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 Griton1,2, Filippo G E Pantellini3 and Michel Moncuquet3, (1)Meudon, France, (2)CNRS, Observatoire de Paris, LESIA, Meudon, France, (3)CNRS, Observatoire de Paris, LESIA, Meudon, France