Probing the Martian Atmosphere with MAVEN/IUVS Stellar Occultations

Hannes Gröller1, Roger V Yelle1, Tommi Koskinen2, Franck Montmessin3, Gaetan Lacombe4, Nicholas McCord Schneider5, Justin Deighan5, Ian F Stewart6, Sonal Jain6, Michael Chaffin5, Matteo Michael James Crismani7, Arnaud Stiepen8, Franck Lefèvre9, Bill McClintock10, John T Clarke11, Greg Holsclaw12, Paul R Mahaffy13, Stephen W Bougher14 and Bruce Martin Jakosky15, (1)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (2)University of Arizona, Tucson, AZ, United States, (3)LATMOS Laboratoire Atmosphères, Observations Spatiales, UVSQ Université Paris-Saclay, Sorbonne université, CNRS, Paris, France, (4)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (5)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (7)California State University, Department of Physics and Astronomy, San Bernardino, United States, (8)University of Colorado at Boulder, Boulder, CO, United States, (9)LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France, (10)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (11)Boston University, Boston, MA, United States, (12)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (13)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (14)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering Department, Ann Arbor, MI, United States, (15)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States