Abstract: Precipitation of radiation belt electrons in a broad energy range from keV to MeV by whistler chorus bursts: Data driven simulation using the ERG plasma wave observations (AGU Fall Meeting 2018)

Precipitation of radiation belt electrons in a broad energy range from keV to MeV by whistler chorus bursts: Data driven simulation using the ERG plasma wave observations

Shinji Saito¹, Yoshizumi Miyoshi², Shoya Matsuda³, Satoshi Kurita⁴, Yoshiya Kasahara⁵, Atsushi Kumamoto⁶, Fuminori Tsuchiya⁶ and Ayako Matsuoka⁷, (1)Nagoya University, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (3)Japan Aerospace Exploration Agency, ISAS, Sagamihara, Japan, (4)Kyoto University, Research Institute for Sustainable Humanosphere, Kyoto, Japan, (5)Kanazawa University, Kanazawa, Ishikawa, Japan, (6)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (7)ISAS/JAXA, Sagamihara, Japan

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