Flux evolution of relativistic electrons of the outer radiation belt associated with coronal hole streams: Arase observations
Yoshizumi Miyoshi1, Satoshi Kurita2, Ryuho Kataoka3, Iku Shinohara4, Takefumi Mitani5, Takeshi Takashima6, Nana Higashio6, Satoshi Kasahara6, Shoichiro Yokota7, Shiang-Yu Wang8, Yoichi Kazama8, Kazushi Asamura6, Mariko Teramoto9, Tomoaki Hori10, Kunihiro Keika11, Yoshiya Kasahara12, Shoya Matsuda12, Atsushi Kumamoto13, Fuminori Tsuchiya13, Masafumi Shoji1, Yasunori Tsugawa9, Ayako Matsuoka14 and Jocelyn Chang10, (1)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (2)Nagoya University, Nagoya, Japan, (3)NIPR National Institute of Polar Research, Tokyo, Japan, (4)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Kanagawa, Japan, (5)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan, (6)ISAS, JAXA, Sagamihara, Japan, (7)ISAS/JAXA, Sagamihara, Japan, (8)ASIAA, Taipei, Taiwan, (9)Nagoya University, ISEE, Nagoya, Japan, (10)ISEE, Nagoya University, Nagoya, Japan, (11)University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan, (12)Kanazawa University, Kanazawa, Ishikawa, Japan, (13)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (14)Kyoto University, Kyoto, Japan
