As a moon shadow falls on the Earth and quickly sweeps through the atmosphere, it behaves like a ship moving on the ocean, pushing water ahead, and developing waves around. Scientists have speculated the atmospheric bow wave due to a supersonic moon shadow since the 1970s (Chimonas, 1970). A moon shadow skimming over dense ground-based Global Navigation Satellite System (GNSS) arrays developed in recent decades offers a rare opportunity for capturing the waves induced by the changes in solar ionizing radiation. The dense GNSS total electron content (TEC) observations present the substantial evidence of the bow waves and wakes with periods of ten minutes triggered by the supersonic moon shadows over eastern Asia (consist of 1,400s receivers) on July 22, 2009 and over the North America continent (consist of 2,200s receivers) on August 21, 2017. However, the wave behaviors are quite different during the two eclipses. Liu et al. (2011) suggested that atmospheric gravity waves originating from the lower atmosphere due to the supersonic moon shadow of the 2009 eclipse induce the fronts of bow and stern waves and wakes that propagate equatorward and persist near one hour as the moon shadow moves away from the eastern Asia area. On the other hand, the bow wave presents around the time of the maximum obscuration and accompanies with the shadow of the 2017 eclipse that sweeps through the continental United States (CONUS,