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 Mitani4, Takeshi Takashima5, Nana Higashio5, Satoshi Kasahara5, Shoichiro Yokota6, Shiang-Yu Wang7, Yoichi Kazama7, Kazushi Asamura5, Mariko Teramoto8, Tomoaki Hori9, Kunihiro Keika10, Yoshiya Kasahara11, Shoya Matsuda11, Atsushi Kumamoto12, Fuminori Tsuchiya13, Masafumi Shoji1, Yasunori Tsugawa8, Ayako Matsuoka14 and Jocelyn Chang9, (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, Japan, (5)ISAS, JAXA, Sagamihara, Japan, (6)ISAS/JAXA, Sagamihara, Japan, (7)ASIAA, Taipei, Taiwan, (8)Nagoya University, ISEE, Nagoya, Japan, (9)ISEE, Nagoya University, Nagoya, Japan, (10)University of Tokyo, Graduate School of Science, Bunkyo-ku, Japan, (11)Kanazawa University, Kanazawa, Ishikawa, Japan, (12)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (13)Tohoku University, Sendai, Japan, (14)Kyoto University, Kyoto, Japan
