Prompt acceleration of relativistic electrons associated with the solar wind pressure pulse: Comparative study between a code-coupling simulation and Arase observations
Yoshizumi Miyoshi1, Shinji Saito2, Takanobu Amano3, Satoshi Kurita4, Kunihiro Keika3, Takeshi Takashima5, Takefumi Mitani6, Mariko Teramoto7, Masafumi Shoji8, Yasunori Tsugawa7, Nana Higashio5, Ayako Matsuoka9, Yoshiya Kasahara10, Syoya Matsuda11, Yasumasa Kasaba12 and Iku Shinohara13, (1)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (2)STEL, Nagoya University, Nagoya, Japan, (3)University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan, (4)Kyoto University, Research Institute for Sustainable Humanosphere, Kyoto, Japan, (5)ISAS, JAXA, Sagamihara, Japan, (6)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan, (7)Nagoya University, ISEE, Nagoya, Japan, (8)ISAS/JAXA, Sagamihara, Japan, (9)Kyoto University, Kyoto, Japan, (10)Kanazawa University, Kanazawa, Ishikawa, Japan, (11)ISAS-JAXA, Sagamihara, Japan, (12)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (13)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Kanagawa, Japan
