Japan Geoscience Union Meeting 2022

Presentation information

[J] Oral

P (Space and Planetary Sciences ) » P-CG Complex & General

[P-CG19] Planetary Magnetosphere, Ionosphere, and Atmosphere

Fri. May 27, 2022 10:45 AM - 12:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Hiroyuki Maezawa(Department of Physical Science Osaka Prefecture University), convener:Naoki Terada(Graduate School of Science, Tohoku University), Kanako Seki(Graduate School of Science, University of Tokyo), convener:Takeshi Imamura(Graduate School of Frontier Sciences, The University of Tokyo), Chairperson:Kazuo Yoshioka(Graduate School of frontier Science, The University of Tokyo), Naoki Terada(Graduate School of Science, Tohoku University)

11:15 AM - 11:30 AM

[PCG19-09] The first simultaneous observation of low energy ions and electrons at Mercury during the first BepiColombo flyby

*Sae Aizawa1,2, Moa Persson1, Nicolas Andre1, Yuki Harada4, Yoshifumi Saito3, Dominique Delcourt5, Lina Z Hadid5, Markus Fraenz8, Shoichiro Yokota7, Andrei Fedorov1, Emmanuel Penou1, Alain Barthe1, Jean Andre Sauvaud1, Bruno Katra5, Shoya Matsuda6, Go Murakami3 (1.Institute de Recherche en Astrophysique et Planetologie, 2.Graduate School of Science, Tohoku University, 3.ISAS/JAXA, 4.Department of Geophysics, Graduate School of Science, Kyoto University, 5.Laboratoire de Physique des Plasmas, CNRS-Observatoire de Paris-Sorbonne Université-Université Paris Saclay-École polytechnique-Institut Polytechnique de Paris, 6.Graduate School of Natural Science and Technology, Kanazawa University, 7.Department of Earth and Space Science, Graduate School of Science, Osaka University, 8.Max-Planck-Institute for Solar System Research)

Keywords:BepiColombo, Mercury's magnetosphere

The first Mercury flyby by BepiColombo was successfully made on 1st of October 2021 and this is the first time to have the simultaneous observation of low energy ions and electrons at Mercury. The data from Mercury Plasma Particle Experiment (MPPE) onboard Mio/BepiColombo shows (1) the compressed Mercury’s magnetosphere compared to the average of MESSENGER observations, (2) boundary motions around magnetopause crossings, (3) low-frequency waves in both dawn and dusk sides, and (4) high energy ions and electrons after the closest approach.