Energetic electron flux variations of the outer radiation belt during magnetic storms observed by Arase/HEP - Calibration of the instrument using Geant4 and superposed epoch analysis
Inchun Park1, Yoshizumi Miyoshi2, Takefumi Mitani3, Tomoaki Hori4, Takeshi Takashima5, Satoshi Kurita6, Mariko Teramoto7, Nana Higashio5, Iku Shinohara8, Ayako Matsuoka9, Satoshi Kasahara5, Shoichiro Yokota9, Mark Dixon Looper10, J Bernard Blake11, Seth G Claudepierre12 and Shrikanth G Kanekal13, (1)Nagoya University, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (3)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan, (4)ISEE, Nagoya University, Nagoya, Japan, (5)ISAS, JAXA, Sagamihara, Japan, (6)Kyoto University, Research Institute for Sustainable Humanosphere, Kyoto, Japan, (7)Nagoya University, ISEE, Nagoya, Japan, (8)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Kanagawa, Japan, (9)ISAS/JAXA, Sagamihara, Japan, (10)The Aerospace Corp, Los Angeles, United States, (11)The Aerospace Corporation, Space Sciences Department, El Segundo, CA, United States, (12)University of California, Los Angeles, Santa Monica, United States, (13)NASA GSFC, Greenbelt, MD, United States
