The understanding of the temporal and spatial evolution of thermospheric neutral species, which act to determine the drag force on space vehicles and debris, is of central importance for geospace environment research (Emmert, 2015; Qian & Solomon, 2012, and references therein). The atomic oxygen (O), molecular oxygen (O 2 ), and molecular nitrogen (N 2 ) are regarded as the thermospheric major species, which control the behavior of the thermosphere. There are, thus, a lot of investigations focused on their characteristics and responses to external forces for several decades (e.g., Meier, 2021;Ren et al., 2020). Recently, observational and simulation studies pointed out that the light species helium (He) can also significantly modulate the variation of thermosphere and its response to geomagnetic storms (Bernstein & Pilinski, 2022;Thayer et al., 2012). The accuracy of thermospheric density predictions was improved via the incorporation of helium in the forecasting model (Kim et al., 2012). In this basis, helium should also be considered as a major part of the thermosphere (Sutton et al., 2015). However, the physical mechanisms that are responsible for the variation of helium in the thermosphere are still primitive owing to the lack of effective measurements and numerical models.Helium is an ideal inert tracer in the thermosphere, because the chemical production and loss of the component are negligible (Kockarts, 1973). As a result, helium behaves differently from other major species in the thermosphere. One of the most significant structures is that helium concentration in winter is higher than that in summer by 1-2 orders of magnitude, termed the winter helium bulge, which was first observed by G. Keating and Prior (1968). Since then, a series of studies devoted on exploring the formation of the anomalous structure and its responses to external forces (e.g.