“…The volume of the entire Apennine crust in Calabria is smaller than the volume of the upper crust that would be involved in the formation of an accretionary prism, assuming that the upper crust had been scraped off during subduction (Doglioni et al, 1999). In general, the compressional structures of both the central and the southern Apennines do not show the thin-skinned geometries typical of subduction-related complexes, but rather they are characterized by a thick-skinned style, typical of ensialic deformations, with basement largely involved in the deformation and with only limited amounts of horizontal shortening (van Dijk et al, 2000;Barchi et al, 2001;Noguera and Rea, 2000;Lavecchia et al, 2003). Tomographic models of the mantle beneath the Apennines and the Tyrrhenian show the presence of a highly discontinuous, intra-asthenosphere, high-velocity body, usually assumed to be the Ionian lithosphere subducted in the course of the Apennine compressional phase, but images a r e v e ry d i f f e r e n t i n l e n g th, position and continuity (Spakman et al, 1993;Cimini and De Gori, 2001;Piromallo and Morelli, 2003;Piromallo and Faccenna, 2004).…”