The primary aim of monitoring the geomagnetic field is to study the variations in the Earth's main field (Chapman & Bartels, 1940) and solar activity (Smith et al., 2004; Vassiliadis et al., 1990). When continuous geomagnetic data recorded by magnetometers located within limited areas are examined, synchronous changes with an insignificant time lag in those data are generally interpreted to be the result of global effects dominated by the interaction of variations in the Earth's main field with solar activity on a worldwide scale. However, on a local scale, the geomagnetic field can also be disturbed by ground motion (e.g., Breiner, 1964; Eleman, 1965; Gao et al., 2016; Yamazaki, 2012). Honkura et al. (2004) reported that P-wave arrivals could vary electric and magnetic fields near the surface. Although geomagnetic pulsations can be directly triggered by P waves (e.g., Breiner, 1964; Eleman, 1965; Tsegmed et al., 2000; Yamazaki, 2012), those pulsations are small and close to the amplitude of background noise (Guglielmi et al., 2004). Guglienlmi et al. (2004) recognized magnetic disturbances triggered by Love waves using a polarization method against background noise. On the other hand, disturbances to the geomagnetic field can also be either generated by Rayleigh waves due to ground motion induced by wave arrivals or excited by acoustic waves that are vertically propagating into the atmosphere and changing the electron contents in the ionosphere (Liu et al., 2016; Lognonné et al., 1998; Occhipinti et al., 2010). All the above-mentioned magnetic signals induced by the seismic waves are just local responses and restricted within the passage of the seismic waves. In contrast to the global effect, the geomagnetic changes reported above usually show significant time differences for the related signals retrieved from adjacent stations. The conversion from a seismic wave to a magnetic disturbance can be caused by several mechanoelectric mechanisms. Both theoretical modelings (e.g.