*Matthieu Civel5, Xavier Crosta1, Giuseppe Cortese2, Elisabeth Michel3, Alain Mazaud3, Samuel Jaccard4, Lena Thöle4, Minoru Ikehara5
(1.UMR 5805 CNRS EPOC, Université de Bordeaux, France, 2.GNS Science, Lower Hutt, New Zealand, 3.LSCE-IPSL, CEA-CNRS-UVSQ, 91198 Gif-sur-Yvette, France, 4.Institute of Geological Sciences & Oeschger Centre for Climate Change Research, University of Bern, Switzerland, 5.Center for Advanced Marine Core Research, Kochi University, Japan)
Keywords:Southern Ocean, Paleoceanography, Micropaleontology, Radiolarian, Kerguelen Plateau
The Southern Ocean (SO) is a place of primordial importance to the understanding of global ocean circulation as it connects the Atlantic, the Pacific and the Indian oceans and thus actively participates in Atlantic Meridional Overturning Circulation (AMOC). Climate processes and variations in the Indian sector of the SO are not as well understood as processes in the Atlantic sector. In this study, sea surface temperatures (SST) are used to better constrain climate and ocean circulation variations in the Indian sector of the SO from Marine Isotopic Stage 3 (MIS 3) to present. We present new high-resolution SST datasets for the past 41kyrs, reconstructed with two statistical approaches Imbrie and Kipp Method (IKM) and Modern Analog Technique (MAT) applied to radiolarian census data. Different signals for surface and subsurface water masses suggest that surface water responded mainly to local processes whereas subsurface waters show a response driven by hemispherical and global processes. Similarly we show that radiolarian and diatom productivity behave differently over the last 41kyrs, probably due to specific oceanic conditions in this zone.