Diurnal Thermal Structure of the Martian Atmosphere from MAVEN/IUVS Stellar Occultations
Diurnal Thermal Structure of the Martian Atmosphere from MAVEN/IUVS Stellar Occultations
Sumedha Gupta1, Roger V Yelle2, Nicholas McCord Schneider3, Sonal Jain4, Francisco Gonzalez-Galindo5, Loic Verdier6, Ashwin S. Braude7, Franck Montmessin8, Majd Mayyasi9 and Justin Deighan4, (1)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, United States, (2)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (3)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (4)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States, (5)IAA-CSIC, Granada, Spain, (6)LATMOS Laboratoire Atmosphères, Observations Spatiales, UVSQ Université Paris-Saclay, Sorbonne université, CNRS, Paris, France, (7)LATMOS Laboratoire Atmosphères, Observations Spatiales, Guyancourt, France, (8)Service d'aéronomie du CNRS, Verrieres Le Buisson, France, (9)Boston University, Center for Space Physics, Boston, MA, United States