The Martian diffuse aurora: Monte Carlo simulations and comparison with IUVS-MAVEN observations
Jean-Claude M. C. Gerard1, Lauriane Soret2, Nicholas McCord Schneider3, Valery Shematovich4, Dmitry Bisikalo4, Stephen W Bougher5, Sonal Jain6, Robert J Lillis7, David L Mitchell8, Bruce Martin Jakosky8, Justin Deighan9 and Davin E Larson10, (1)Université de Liège, Liege, Belgium, (2)Université de Liège, STAR-LPAP, Liège, Belgium, (3)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (4)Institute of Astronomy, Moskow, Russia, (5)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering Department, Ann Arbor, MI, United States, (6)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (7)University of California Berkeley, Berkeley, CA, United States, (8)University of Colorado at Boulder, Boulder, CO, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (10)Space Sciences Laboratory, Berkeley, United States
