Where is nonlinear growth of whistler-mode chorus waves preferred to occur in the inner magnetosphere?: Coupled MHD and advection simulations
- ADS bibcode
- 2019AGUFMSM51H3273E
- year
- 2019
- Listed Authors
- Ebihara, Y.
- Ikeda, T.
- Omura, Y.
- Tanaka, T.
- Fok, M. C. H.
- Listed Institutions
- Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japan
- Kyoto University, Uji, Japan
- Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Kyoto, Japan
- Kyushu University, Fukuoka, Japan
- Heliophysics Division, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Linked Authors [?]
Linked Institutions