Mars’ ultraviolet dayglow observations by IUVS/MAVEN: Structure and variability of Martian upper atmosphere
Sonal Jain1, Ian F Stewart2, Nicholas McCord Schneider3, Justin Deighan3, Arnaud Stiepen4, J. Scott Evans5, Michael H Stevens6, Michael Chaffin3, Matteo Michael James Crismani7, Bill McClintock1, John T Clarke8, Greg Holsclaw9, Daniel Lo10, Franck Lefèvre11, Franck Montmessin12, Ed Thiemann2, Dr. Francis Gerard Eparvier, Ph.D.13 and Bruce Martin Jakosky14, (1)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (3)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (4)University of Colorado at Boulder, Boulder, CO, United States, (5)Computational Physics, Inc., Springfield, United States, (6)Naval Research Lab DC, Space Science Division, Washington, DC, United States, (7)California State University, Department of Physics and Astronomy, San Bernardino, United States, (8)Boston University, Boston, MA, United States, (9)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (10)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (11)LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France, (12)LATMOS Laboratoire Atmosphères, Observations Spatiales, UVSQ Université Paris-Saclay, Sorbonne université, CNRS, Paris, France, (13)Univ Colorado, Boulder, CO, United States, (14)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States
