*Kanako Seki1, Takuya Hara2, Dave A Brain3, Rob J. Lillis2, Naoki Terada4, Hiromu Nakagawa4, Darvin E. Larson2, Dave L. Mitchell2, Gina A. Dibraccio5, Nicholas McCord Schneider3, Sonal K. Jain3, Janet G. Luhmann2, Bruce M. Jakosky3 (1.Graduate School of Science, University of Tokyo, 2.Space Sciences Laboratory, University of California, Berkeley, 3.LASP, University of Colorado, Boulder, 4.Graduate School of Science, Tohoku University, 5.Goddard Space Flight Center, NASA)
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
[P-PS08] Mars and Mars system: results from a broad spectrum of Mars studies and aspects for future missions
NASA's Magnetospheric Multiscale (MMS) formation flying satellites have been making unprecedentedly high time resolution measurements of collisionless plasmas in and around Earth's magnetosphere since it was launched in 2015. After completing its nominal mission in 2018, MMS has continued its observations including targeting the magnetic reconnection in the Earth's magnetotail.
The major purpose of this session is to summarize the new world of electron physics that MMS has so far revealed and also to consider a future observation plan recently submitted by the mission team for the extended mission of MMS especially during the coming several years.
The collaboration with multiple missions including Geotail, Cluster II, THEMIS, Arase and other solar terrestrial probes while MMS focuses into electron scale is the key to understanding multiscale phenomena in the Earth's magnetosphere.
We solicit contributions from satellite observations, numerical simulations, laboratory observations, and theories that relate MMS observations. Contributions to the possible future observation plans are especially welcome.
This is a joint session with American Geophysical Union (AGU).
We hope this session will promote further international collaboration among Japan, United States and space physicists all over the world.
[PPS08-02] Low electron temperatures observed at Mars by MAVEN on dayside crustal magnetic field lines
*Shotaro Sakai1,2, Thomas E. Cravens3, Laila Andersson4, Christopher M. Fowler5, David L. Mitchell5, Christian Mazelle6, Edward M. B. Thiemann4, David A. Brain4, Kanako Seki1 (1.Graduate School of Science, University of Tokyo, 2.Graduate School of Science, Tohoku University, 3.Department of Physics and Astronomy, University of Kansas, 4.Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, 5.Space Science Laboratory, University of California, Berkeley, 6.IRAP, Université de Toulouse, CNRS, CNES, UPS-OMP)
*Hiromu Nakagawa1, Sonal K Jain2, Nicholas M Schneider2, Franck Montmessin3, Roger V Yelle4, Fayu Jiang4, Loic Verdier3, Takeshi Kuroda1, Nao Yoshida1, Hitoshi Fujiwara5, Takeshi Imamura6, Kaori Terada1, Naoki Terada1, Kanako Seki7, Hannes Groller4, Justin I Deighan2 (1.Planetary Atmosphere Physics Laboratory, Department of Geophysics, Graduate School of Science, Tohoku University, 2.Laboratory for Atmospheric and Space Physics, University of Colorado, 3.Laboratoire Atmosphères, Milieux, Observations Spatiales, 4.Lunar and Planetary Laboratory, University of Arizona, 5.Faculty of Science and Technology, Seikei University, 6.Graduate School of Frontier Sciences, The University of Toky, 7.Graduate School of Science, The University of Tokyo)
*Kazunori Ogohara1 (1.School of Engineering, University of Shiga Prefecture)
*Ann Carine Vandaele1, Frank Daerden1, Ian R. Thomas1, Shohei Aoki1,2, Cédric Depiesse1, Justin T. Erwin1, Lori Neary1, Bojan Ristic1, Yannick Willame1, Jean-Claude Gérard2, Giuliano Liuzzi3, Geronimo Villanueva3, Jon Mason4, Manish R. Patel4, Francesca Altieri5, Giancarlo Bellucci5, Miguel Lopez-Valverde6, Jose-Juan Lopez-Moreno6 (1.Royal Belgian Institute for Space Aeronomy, Brussels, Belgium, 2.Laboratory for Planetary and Atmospheric Physics, University Liège, Belgium, 3.NASA Goddard Space Flight Center, Greenbelt, MD, USA, 4.School of Physical Sciences, The Open University, Milton Keynes, UK, 5.Istituto di Astrofisica e Planetologia Spaziali (IAPS/INAF), Rome, Italy, 6.Instituto de Astrofisica de Andalucia (IAA/CSIC), Granada, Spain )