelf Water (SW), Ice Shelf Water (ISW), Warm Deep Water (WDW) and Modified Warm Deep Water (MWDW).