Rayleigh and Love wave dispersion curves are known as normal modes and are utilized for inversion. These two waves arrive after the S wave and account for the main energy in all waveforms. However, weaker signals arriving between the P and S waves also have dispersive properties, which are controlled by so-called leaking modes.Studies of leaking mode can be traced back to Somville (1930), who identified and named the PL phase. The PL phase is a train of long-period (>10 s) dispersed waveforms that arrive shortly after the P wave. Oliver and Major (1960) measured PL phase dispersion curves and linked the PL phase with the leaking mode of the crust-mantle waveguide. In addition to the PL phase, some other phases are also considered to have the same wave behavior as the PL phase, which can be explained by the leaking mode (e.g., Pg phase, Shaw & Orcutt, 1984; W phase, Furumura & Kennett, 2018). The leaking mode describes waveguides (leaking waves) whose radiation energy leaks into half-space and phase velocities are higher than the maximum shear velocity (Phinney, 1961). Subsequently, studies have mainly focused on how to calculate leaking modes and simulate leaking waves through leaking modes (e.g., Gilbert, 1964;Haddon, 1984Haddon, , 1986Watson, 1972). However, due to the complexity of leaking modes, limited research has been conducted on imaging underground structures by using the dispersion of leaking waves, and most of the extracted dispersion is below 0.1 Hz for lithospheric research (e.g.,