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 Shinohara3, Ayako Matsuoka8, Satoshi Kasahara5, Shoichiro Yokota8, Mark Dixon Looper9, J Bernard Blake10, Seth G Claudepierre11 and Shrikanth G Kanekal12, (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)ISAS/JAXA, Sagamihara, Japan, (9)The Aerospace Corp, Los Angeles, United States, (10)The Aerospace Corporation, Space Sciences Department, El Segundo, CA, United States, (11)University of California, Los Angeles, Santa Monica, United States, (12)NASA GSFC, Greenbelt, MD, United States
