Traveling ionospheric disturbances (TIDs) are quasi-periodic variations of ionospheric densities in the Earth's upper atmosphere, believed to be the ionospheric signatures of atmospheric gravity waves (AGWs;Hines, 1960). TIDs are generally categorized as either Large Scale TIDs (LSTIDs, horizontal speeds between 400 and 1,000 m s −1 , periods between 30 min and 3 hr, horizontal wavelengths greater than 1,000 km) or Medium Scale TIDs (MSTIDs, horizontal speeds between 100 and 250 m s −1 , periods between 15 min and 1 hr, and horizontal wavelengths of several hundred km; e.g., Francis, 1975;Georges, 1968;Ogawa et al., 1987). LSTIDs are typically associated with AGWs generated by Joule heating and particle precipitation from auroral zone disturbances (Hunsucker, 1982;Lyons et al., 2019). These AGWs may propagate equatorward for long distances, transporting energy from the auroral zone to middle and low latitudes (Richmond, 1979) and can even reach the opposite hemisphere (Zakharenkova et al., 2016).