The height of the ionosphere, which is usually represented by the peak electron density height, shows significant local time, seasonal, and geographic variations, most of which can be empirically well modeled (e.g., Bilitza et al., 2017). In the low-latitude and equatorial region, the ionospheric peak height is significantly influenced by the electric field drift and neutral wind; therefore, it usually serves as a low-latitude ionospheric electrical dynamic indicator (e.g., Kelley, 2009;Yue et al., 2008) and has been frequently used in case studies of ionospheric disturbances (e.g., Batista et al., 2006;X. Chen et al., 2016). The ionospheric height determines the reflection point of the high-frequency radio propagation assisted by the ionosphere over distance. Therefore, further investigations of ionospheric height variability are significant for both ionospheric science and applications.At nighttime, the ionospheric height is mostly dynamically controlled due to the disappearance of solar photoelectronic ionization. Numerous previous investigations have studied the ionospheric uplift during the pre-reversal enhancement (PRE) of E × B drift and associated electron density variations such as the nighttime enhancement (