Fig. 7From: Thermal maturity structures in an accretionary wedge by a numerical simulationA comparison of the numerical model and the natural accretionary wedge. The geological structure (a) and the horizontal profiles of the vitrinite reflectance (b) of the numerical simulation (Fig. 6). Schematic cross-section of the Miura–Boso subduction margin showing maximum paleo-temperatures deduced from the Boso Peninsula (c, d) (modified after Yamamoto et al. 2017)Back to article page