*Adrian Brines1,2, Shohei Aoki1,3, Frank Daerden4, Michael S. Chaffin5, Samuel A. Atwood6,7, Susarla Raghuram5, Bruce A. Cantor8, Yannick Willame4, Loïc Trompet4, Geronimo L. Villanueva7, Michael J. Wolff9, Michael D. Smith7, Christopher S. Edwards10, Ian R. Thomas4, Giuliano Liuzzi11, Lori Neary4, Manish R. Patel12, Miguel Angel Lopez Valverde2, Armin Kleinböhl13, Hoor AlMazmi14, James Whiteway15, Ann Carine Vandaele3,4, Bojan Ristic4, Giancarlo Bellucci16
(1. Department of Complexity Science and Engineering, University of Tokyo, Kashiwa, Japan, 2. Solar System Department, Instituto de Astorfísica de Andalucía (IAA-CSIC), Granada, Spain, 3. Department of Geophysics, Graduate School of Science, Tohoku University, Sendai, Japan, 4. Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels, Belgium, 5. Laboratory for Atmospheric and Space Physics (LASP), University of Colorado Boulder, Boulder, CO, USA, 6. University of Maryland Baltimore County, Baltimore, MD, USA, 7. NASA Goddard Space Flight Center, Greenbelt, MD, USA, 8. Malin Space Science Systems, San Diego, CA, USA, 9. Space Science Institute, Boulder, CO, USA, 10. Radiant Center for Remote Sensing, Department of Astronomy and Planetary, Northern Arizona University, Flagstaff, AZ, USA, 11. School of Engineering, Universitá degli Studi della Basilicata, Potenza, Italy, 12. School of Physical Sciences, The Open University, Milton Keynes, UK, 13. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA, 14. United Arab Emirates Space Agency, Abu Dhabi, UAE, 15. Centre for Research in Earth and Space Science, York University, Toronto, ON, Canada, 16. Istituto di Astrofisica e Planetologia, Rome, Italy)
Keywords:Mars, Dust Storm, Hydrogen escape, Water vapor