“…Generally, the ionospheric response to the solar eclipse is manifested as a decrease in total electron content [ Salah et al , 1986; Jakowski et al , 2008]. When the lunar shadow travels through the atmosphere during a solar eclipse, many other phenomena also have taken place, for instance, the electron density enhancement of ionospheric F 2 layer during the solar eclipse of July 1963 [ Evans , 1965]; the increasing critical frequency of sporadic E layer on the solar eclipse day of June 1955 and July 2009, respectively [ Datta , 1973; Chen et al , 2010]; a short or long time delay of the decline of foF2 responding to the solar eclipse [ Cheng et al , 1992; Adeniyi et al , 2007]; the nighttime‐like quasiperiodic (QP) echoes recorded by the middle and upper atmosphere radar (MU radar) at Shigaraki during a partial solar eclipse [ Thampi et al , 2010]; the periodic modulation of the ionospheric electron density and Doppler echoes reflected from ionosphere [ Hanuise et al , 1982; Altadill and Solé , 2001; Jones et al , 2004; Jakowski et al , 2008]. The gravity waves produced by a solar eclipse may be responsible for most of these phenomena.…”