“…Different mélanges and broken formations have been related to tectonic processes that occurred during the evolution of accretionary wedges (Fig. 1), as in the Franciscan Complex and in the Western US Cordillera (e.g., Ernst, 1965;Hsü, 1968;Cowan, 1974Cowan, , 1978Cowan, , 1985Cloos, 1982;Dilek, 1989;Maekawa and Brown, 1991;Dilek and Moores, 1993;Kimura et al, 1996), in Alaska (e.g., Moore and Wheeler, 1978;Orange, 1990;Bradley and Kusky, 1992;Kusky and Bradley, 1999), in Shimanto (e.g., Ditullio and Byrne, 1990;Taira et al, 1992;Kimura, 1997;Ikesawa et al, 2005;Shibata and Hashimoto, 2005), Sambagawa (Takasu et al, 1994), Mino-Tamba-Ashio (Kimura and Hori, 1993) and, Chichibu (Matsuda and Ogawa, 1993;Takahashi, 1999) Belts, the Miura-Bozo accretionary complex (Yamamoto et al, 2009) of Japan and in the Torlesse Group (Esk Head mélange and North Island equivalents, Barnes and Korsch, 1991;Orr et al, 1991;Sunesson, 1993) and the Coastal Range of Hikurangi margin in New Zealand (Pettinga, 1982;Chanier and Ferrière, 1991). Mélanges occur in these places commonly at the base of imbricate thrust sheets (e.g.…”