“…Chorus waves are typically detected in the vicinity of the magnetic equator (|MLAT| < 10°, where MLAT is the magnetic latitude) [ LeDocq et al , ; Santolik et al , ; Li et al , ], which has been recognized as their main source region. It has been widely accepted that chorus waves are excited through linear and nonlinear resonant interactions with hot and anisotropic electrons (tens of keV) injected from the plasma sheet during substorms [ Nunn , ; Karpman et al , ; Omura et al , , ; Shklyar and Matsumoto , ; Li et al , ; Demekhov , ; Omura and Nunn , ; Nunn and Omura , ; Gao et al , ; Nunn and Omura , ]. By considering the relativistic second‐order resonant condition, Omura et al [] found that the evolution of wave frequencies and amplitudes of chorus waves is controlled by the nonlinear resonant current resulting from resonant electron trapping into the effective potential generated by the wave electric field and the mirror force acting together on particles in the inhomogeneous geomagnetic field [see Trakhtengerts et al , ].…”