A statistical study of the behaviors of energetic ions (H+, He+, and O+) in the inner magnetosphere using the Arase satellite observations

Chae Woo Jun1, Yoshizumi Miyoshi2, Tomoaki Hori3, Satoko Nakamura4, Masafumi Shoji1, Sandeep Kumar3, Lynn M Kistler5, Chao Yue6, Jacob Bortnik7, Larry R Lyons8, Kazushi Asamura9, Shoichiro Yokota10, Satoshi Kasahara9, Kunihiro Keika11, Iku Shinohara9 and A Matsuoka12, (1)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research (ISEE), Nagoya, Japan, (3)ISEE, Nagoya University, Nagoya, Japan, (4)Kyoto University, Graduate School of Science, Kyoto, Japan, (5)Univ New Hampshire, Durham, NH, United States, (6)Peking University, Institute of space physics and applied technology, Beijing, China, (7)University of California Los Angeles, Atmospheric and Oceanic Sciences, Los Angeles, United States, (8)University of California Los Angeles, Department of Atmospheric and Oceanic Sciences, Los Angeles, CA, United States, (9)ISAS/JAXA, Sagamihara, Japan, (10)Osaka University, Osaka, Japan, (11)University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan, (12)Kyoto University, Kyoto, Japan