Study of the Martian cold oxygen corona from the O I 130.4 nm by IUVS/MAVEN
Jean-Yves Chaufray1, Justin Deighan2, Michael Chaffin2, Nicholas McCord Schneider2, Bill McClintock3, Ian F Stewart4, Sonal Jain4, Matteo Michael James Crismani5, Arnaud Stiepen6, Greg Holsclaw7, John T Clarke8, Franck Montmessin9, Dr. Francis Gerard Eparvier, Ph.D.10, Ed Thiemann4, Phillip C Chamberlin11 and Bruce Martin Jakosky12, (1)LATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, Guyancourt, France, (2)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (4)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (5)California State University, Department of Physics and Astronomy, San Bernardino, United States, (6)University of Colorado at Boulder, Boulder, CO, United States, (7)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (8)Boston University, Boston, MA, United States, (9)LATMOS Laboratoire Atmosphères, Observations Spatiales, UVSQ Université Paris-Saclay, Sorbonne université, CNRS, Paris, France, (10)University of Colorado at Boulder, Boulder, United States, (11)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (12)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States
