“…However, basin-scale modeling is also required to get a more regional understanding of fluid migration, and to know both at what time tectonic stress or rising topography of the foothills are likely to have reorganised previous circulation regimes inherited from the former passive margin, and the composition of the circulating fluids (marine fluids versus meteoric water or hydrothermal brines). Numerous papers have described the fluid flow regime associated with dewatering processes in modern accretionary wedges and seismically active areas (Moore et al, 1991;Muir Wood, 1994;Henry, 2000), as well as paleo-fluid flow in Paleozoic and Alpine orogens (Oliver, 1986;Demicco, 1995, 1997;Muchez et al, 1995Muchez et al, , 2000Muchez et al, , 2002Travé et al, 1998Travé et al, , 2000Travé et al, and 2004Roure and Swennen, 2002;Swennen et al, 2003aSwennen et al, , 2004. Numerical simulations have been used recently to account for the topographic gravity driven regional fluid flow currently observed in foreland foldand-thrust belts (Garven, 1985;Ge and Garven, 1989Nesbitt and Muehlenbachs, 1994;Bachu, 1999).…”