High-speed solar wind with southward interplanetary magnetic field causes relativistic electron flux enhancement of the outer radiation belt via enhanced condition of whistler waves
Acceleration mechanisms
; Electron acceleration
; High-speed solar wind
; High-speed solar wind streams
; Interplanetary magnetic fields
; Outer radiation belt
; Relativistic electron
; Wave-particle interactions
; Electrons
; Magnetic fields
; Plasma density
; Solar energy
; Solar wind
; Radiation belts
; electron
; interplanetary dust
; magnetic field
; plasma
; solar cycle
; solar wind
Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601, Japan
Recommended Citation:
Miyoshi Y.,Kataoka R.,Kasahara Y.,et al. High-speed solar wind with southward interplanetary magnetic field causes relativistic electron flux enhancement of the outer radiation belt via enhanced condition of whistler waves[J]. Geophysical Research Letters,2013-01-01,40(17).