Traveling ionospheric disturbances (TIDs) were discovered long time ago (Hines, 1960;Hooke, 1968). Their propagation leads to variations in the parameters of radio signals propagating in the ionosphere. The TID parameters satisfy the dispersion equation for atmospheric gravity waves (AGWs) in the thermosphere (Hooke, 1977;Gershman et al., 1984;Gossard & Hooke, 1978) and hence TIDs represent the ionospheric plasma response to AGWs. Identification of TIDs with AGWs, in turn, makes possible studying AGWs by means of radio techniques. Traditionally, AGWs are separated into the small-, medium-and large-scale ranges according to horizontal wavelengths of ≤100, 100-1,000, and >1,000 km, respectively (Francis, 1975;Georges, 1968;Hocke & Schlegel, 1996). AGWs may be excited by a wide variety of natural and artificial sources. Some of these sources like earthquakes, volcanic eruptions, cyclones, hurricanes and other meteorological phenomena, powerful explosion and rocket launches (