Whistler-mode waves are one of the most common plasma waves in the Earth's inner magnetosphere (Burtis & Helliwell, 1969;Tsurutani & Smith, 1974, 1977W. Li et al., 2009), which usually regulate the energetic electron distributions by wave-particle interactions. On the other hand, the modified electron distributions can affect wave evolution. To name a few, nonparallel whistler waves can interact with the energetic electrons through Landau resonance to form a plateau in the parallel velocity distribution, which may play a key role in forming the wellknown 0.5 𝐴𝐴 𝐴𝐴𝑐𝑐𝑐𝑐 ( 𝐴𝐴 𝐴𝐴𝑐𝑐𝑐𝑐 is the equatorial electron gyrofrequency) power gap of whistler-mode chorus waves (Chen et al., 2021;. This electron distribution is also conducive to the generation and propagation of highly oblique whistler waves (Ma et al., 2017;Mourenas et al., 2015;. Besides, whistler waves can modify the electron phase space distribution, and the resultant phase space structures such as phase space holes potentially produce nonlinear wave structures, like Langmuir waves, bipolar and unipolar electric fields (An et al., 2019).Therefore, how whistler waves affect the energetic electron distributions in the Earth's inner magnetosphere has been an important and attractive topic. Previous studies have shown that whistler waves, as well as magnetosonic waves, can cause the gradual formation of electron butterfly distributions on a time scale from hours to days via quasi-linear diffusion processes (