Martian upper-atmosphere circulation and tides revealed through MAVEN/IUVS observations of nitric oxide nightglow
Nicholas McCord Schneider1, Arnaud Stiepen2, Zachariah Milby3, Sonal K Jain4, Emilie M Royer5, Justin Deighan6, Francisco Gonzalez-Galindo7, Jean-Claude M. C. Gerard8, Franck Lefèvre9 and Ian F Stewart6, (1)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (2)University of Colorado at Boulder, Boulder, CO, United States, (3)University of Colorado, Boulder, United States, (4)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States, (5)Laboratory for Atmospheric and Space Physics, Boulder, United States, (6)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (7)IAA-CSIC, Granada, Spain, (8)Université de Liège, LPAP - STAR Institute, Liege, Belgium, (9)LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France
