Fig. 7: Representative numerical model of the second-type scenario in Fig. 2 (Run 10, Fig. 6).
From: Horizontally forced initiation of the Izu-Bonin-Mariana subduction zone

a–j Model evolution regarding material, temperature, and velocity fields (Initial condition in Fig. 3). k Volume evolution of scraped slab materials. l Time-space distribution of asthenospheric mantle melts. m Dehydration behaviors of slab materials. Plotting habits are the same as in Fig. 5. A complete evolution of this model is in Supplementary Movie 5.