Comparison of the Active Bagnold Dune Field with Other Aeolian Deposits Observed at Gale using ChemCam Data.
Agnes Cousin1, Erwin Dehouck2, Pierre-Yves Meslin2, Amy J Williams3, Nathaniel Stein4, Olivier Gasnault1, Nathan Bridges5, Bethany L Ehlmann6, Susanne Schröder7, Valerie Payre8, William Rapin9, Patrick Claude Pinet2, Violaine Sautter10, Nina Lanza11, Jeremie Lasue2, Sylvestre Maurice12 and Roger C Wiens13, (1)IRAP, Toulouse, France, (2)Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)California Institute of Technology, Pasadena, CA, United States, (5)American Geophysical Union, Washington, DC, United States, (6)California Institute of Technology, Geological and Planetary Sciences, Pasadena, CA, United States, (7)German Aerospace Center, Berlin, Germany, (8)Université de Lorraine, Nancy, France, (9)Universite de Toulouse, Toulouse Cedex 4, France, (10)MNHN, CNRS, Paris Cedex 16, France, (11)Los Alamos National Laboratory, Los Alamos, NM, United States, (12)IRAP, CNRS, Université de Toulouse, UPS-OMP, Toulouse, France, (13)CNRS, Paris Cedex 16, France
