[P-EM21] 惑星大気圏・電磁圏

[PEM21-07] New pathway for water loss to space driven by a northern regional dust storm during the local summer

*Adrian Brines^1,2, Shohei Aoki^1,3, Frank Daerden⁴, Michael S. Chaffin⁵, Samuel A. Atwood^6,7, 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 Vandaele^3,4, 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)

キーワード：Mars, Dust Storm, Hydrogen escape, Water vapor