Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
DESPA, Meudon Observatory - France
Institut de Physique du Globe de Paris, University Paris 7, Paris, France
Département de Modélisation Physique et Numérique, GREEC, IPGP, 4, Place Jussieu, Paris, 75005 France de Paris-Meudon
Équipe de Sismologie, Institut de Physique du Globe de Paris, Université Denis Diderot, Paris, France
Departement de Recherche Spatiale, Observatoire de Meudon, 92190 Meudon, France
Paris, Observatoire, Meudon, France
Meudon, Observatoire, Meudon, Hauts-de-Seine, France
Paris, Observatoire, Meudon, Hauts-de-Seine, France
Observatoire de Paris-Meudon, DESPA, F-92195 Meudon, France
CNRS, Meudon, France
DESPA, France
LESIA, Observatoire de Paris-Meudon, 5 Place Jules Janssen, Meudon, F92195 France de Paris, LESIA, Meudon Cedex, 92195 France STEP, Université Paris-Diderot 7, Paris, France
LESIA, Observatoire de Paris, 5, place Jules Janssen, Meudon, 92195, France de Paris, DESPA, URA 264 CNRS, Meudon, France de Physique du Globe de Paris, Equipe Sismologie, CNRS-UMR 7154, Université Paris Diderot 7, PRES Sorbonne Paris Cité, Paris, France; de Paris-Meudon, Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique, CNRS, Meudon, France
Observatoire de Paris-Meudon, place Jules Janssen, Meudon, 92195, France Observatoire de Paris, CNRS, UPMC, Universite Paris Diderot, 5 Place Jules Janssen, Meudon, 92190, France
Observatoire de Paris-Meudon, Centre National de la Recherche Scientifique, Meudon, France
LESIA, Observatoire de Paris-Meudon, Meudon, France
LESIA, Observatoire de Paris, Université Paris Diderot, CNRS, UPMC, Meudon, France
IPGP, Paris de Physique du Globe de Paris, 4
'Alfvenic' versus 'standard' turbulence in the solar wind
3D Hybrid Simulations of Finite Amplitude Alfven Wave Filamentation.
A large-scale meridional circulation in the convective zone
A New Insight on the Dynamics of Martian Granular Flows in Valles Marineris
A one dimensional, electrostatic Vlasov model for the generation of suprathermal electron tails in solar wind conditions
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