Effects of the Crustal Magnetic Fields and Changes in the IMF Orientation on the Magnetosphere of Mars: MAVEN Observations and LATHYS Results.
Norberto Romanelli1, Ronan Modolo1, Francois Leblanc2, Jean-Yves Chaufray3, Sebastien Hess4, Dave A Brain5, John E P Connerney6, Jasper S Halekas7, James P McFadden8 and Bruce Martin Jakosky9, (1)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (2)LATMOS/IPSL, CNRS, Sorbonne Université, UVSQ, Paris, France, (3)LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, Guyancourt, France, (4)ONERA Toulouse, Toulouse Cedex 04, France, (5)University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)Space Research Corporation, Annapolis, United States, (7)University of California Berkeley, Berkeley, CA, United States, (8)SSL, University of California Berkeley, Berkeley, United States, (9)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States
