Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Service d'Aeronomie, CNRS, verrieres, 91371 France d'Aéronomie, Institut Pierre Simon Laplace, Université Paris 6 / CNRS, Verrières-le-Buisson, France
Service d'Aéronomie du Centre National de la Recherche Scientifique / Institut Pierre-Simon Laplace, Verrières-le-Buisson, France
Service d'Aéronomie du CNRS / IPSL, Paris, France
Service d'Aronomie du CNRS / IPSL, Verrières-Le-Buisson, France
LATMOS / IPSL, Université Versailles Saint Quentin, CNRS, France
Department of Astronomy and Engineering, University of Virginia
LATMOS, UVSQ, Versailles Saint Quentin, France;
Engineering Physics - Department of Astronomy, University of Virginia
LATMOS, UVSQ & IPSL, Guyancourt, France;
LATMOS - IPSL / UVSQ, Guyancourt, France;
Laboratoire de Physique des Plasmas, Ecole Polytechnique / UPMC / CNRS, Saint-Maur des Fossés, France; d'Aéronomie du CNRS / IPSL, Université Pierre et Marie Curie, France
Laboratoire Atmospheres, Milieux, Observations Spatiales, IPSL, CNRS, Verrières-le-Buisson, France
Engineering Physics and Department of Astronomy, University of Virginia, 102, Charlottesville, 22903, VA, USA
Service d'Aeronomie du CNRS
Service d'aeronomie, France
Service d'aeronomie du CNRS, Reduit de Verrieres BP 3 Route des Gatines, Verrieres le Buisson, 91371 France
Service d'Aéronomie du CNRS / Institut Pierre-Simon Laplace, Université Pierre et Marie Curie, Verrières-Le-Buisson, France
Service d'aéronomie du CNRS / IPSL, Verrières-le-Buisson, France
Service d'Aéronomie du CNRS / IPSL, Université Pierre et Marie Curie, Paris, France
Service d'aeronomie du CNRS, Reduit de Verrieres, BP 3, Routes des Gatines, Verrieres le Buisson, 91371 France d'aeronomie du CNRS, Reduit de Verrieres BP 3 Route des Gatines, Verrieres le Buisson, 91371, France d'Aéronomie du CNRS, Verr
3d GCM-Ionosphere Model To Describe the Martian Ionospheric Dynamics
A Fokker-Planck Approach for the Expansion of the Fast Solar Wind: Why and How?
A Generalized Model for the Proton Expansion in Astrophysical Winds. I. The Velocity Distribution Function Representation
A model of interaction of Phobos' surface with the martian environment
A Model of Phobos Surface Interaction with the Solar Wind and the Martian Environment
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