Are the different gully morphologies due to different formation processes on the Kaiser dune field on Mars?
Kelly Pasquon1, Julien Gargani1, Marion Nachon2, Susan J Conway3, Marion Massé4, Gwenael Jouannic5, Matthew R Balme6, François Costard1 and Mathieu Vincendon7, (1)GEOPS Géosciences Paris-Sud, Université Paris-Sud, CNRS, Université Paris-Saclay, Orsay, France, (2)UC Davis Earth and Planetary Sciences, University of California, Davis, CA, United States, (3)LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes, France, (4)Laboratoire de Planétologie et Géodynamique, Nantes, France, (5)Center for expertise and engineering on risks, urban and country planning, environment and mobility - Cerema, Laboratoire Régional de Nancy, TOMBLAINE, France, (6)The Open University, School of Physical Sciences, Milton Keynes, United Kingdom, (7)IAS, Institut d'astrophysique Spatiale, Université Paris-Sud, Université Paris-Saclay, Orsay, France
