Large-scale caldera-forming eruptions can occur in time intervals of tens of thousands to hundreds of thousands of years and discharge more than ∼10 km 3 dense rock equivalent (DRE) magmas, severely damaging infrastructure and threatening human populations. Because these eruptions require a substantial volume of accumulated silicic magma in the crust, locating a large eruptible magma body using geophysical techniques such as seismic tomography, magnetotellurics (MT), and gravimetry is fundamentally important for assessing and mitigating the risks of future serious volcanic hazards. In particular, the depth (i.e., pressure) of magma storage is an important factor that affects the growth of eruptible magma chambers (Huber et al., 2019). It can also be a fundamental parameter for modeling and interpreting the surface displacement relevant to the evolution of huge magmatic systems (Townsend, 2022;Wasser et al., 2021;Weber & Castro, 2017). However, geophysical observations fail to detect large melt-dominated magma bodies beneath the active volcanic systems; most of the observed anomalies are interpreted as uneruptible mushy zones with ≤50% melt (Lees, 2007;Pritchard & Gregg, 2016). Advances in understanding the timescale of magma accumulation have shown that the eruptible