Abundances of O3 and O2 in the Martian Atmosphere Retrieved from MAVEN/IUVS Stellar Occultations
Hannes Gröller1, Franck Lefèvre2, Francisco Gonzalez-Galindo3, Roger V Yelle4, Tommi Koskinen5, Franck Montmessin6, Nick Schneider7, Justin Deighan7 and Sonal Jain7, (1)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (2)LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France, (3)IAA-CSIC, Granada, Spain, (4)University of Arizona, Lunar and Planetary Laboratory, Tucson, United States, (5)University of Arizona, Tucson, United States, (6)Laboratoire Atmosphères, Observations Spatiales, IPSL, CNRS, UVSQ, Sorbonne Université, Guyancourt, France, (7)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
