“…The origin of neptunian dykes is widely attributed to seismic activity (Playford, 1980;Winterer and Bosellini, 1981;Lehner, 1991;Montenat et al, 1991;Cozzi, 2000), although similar features have also been reported from the surfaces of submarine slides (Winterer et al, 1991;Winterer and Sarti, 1994). The formation of open fissures is related to extension in cohesive or consolidated sediment (Moretti and Sabato, 2007), caused by such factors as a surficial stretching associated with the strain relaxation of fault scarps, slide extension gashes, diapir rising, or overloading (Montenat et al, 2007).…”