Where is nonlinear growth of whistler-mode chorus waves preferred to occur in the inner magnetosphere?: Coupled MHD and advection simulations

Yusuke Ebihara1, Takuya Ikeda2, Yoshiharu Omura1, Takashi Tanaka3 and Mei-Ching Hannah Fok4, (1)Kyoto University, Research Institute for Sustainable Humanosphere, Kyoto, Japan, (2)Kyoto University, Uji, Japan, (3)Kyushu University, Fukuoka, Japan, (4)NASA Goddard Space Flight Center, Heliophysics Division, Greenbelt, MD, United States