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of buoyancy and topographic effects. Beyond planetary cores, such models are relevant for oceanic and atmospheric flows, where these effects modifies the stress on the ground floor. the ERC THEIA group have
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of flexible fibres by a turbulent flow, such as plastic debris or organic matter in oceans and rivers. Modelling the dynamics of such deformable particles in these environmental flows remains a major challenge
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the study of the physico-chemical processes governing the Earth's and planetary atmospheres and their interfaces with the surface, the ocean and the interplanetary environment. The team involved in
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OSSO BUCO: Outer Solar System Objects with high BUlk Carbon cOntent. It aims at determining the nature of the fluids emitted by carbon-rich planetary cores in the oceans and ices of the moons of giant