Plasma pressure distribution of ions and electrons in the inner magnetosphere during CIR and CME driven storms observed by Arase satellite
Plasma pressure distribution of ions and electrons in the inner magnetosphere during CIR and CME driven storms observed by Arase satellite
Sandeep Kumar1, Yoshizumi Miyoshi2, Vania K Jordanova3, Lynn M Kistler4, Shreedevi Porunakatu Radhakrishna5, Kazushi Asamura6, Shoichiro Yokota7, Satoshi Kasahara6, Yoichi Kazama8, S. Y. Wang8, Sunny W. Y. Tam9, Takefumi Mitani10, Nana Higashio11, Kunihiro Keika12, Inchun Park13, Tomoaki Hori14, Chae Woo Jun15, Ayako Matsuoka16, Shun Imajo16 and Iku Shinohara17, (1)Nagoya University, ISEE, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research (ISEE), Nagoya, Japan, (3)Los Alamos National Laboratory, Los Alamos, NM, United States, (4)Univ New Hampshire, Durham, NH, United States, (5)Nagoya University, Institute for Space Earth Environment Research, Nagoya, Japan, (6)ISAS/JAXA, Sagamihara, Japan, (7)Osaka University, Osaka, Japan, (8)ASIAA, Taipei, Taiwan, (9)National Cheng Kung University, Tainan, Taiwan, (10)Japan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical Science (ISAS), Sagamihara, Japan, (11)JAXA, Tukuba, Japan, (12)University of Tokyo, Department of Earth and Planetary Science, Bunkyo-ku, Japan, (13)Nagoya University, Nagoya, Japan, (14)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (15)ISEE, Nagoya University, Nagoya, Japan, (16)Kyoto University, Kyoto, Japan, (17)Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan