According to the Chapman theory (Rishbeth & Garriott, 1969), the plasma density of the ionosphere is expected to continuously increase after sunrise under the control of continuously enhancing photoionization production until local noon. However, various sources from the solar, geomagnetic, or meteorological activities can significantly influence the plasma density via modulating the production, recombination, and transportation processes. The complex interplay among multiple drivers can result in either enhancements or depressions of ionization to varying degrees over different regions. Thus, instead of a continuously enhancing ionization, the plasma density of the daytime ionosphere may also undergo remarkable depletions, especially under geomagnetic disturbed conditions.During severe geomagnetic storms, significant plasma density depletions were frequently detected and termed as negative storm effects (Prölss, 2008, and the references therein). The duration of the storm-time plasma density depletion can vary from several hours to a few days and can be observed over wide longitude and latitude regions