Atmospheric tides are global-scale atmospheric oscillations. The periods of atmospheric tides are subharmonic and corresponding to solar or lunar days, and the maximum atmospheric tide amplitude in the neutral atmosphere mainly occurs at altitudes ranging between 80 and 150 km (Forbes, 1995). Atmospheric tides can propagate westward or eastward, and several westward propagating atmospheric tides that are synchronized with the motion of the sun or moon are called migrating solar or lunar tides. Since migrating tides are a large component of all atmospheric tides, many studies have focused on their occurrence (Chang et al., 2013;Hagan et al., 1995;Lin et al., 2019). Meanwhile, due to the presence of large vertical wavelengths, atmospheric tides can propagate from the lower atmosphere to the upper atmosphere and easily cause variabilities in the atmosphere. More systematic and detailed descriptions of atmospheric tides have been provided by Forbes (1995), Forbes and Garrett (1979), Lindzen and Chapman (1969), and the references therein.During the annual Northern Hemisphere (NH) winter, a dramatic large-scale meteorological phenomenon referred to as sudden stratospheric warming (SSW) occurs in the winter polar stratospheric region. Current theories mainly suggest that upward propagating quasi-stationary planetary waves (SPWs) play a crucial role in the dynamics of SSWs and that the interaction between quasi-SPWs and mean flow patterns in the stratosphere leads to SSW (Andrews et al., 1987;Butler et al., 2015;Matsuno, 1971). All SSW events are accompanied by substantial changes in both the temperature and horizontal wind components, and the temperature and winds have different changes at different altitudes. SSW can also occur in the Southern Hemisphere (SH) during winter but much less frequently than that during the NH winter due to the smaller SPW amplitudes (