“…The high‐latitude ionosphere (geomagnetic latitudes over ~50°) is a highly dynamic region because of the energetic particle precipitation from the radiation belts and a variety of intense electromagnetic emissions, especially the whistler‐mode waves in the extremely/very low frequency (ELF/VLF) range (e.g., Materassi et al, 2018 ; Parrot et al, 2014, 2016; Santolík et al, 2006). The most common and typical ELF/VLF whistler‐mode waves in the high‐latitude ionosphere include ionospheric hiss waves (Chen et al, 2017; Xia et al, 2019; Zhima et al, 2017), chorus waves (which occasionally appear) (Cao et al, 2005; Parrot et al, 2016; Santolík et al, 2006; Yang et al, 2008; Zhima et al, 2013), and quasiperiodic (QP) waves (e.g., Hayosh et al, 2014, 2013; Němec, Hospodarsky, et al, 2016, Němec, Bezděková, et al, 2016). In this paper, we studied the QP whistler‐mode waves in the ELF/VLF range based on the observations from the China Seismo‐Electromagnetic Satellite (CSES) satellite, which was launched in 2018 at an altitude of 507 km in the upper ionosphere.…”