Very low frequency (VLF) triggered emissions are due to generation of new waves with different frequencies from the VLF radio waves transmitted from the ground station (Helliwell, 1967;Helliwell & Katsufrakis, 1974), which is the manifestation of the nonlinear processes (see reviews by Omura et al., 1991 andGołkowski et al., 2019). The generation of the VLF triggered emissions is controlled by wave-particle interactions in the equatorial magnetosphere when the incident VLF waves propagate along with the geomagnetic field. The wave-particle interaction is also the key driver for generating whistler-mode chorus emissions. Recently, the Demonstration and Science eXperiments (DSX) have been conducted for a study of VLF radio wave transmission from space to space (McCollough et al., 2022;Reid et al., 2022), showing the feasibility and the capability of active experiments in the magnetosphere (McCollough et al., 2022).Whistler-mode chorus emissions are generated near the equator, growing initially with linear growth rates due to the temperature anisotropy of energetic electrons. A coherent wave grows at a fixed frequency up to a certain level of the wave amplitude (Omura & Nunn, 2011), and new wave packets with varying frequencies are formed through nonlinear wave-particle interaction (Hikishima et al., 2009). Therefore, we can regard chorus emissions with frequency variation as emissions triggered by wave packets naturally growing from thermal fluctuations because of an instability driven by temperature anisotropy of energetic electrons.