Mars’ ultraviolet dayglow observations by IUVS/MAVEN: Structure and variability of Martian upper atmosphere
Mars’ ultraviolet dayglow observations by IUVS/MAVEN: Structure and variability of Martian upper atmosphere
Sonal Jain1, Ian F Stewart2, Nicholas McCord Schneider3, Justin Deighan4, Arnaud Stiepen5, J. Scott Evans6, Michael H Stevens7, Michael Chaffin3, Matteo Michael James Crismani8, Bill McClintock1, John T Clarke9, Greg Holsclaw10, Daniel Lo11, Franck Lefèvre12, Franck Montmessin13, Ed Thiemann2, Dr. Francis Gerard Eparvier, Ph.D.14 and Bruce Martin Jakosky15, (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)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States, (5)University of Colorado at Boulder, Boulder, CO, United States, (6)Computational Physics, Inc., Springfield, United States, (7)Naval Research Lab DC, Space Science Division, Washington, DC, United States, (8)California State University, Department of Physics and Astronomy, San Bernardino, United States, (9)Boston University, Boston, MA, United States, (10)Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, (11)University of Michigan, Ann Arbor, United States, (12)LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France, (13)Laboratoire Atmosphères, Observations Spatiales, IPSL, CNRS, UVSQ, Sorbonne Université, Guyancourt, France, (14)Univ Colorado, Boulder, CO, United States, (15)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States