The existing observations and model simulations indicate that mesoscale eddies and the Eastern Boundary Current (EBC) have a significant role in the complex circulation of the Red Sea. However, a full understanding of the processes that contribute to the physics and biological responses of the central Red Sea (CRS) has been limited due to the lack of sustained in-situ observations. In this dissertation study, in-situ observations extending over a thirty-three month period from spring 2013 through winter 2015 include an intensive ship-based and glider monitoring program to understand the key dynamic features of the CRS circulation. Nine glider missions and five ship-based surveys provide concrete resolution of both spatial and temporal variability in the CRS. The quasicontinuous glider observations resolve the influence of distinct water masses with a different origin that is present in the study area. Our results show that mesoscale eddies and the an intrusion of Gulf of Aden water governs the physical and biochemical characteristics of the CRS during the winter to summer transition period in 2013. During this period, an anticyclonic eddy appears to redirect the northward flow along the eastern boundary. Ship-based observations in fall 2013 indicate that the EBC can periodically transport patches of less salty and warmer water containing higher chlorophyll concentrations from south into the CRS. During spring 2014, ship observations show the presence of a cyclonic/anticyclonic eddy pair. The cyclonic eddy contribute an upward nutrient flux, resulting in an increase integrated chlorophyll concentration within the eddy. Higher chlorophyll and CDOM concentrations and lower N:P ratios characterized the inflow of lower salinity Gulf of Aden water from the south. To understand better how the mesoscale eddy activity, stratification, and the EBC modulate the nutrient availability and planktonic food web architecture in Red Sea two addition hydrographic surveys with plankton sampling were conducted in fall 2014 and spring 2015. The seasonal availability of Gulf of Aden water, stratification and eddies exerted a demonstrable effect on the plankton community by modulating the availability and utilization of allochthonous vs. autochthonous macronutrients by phytoplankton. Strong stratification, higher temperatures and depletion of nutrients by phytoplankton, subjected the plankton community to an overall nitrogen and phosphorus deficit in fall. To evaluate the role of the winter mixing, mesoscale eddies, and EBC within CRS during the winter to spring period, a sustained glider study (~91 days) was initiated from December 2014 to March 2015. Glider observations show the seasonal contrasts and transitions from strong summer stratification to winter mixing, with a corresponding transition from a well defined deep chlorophyll maximum to phytoplankton population intrusions of lower salinity water from the Gulf of Aden contributed to both the physical and biochemical variability within the region. Both GASW and GAIW can be entrained and diverted across the basin by larger eddies. Eddies play a role in the mixing between warmer, fresher water from the Gulf of Aden, and cooler, saltier water from the northern Red Sea.

We use hydrographic and direct velocity observations from two quasi-synoptic cruises in conjunction with a primitive equation linear instability model, to investigate the Brazil Current (BC) downstream change effect between 23°S-30°S on the temporal mixed instabilities properties. The quasi-synoptic data revealed that the BC is ∼400-500 m deep to the north of the so-called Santos Bifurcation (26°S-28°S) and extends down to 1000 m to the south of it. We estimated that the BC receives at least 7 Sv from the Santos Bifurcation, which drastically alters the BC\'s velocity vertical structure and meanders characteristics as it flows poleward. Based on direct velocity measurements, we computed the mixed-instability properties at three different latitudes (24°S, 26°S and 30°S). The instability analysis revealed unstable current systems to mesoscale perturbations with maximum growth rates of 0.12, 0.19 and 0.06 day-1 at 24°S, 26°S and 30°S respectively. The corresponding downstream phase speeds are -0.19, -0.24 and -0.26 m s-1. The analysis of the mean-to-eddy energy conversion terms show that the barotropic instability drains 60-90% less energy from the background state than the baroclinic instability. Nevertheless, the maximum growth rates are at least the double in magnitude when both instabilities occur simultaneously. The topography presents a stabilizing effect for both kind of instabilities along all the BC path. At the vicinities of the Cape Santa Marta (28°S), we explored the the recurrent cyclonic meanders of the BC. Combining a wide range of observations, we provided a overview of such features and the relations between its velocity patterns, the water properties (temperature, salinity, nutrients), chlorophyll-a distribution and the BC variability. The top-bottom quasi-synoptic velocity measurements depicted cyclonic meanders over the continental slope with diameters larger than 100 km and vertically extending to approximately 1500 m depth. Moreover, the observed eddies seems to trap and recirculate a small portion (∼1.5 to 4 Sv) of the BC main flow (-13.16 to -17.89 Sv), which is consisted of Tropical Water (TW), South Atlantic Central Water (SACW), Antarctic Intermediate Water (AAIW) and Upper Circumpolar Deep Water (UCDW). Additionally, we presented observational evidence that the meanders actively influence the transport of nutrient-rich shelf waters to the open ocean enhancing the primary productivity at the photic zone over the continental slope. Satellite imagery show that these cyclonic events occur 5-6 times per year and are generally associated with wave-like perturbations on the flow with mean wavelength of ∼219 km. Finally, Empirical Orthogonal Functions (EOF) analysis computed from an array of mooring lines show that more than half of the along-isobath velocity variance on the continental slope is explained by the BC mesoscale activity. / As propriedades de instabilidade temporal mista da Corrente do Brasil (CB), entre 23°S-30°S, foram investigadas combinando dados hidrográficos e medições diretas de velocide com modelagem numérica. As observações revelaram uma CB com ∼400-500 m de profundidade ao norte da Bifurcação de Santos (26°S-28°S). Em contrapartida, a CB ao sul da bifurcação se mostrou muito mais profunda (> 1000 m) devido ao aporte de aproximadamente 7 Sv de águas em profundidades intermediárias (∼500-1500 m) oriundas do ramo sul da Bifurcação de Santos. Baseado-se nas observações, experimentos numéricos foram conduzidos em três latitudes (24°S, 26°S and 30°S), com o intuito de se estudar as propriedades da instabilidade geofísica da CB. Tais experimentos mostraram que o sistema de correntes é instável para perturbações de mesoescala com taxas de crescimento máximas de 0,12, 0,19 and 0,06 dia-1 nas latitudes de 24°S, 26°S and 30°S, respectivamente. A análise das taxas de transferências de energia das correntes médias para as pertubações revelou que a instabilidade barotrópica é de 60 a 90% menor que a instabilidade baroclínica. No entanto observou-se que as propriedades das instabilidades da BC são altamente sensíveis à presença de instabilidade barotrópica. A topografia demonstrou possuir um efeito estabilizador ao longo de toda trajetória da CB. Ao largo do Cabo de Santa Marta (28°S) os meandros ciclônicos da CB tiveram suas características exploradas do ponto de vista observacional. Combinando uma grande variedade de observações, foi obtido uma visão geral de tais feições, assim como as relações entre seus padrões de velocidade, propriedades da água do mar (temperatura, salinidade, nutrientes), distribuição de clorofila A e a variabilidade da BC. As observações quasi-sinóticas de velocidade em toda a coluna mostraram que os meandros possuem diâmetro superiores à 100 km e extensão vertical de aproximadamente 1500 m. Desta forma, observou-se feições que recirculam uma pequena parte (∼1.5 à 4 Sv) do eixo principal da CB (-13.16 à -17.8 Sv) composta por Água Tropical, Água Central do Atlântico Sul, Água Intermediária Antártica e Água Circumpolar Superior. Além disso, evidências de que tais meandros influenciam ativamente no transporte de águas da Plataforma Continental, ricas em nutrientes, para regiões profundas do Talude Continental foram encontradas. A análise de imagens de satelitárias indicaram que essas feições são efetivamente recorrentes na região e ocorrrem entre 5 a 6 vezes por ano. Para concluir, registros correntográficos indicaram que aproximadamente metade da variância da componente da velocidade ao logo das isóbatas, sobre o talude continental, é devido à atividade de mesoescala da CB.

We use hydrographic and direct velocity observations from two quasi-synoptic cruises in conjunction with a primitive equation linear instability model, to investigate the Brazil Current (BC) downstream change effect between 23°S-30°S on the temporal mixed instabilities properties. The quasi-synoptic data revealed that the BC is ∼400-500 m deep to the north of the so-called Santos Bifurcation (26°S-28°S) and extends down to 1000 m to the south of it. We estimated that the BC receives at least 7 Sv from the Santos Bifurcation, which drastically alters the BC\'s velocity vertical structure and meanders characteristics as it flows poleward. Based on direct velocity measurements, we computed the mixed-instability properties at three different latitudes (24°S, 26°S and 30°S). The instability analysis revealed unstable current systems to mesoscale perturbations with maximum growth rates of 0.12, 0.19 and 0.06 day-1 at 24°S, 26°S and 30°S respectively. The corresponding downstream phase speeds are -0.19, -0.24 and -0.26 m s-1. The analysis of the mean-to-eddy energy conversion terms show that the barotropic instability drains 60-90% less energy from the background state than the baroclinic instability. Nevertheless, the maximum growth rates are at least the double in magnitude when both instabilities occur simultaneously. The topography presents a stabilizing effect for both kind of instabilities along all the BC path. At the vicinities of the Cape Santa Marta (28°S), we explored the the recurrent cyclonic meanders of the BC. Combining a wide range of observations, we provided a overview of such features and the relations between its velocity patterns, the water properties (temperature, salinity, nutrients), chlorophyll-a distribution and the BC variability. The top-bottom quasi-synoptic velocity measurements depicted cyclonic meanders over the continental slope with diameters larger than 100 km and vertically extending to approximately 1500 m depth. Moreover, the observed eddies seems to trap and recirculate a small portion (∼1.5 to 4 Sv) of the BC main flow (-13.16 to -17.89 Sv), which is consisted of Tropical Water (TW), South Atlantic Central Water (SACW), Antarctic Intermediate Water (AAIW) and Upper Circumpolar Deep Water (UCDW). Additionally, we presented observational evidence that the meanders actively influence the transport of nutrient-rich shelf waters to the open ocean enhancing the primary productivity at the photic zone over the continental slope. Satellite imagery show that these cyclonic events occur 5-6 times per year and are generally associated with wave-like perturbations on the flow with mean wavelength of ∼219 km. Finally, Empirical Orthogonal Functions (EOF) analysis computed from an array of mooring lines show that more than half of the along-isobath velocity variance on the continental slope is explained by the BC mesoscale activity. / As propriedades de instabilidade temporal mista da Corrente do Brasil (CB), entre 23°S-30°S, foram investigadas combinando dados hidrográficos e medições diretas de velocide com modelagem numérica. As observações revelaram uma CB com ∼400-500 m de profundidade ao norte da Bifurcação de Santos (26°S-28°S). Em contrapartida, a CB ao sul da bifurcação se mostrou muito mais profunda (> 1000 m) devido ao aporte de aproximadamente 7 Sv de águas em profundidades intermediárias (∼500-1500 m) oriundas do ramo sul da Bifurcação de Santos. Baseado-se nas observações, experimentos numéricos foram conduzidos em três latitudes (24°S, 26°S and 30°S), com o intuito de se estudar as propriedades da instabilidade geofísica da CB. Tais experimentos mostraram que o sistema de correntes é instável para perturbações de mesoescala com taxas de crescimento máximas de 0,12, 0,19 and 0,06 dia-1 nas latitudes de 24°S, 26°S and 30°S, respectivamente. A análise das taxas de transferências de energia das correntes médias para as pertubações revelou que a instabilidade barotrópica é de 60 a 90% menor que a instabilidade baroclínica. No entanto observou-se que as propriedades das instabilidades da BC são altamente sensíveis à presença de instabilidade barotrópica. A topografia demonstrou possuir um efeito estabilizador ao longo de toda trajetória da CB. Ao largo do Cabo de Santa Marta (28°S) os meandros ciclônicos da CB tiveram suas características exploradas do ponto de vista observacional. Combinando uma grande variedade de observações, foi obtido uma visão geral de tais feições, assim como as relações entre seus padrões de velocidade, propriedades da água do mar (temperatura, salinidade, nutrientes), distribuição de clorofila A e a variabilidade da BC. As observações quasi-sinóticas de velocidade em toda a coluna mostraram que os meandros possuem diâmetro superiores à 100 km e extensão vertical de aproximadamente 1500 m. Desta forma, observou-se feições que recirculam uma pequena parte (∼1.5 à 4 Sv) do eixo principal da CB (-13.16 à -17.8 Sv) composta por Água Tropical, Água Central do Atlântico Sul, Água Intermediária Antártica e Água Circumpolar Superior. Além disso, evidências de que tais meandros influenciam ativamente no transporte de águas da Plataforma Continental, ricas em nutrientes, para regiões profundas do Talude Continental foram encontradas. A análise de imagens de satelitárias indicaram que essas feições são efetivamente recorrentes na região e ocorrrem entre 5 a 6 vezes por ano. Para concluir, registros correntográficos indicaram que aproximadamente metade da variância da componente da velocidade ao logo das isóbatas, sobre o talude continental, é devido à atividade de mesoescala da CB.

O meandramento da Corrente do Brasil (CB) ao sul da Bifurcação de Santos é investigada por meio de imagens satelitárias, dados quase-sinóticos, análise de funções ortogonais empíricas (EOF) de correntômetros de fundeios e um modelo analítico semi-teórico. A análise das imagens satelitárias revelam que em média 1,2 meandros ciclônicos de grande amplitude são formados anualmente nas vizinhanças do Cabo de Santa Marta (∼28,5°S). Os meandros parecem ser geostroficamente instáveis e a taxa de crescimento típica estimada é de 0,05 m s-1 . Eles ainda se propagam para sul com velocidade de fase de 0,07 m s-1 . A seção de velocidade, como a inferida por perfis de L-ADCP obtidos durante cruzeiros hidrográficos, revelam que os meandros do Cabo de Santa Marta possuem estrutura de velocidade distinta daquelas observadas em Cabo Frio (23°S) e Cabo de São Tomé (22°S). Os meandros alcançam profundidades maiores que 1400 m e recirculam Água Tropical, Água Central do Atlântico Sul, Água Intermediária Antártica e Água Circumpolar Superior. Ocasionalmente, a estrutura do vórtice se funde com a camada subjacente da Corrente de Contorno Oeste Profunda. O padrão geostrófico horizontal dos meandros foram mapeados usando dados de temperatura e salinidade de cruzeiros históricos e foi obtido que a estrutura ciclônica do meandro possui número de Rossby (∼0,07) e número de Burger (∼0,06) pequenos. Portanto, vorticidade de estiramento parece ter papel importante na dinâmica de meandramento e, consequentemente, instabilidade baroclínica é o fenômeno primariamente responsável pelo crescimento do ciclone. O número de Burger pequeno também sugere que a dinâmica do meandro é influênciada pela topografia. A análise de EOFs bidimensionais conduzida no transecto WOCE 28°S de fundeios históricos dos anos 90 mostram que o primeiro modo seccional explica cerca de 54% da variância das séries e está relacionado ao meandramento da CB. A amplitude do meandro ciclônico é aproximadamente 200 km uma vez que cruza o transecto e a onda de vorticidade baroclínica associada tem tipicamente 26 dias. Finalmente, um modelo de Dinâmica de Contornos idealizado de 2 camadas é construído para isolar o mecanismo de instabilidade baroclínica e para investigar as razões do crescimento e velocidade de fase para sul. A estrutura do fluxo básico do modelo é construído baseado no ajuste por mínimos quadrados das funções teóricas à média das observações nas espessuras das camadas. A simulação mostrou que o meandro evolui e se desenvolve devido ao fechamento de fase da camada inferior mais lenta relativo à camada superior mais rápida. Além disso, a propagação de fase para sul ocorre como uma consequência direta da componente barotrópica robusta, adquirida pela CB devido o ramo sul da Bifurcação de Santos. / The Brazil Current (BC) meandering south of the so-called Antarctic Intemediate Water\'s Santos Bifurcation is investigated by means of satellite imagery, quasi-synoptic data, empirical orthogonal function (EOF) analysis of currentmeter moorings and a semi-theoretical dynamical model. The analysis of the infrared imagery revealed that on average 1.2 large amplitude cyclonic meanders are formed annualy in the vicinities of Cape Santa Marta (∼28.5°S). The meanders seem to be geophysically unstable and the estimated typical growth rate is of 0.05 days-1 . They also propagate southward with phase speed of 0.07 m s-1 . The sectional velocity distributions, as inferred from L-ADCP profiles obtained during hydrographic cruises, revealed that the Cape Santa Marta meanders have a very distinct vertical structure from those observed off Cape Frio (23°S) and Cape São Tomé (22°S). The meanders reach much depths of 1400 m and recirculated Tropical Water, South Atlantic Central Water, Antarctic Intemediate Water and Upper Circumpolar Waters. Occasionally, the eddy structure melds with the underlying Deep Western Boundary Current. Geostrophic horizontal patterns of the meanders were mapped using T-S information from historical cruises and it is obtained that the meander is a low-Rossby number (∼0.07) and low-Burger(∼0.06) number cyclone feature. Therefore, stretching vorticity seems to play a major role on the meandering dynamics and, consequently, baroclinic instability is the phenomenon primairily responsible for the cyclone growth. The low-Burger number also suggests that the meander dynamics is influenced by the topography. The two-dimensional EOF analysis conducted on the historical 28°S WOCE mooring transect from the 90s shows that the first sectional mode explains about 54% of the series variance and is related to the BC meandering. The amplitude of the cyclonic meander is roughly 200 km as it crosses the transect and the associated baroclinic vorticity wave period is typically 26 days. Finally, an idealized 2-layer Contour Dynamics model is constructed to isolate the baroclinic instability mechanism and to investigate the reasons for the growth and the southward phase speeds. The model\'s basic flow structure is built based on least-square fits of the observations averaged within the two layer\'s vertical extensions. The simulation showed that the meander evolve and grow due to the phase-locking of the slower lower layer relative to the faster upper layer. Also, the southward phase speed occurs as a direct consequence of the robust barotropic component acquired by the BC due to the southern branch of the Santos Bifurcation of the Antarctic Intemediate Water.

A partir d'un ensemble de données d'observation ainsi qu'un modèle couplé physiquebiogéochimique à haute résolution (CROCO-PISCES), cette thèse explore les processus biophysiques associés à l’une des plus grandes floraisons phytoplanctoniques de l’océan global, au Sud-Est de Madagascar, et le possible rôle des tourbillons sur ces blooms. L’étude montre que ce phénomène se produit dans une région caractérisée par une couche de mélange peu profonde, avec des eaux de surface moins salées probablement associées au courant Sud-Est de Madagascar (SEMC), et avec une structure dipolaire dans la circulation moyenne. Les observations ont révélé une diminution des remontées d’eaux froides (upwelling) le long des côtes sud-est de Madagascar pendant les mois de bloom. Dans le modèle, les nitrates provenant des niveaux de subsurface (advection verticale ; upwelling) ainsi que de la côte malgache (advection horizontale) favorisent la production phytoplanctonique simulée. Une expérience lagrangienne de particules montre une plus forte advection de ces dernières dans la zone de floraison pendant les périodes de bloom alors qu’elles sont déviées vers le sud de Madagascar vers le continent Africain pendant les années sans floraison. Une étude est réalisée à partir d’un jeu de données de suivi des tourbillons co-localisés avec des flotteurs de profilage Argo, pour mieux comprendre des tourbillons intensifiés en surface et subsurface. Une méthode d’identification des structures tourbillonnaires de subsurface a été mise en place en se basant sur l’anomalie de la hauteur dynamique stérique. Ces tourbillons, appelés ‘SIDDIES’ (South Indian ocean eDDIES), se produisent en tant que tourbillon intensifié en surface (surfSIDDIES) et en subsurface (subSIDDIES). Ils se déplacent le long d’une bande de latitude située entre 15°S et 35°S appelée « couloir SIDDIES ». Au cours de leurs déplacements, les subSIDDIES cycloniques (anticycloniques) transportent via les processus d’advection, des masses d’eaux chaudes et peu salées de l’Est vers l’Ouest de l’Océan Indien, contribuant ainsi à environ 58% (32%) du flux total de chaleur par tourbillons dans le sud de l'océan Indien. / Using observational datasets and a high resolution coupled biophysical model (CROCOPISCES), the main aims of this thesis is to study the biophysical processes associated with one of the largest phytoplankton blooms in global ocean, southeast of Madagascar, and the possible role of mesoscale eddies.The study has shown that the bloom occurs in a region of shallow-stratified mixed layer water, with low-salinity waters at the surface possibly associated with the South-East Madagasacar Current (SEMC), and dipole structure in the mean circulation. Observations show that curren-driven upwelling south of Madagascar is reduced during bloom months. It is shown in the model that nitrate from subsurface levels (upwelling) as well as from the Madagascan coast (advection) fertilize the simulated bloom. A Lagrangian analysis shows dispersion of higher percentages of particles in the bloom region during bloom years and south of Madagascar during non-bloom years.Using co-located Argo profiles and an eddy detected algorithm dataset, surface and subsurface-intensified eddies are studied. Subsurface eddies are identified using a detection method based on their steric dynamic height anomaly. Referred to as `SIDDIES’ (South Indian ocean eDDIES), they occur as surface (surfSIDDIES) or subsurface (subSIDDIES) and propagate along a latitudinal band (15°S-35°S) termed as `SIDDIES Corridor’. Advecting warm and fresh water during their propagation, cyclonic (anticyclonic) subSIDDIES contribute about 58% (32%) of the total eddy-heat flux in the South Indian Ocean.

O meandramento da Corrente do Brasil (CB) ao sul da Bifurcação de Santos é investigada por meio de imagens satelitárias, dados quase-sinóticos, análise de funções ortogonais empíricas (EOF) de correntômetros de fundeios e um modelo analítico semi-teórico. A análise das imagens satelitárias revelam que em média 1,2 meandros ciclônicos de grande amplitude são formados anualmente nas vizinhanças do Cabo de Santa Marta (∼28,5°S). Os meandros parecem ser geostroficamente instáveis e a taxa de crescimento típica estimada é de 0,05 m s-1 . Eles ainda se propagam para sul com velocidade de fase de 0,07 m s-1 . A seção de velocidade, como a inferida por perfis de L-ADCP obtidos durante cruzeiros hidrográficos, revelam que os meandros do Cabo de Santa Marta possuem estrutura de velocidade distinta daquelas observadas em Cabo Frio (23°S) e Cabo de São Tomé (22°S). Os meandros alcançam profundidades maiores que 1400 m e recirculam Água Tropical, Água Central do Atlântico Sul, Água Intermediária Antártica e Água Circumpolar Superior. Ocasionalmente, a estrutura do vórtice se funde com a camada subjacente da Corrente de Contorno Oeste Profunda. O padrão geostrófico horizontal dos meandros foram mapeados usando dados de temperatura e salinidade de cruzeiros históricos e foi obtido que a estrutura ciclônica do meandro possui número de Rossby (∼0,07) e número de Burger (∼0,06) pequenos. Portanto, vorticidade de estiramento parece ter papel importante na dinâmica de meandramento e, consequentemente, instabilidade baroclínica é o fenômeno primariamente responsável pelo crescimento do ciclone. O número de Burger pequeno também sugere que a dinâmica do meandro é influênciada pela topografia. A análise de EOFs bidimensionais conduzida no transecto WOCE 28°S de fundeios históricos dos anos 90 mostram que o primeiro modo seccional explica cerca de 54% da variância das séries e está relacionado ao meandramento da CB. A amplitude do meandro ciclônico é aproximadamente 200 km uma vez que cruza o transecto e a onda de vorticidade baroclínica associada tem tipicamente 26 dias. Finalmente, um modelo de Dinâmica de Contornos idealizado de 2 camadas é construído para isolar o mecanismo de instabilidade baroclínica e para investigar as razões do crescimento e velocidade de fase para sul. A estrutura do fluxo básico do modelo é construído baseado no ajuste por mínimos quadrados das funções teóricas à média das observações nas espessuras das camadas. A simulação mostrou que o meandro evolui e se desenvolve devido ao fechamento de fase da camada inferior mais lenta relativo à camada superior mais rápida. Além disso, a propagação de fase para sul ocorre como uma consequência direta da componente barotrópica robusta, adquirida pela CB devido o ramo sul da Bifurcação de Santos. / The Brazil Current (BC) meandering south of the so-called Antarctic Intemediate Water\'s Santos Bifurcation is investigated by means of satellite imagery, quasi-synoptic data, empirical orthogonal function (EOF) analysis of currentmeter moorings and a semi-theoretical dynamical model. The analysis of the infrared imagery revealed that on average 1.2 large amplitude cyclonic meanders are formed annualy in the vicinities of Cape Santa Marta (∼28.5°S). The meanders seem to be geophysically unstable and the estimated typical growth rate is of 0.05 days-1 . They also propagate southward with phase speed of 0.07 m s-1 . The sectional velocity distributions, as inferred from L-ADCP profiles obtained during hydrographic cruises, revealed that the Cape Santa Marta meanders have a very distinct vertical structure from those observed off Cape Frio (23°S) and Cape São Tomé (22°S). The meanders reach much depths of 1400 m and recirculated Tropical Water, South Atlantic Central Water, Antarctic Intemediate Water and Upper Circumpolar Waters. Occasionally, the eddy structure melds with the underlying Deep Western Boundary Current. Geostrophic horizontal patterns of the meanders were mapped using T-S information from historical cruises and it is obtained that the meander is a low-Rossby number (∼0.07) and low-Burger(∼0.06) number cyclone feature. Therefore, stretching vorticity seems to play a major role on the meandering dynamics and, consequently, baroclinic instability is the phenomenon primairily responsible for the cyclone growth. The low-Burger number also suggests that the meander dynamics is influenced by the topography. The two-dimensional EOF analysis conducted on the historical 28°S WOCE mooring transect from the 90s shows that the first sectional mode explains about 54% of the series variance and is related to the BC meandering. The amplitude of the cyclonic meander is roughly 200 km as it crosses the transect and the associated baroclinic vorticity wave period is typically 26 days. Finally, an idealized 2-layer Contour Dynamics model is constructed to isolate the baroclinic instability mechanism and to investigate the reasons for the growth and the southward phase speeds. The model\'s basic flow structure is built based on least-square fits of the observations averaged within the two layer\'s vertical extensions. The simulation showed that the meander evolve and grow due to the phase-locking of the slower lower layer relative to the faster upper layer. Also, the southward phase speed occurs as a direct consequence of the robust barotropic component acquired by the BC due to the southern branch of the Santos Bifurcation of the Antarctic Intemediate Water.