MHD simulations of the interaction of the Solar Wind with fast-rotating planetary magnetospheres using a time-dependant background/residual decomposition of the magnetic field

Léa Sophie Griton, IRAP, Université Toulouse III—Paul Sabatier, CNRS, CNES, Toulouse, France, Filippo G E Pantellini, CNRS, Observatoire de Paris, LESIA, Meudon, France and Michel Moncuquet, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, LESIA, Meudon, France
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