Temporal variations of the atomic oxygen on Mars’ upper atmosphere derived from the O I 130.4 nm triplet observed by MAVEN/IUVS
Jean-Yves Chaufray1, Justin Deighan2, Sonal K Jain3, Nick Schneider2, Ian F Stewart2, Michael Chaffin4, Dr. Francis Gerard Eparvier, Ph.D.5, Edward Thiemann4, Phillip C Chamberlin4, Bruce Martin Jakosky6, John T Clarke7 and Majd Mayyasi8, (1)LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, Guyancourt, France, (2)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (3)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States, (4)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (5)University of Colorado at Boulder, Boulder, United States, (6)University of Colorado Boulder, Boulder, CO, UNITED STATES, (7)Boston University, Boston, MA, United States, (8)Boston University, Center for Space Physics, Boston, MA, United States
