Whistler mode chorus waves are bursty electromagnetic emissions that are often observed as the lower band mode below half of the electron cyclotron frequency f ce and/or the upper band mode between 0.5f ce and 1.0f ce . The Earth's magnetosphere naturally generates the whistler chorus with the injection of several tens of keV electrons associated with substorms (e.g., Miyoshi et al., 2003Miyoshi et al., , 2013Tsurutani & Smith, 1977). The whistler chorus waves play an important role in accelerating energetic electrons over a wide energy range from keV to MeV order through Doppler-shifted cyclotron resonance (Horne & Thorne, 2003). Cyclotron resonant interactions result in the pitch angle and energy diffusion of electrons bouncing along a magnetic field line, and more energetic electrons can resonate with chorus waves at higher magnetic latitudes. A quasi-linear theory, which assumes the resonant interactions by incoherent, broadband, and small-amplitude