Les eaux modales de l'Océan Austral

• Main Author: Sallée, Jean-Baptiste
• Other Authors: Laboratoire d'études en Géophysique et océanographie spatiales (LEGOS), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), Université Paul Sabatier - Toulouse III, Rosemary Morrow
• Format: Doctoral or Postdoctoral Thesis
• Language: French
• Published: HAL CCSD 2007
• Subjects: Ocean; Subantarctic mode water; Diffusion; Océan Austral; Eaux modales; Tourbillons; Fronts; Couche de mélange; [SDU.OCEAN]Sciences of the Universe [physics]/Ocean; Atmosphere; Southern Ocean
• Online Access: https://theses.hal.science/tel-00193791; https://theses.hal.science/tel-00193791/document; https://theses.hal.science/tel-00193791/file/merged.pdf

Subantarctic mode water (SAMW) are formed in the Southern Ocean in the deep winter mixed layers north of the Subantarctic front. They influence the climate at interannual and decadal scales and play a fundamental role in the ventilation of Southern Hemisphere thermocline. We study the details of SAMW formation using the recent deployment of ARGO profiling floats and GDP surface drifters, which provide an excellent space-time coverage of the Southern Ocean upper ocean processes. Since the beginning of the ARGO international program, the number of vertical hydrographic profiles in the Southern Ocean have increased considerably so that nowadays we have a comparable number of profiles to decades of hydrographic ship data. Based on this dataset, we found that the dominant forcing for SAMW formation in winter in the Southern Indian Ocean was due to air-sea and Ekman fluxes. We found a rapid transition to thicker surface mixed layers in the central South Indian Ocean, at about 70°, associated with a reversal of the horizontal eddy heat diffusion in the surface layer and the meridional expansion of the ACC as it rounds the Kerguelen Plateau. These effects are ultimately related to the bathymetry of the region, leading to the seat of formation in the region southwest of Australia. SAMW formation is tightly linked to the Southern Ocean dynamics and position of the main polar fronts. A second study concerned the ACC circulation and frontal variability. In this study we mixed in-situ and altimeter data to monitor the position of the two main fronts of the ACC during the period 1993-2005. Then, we related their movements to the two main atmospheric climate modes of the Southern Hemisphere, the Southern Annular Mode (SAM) and the El-Nino Southern Oscillation (ENSO). We found that although the fronts are steered by the bathymetry, which sets their mean pathway at first order, in flat-bottom areas the fronts are subject to large meandering due to mesoscale activity and atmospheric forcing. In parallel, we developed a new ...