“…Within the mélange zone, the same shear zones may be stacked up by duplex structures to form underplated accretionary complexes (e.g., Hashimoto and Kimura, 1999). The thickness of each horse of ocean floor stratigraphy has been reported to be up to a few hundred meters in the mélange zone focused on in this study Hashimoto and Kimura, 1999;Ikesawa et al, 2005;Hashimoto et al, 2012). Although mélanges have been suggested to be sedimentary, tectonic, and diapiric, most mélange zones in the Shimanto Belt are inferred to be tectonic mélanges (e.g., Kimura and Mukai, 1991;Onishi and Kimura, 1995;Hashimoto and Kimura, 1999), with some exceptions (Osozawa et al, 2009).…”