Ionospheric disturbances generated by earthquakes, known as coseismic ionospheric disturbances (CIDs), have been observed after many large earthquakes (Bolt, 1964;Calais & Minster, 1998;Yuen et al., 1969). The amplitudes of small ground vibrations increase thousands of times as they propagate upward to the ionosphere due to the exponential decrease of air density decrease and near conservation of kinetic energy associated with long-period waves (e.g., Ducic et al., 2003;Imtiaz & Marchand, 2012). Perevalova et al. (2014) demonstrated that earthquakes with magnitudes greater than 6.5 can generate observable disturbances in the ionosphere. These signals were first captured by ionosondes after the 1960 Alaskan earthquake. In recent decades, total electron content (TEC) data from dense GNSS networks worldwide have revealed the characteristics of CIDs in detail. Most CIDs have been observed near epicenters (Liu et al., 2017). In the previous CIDs work, the term far-field were commonly used. Here, by far-field CIDs we mean those