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SUBDUCTION ZONES  269



                              (a)  3

                                  4           Accreted sediment      Décollement
                                                  0.40
                                 Depth (km)  5  0.60
                                  6
                                  7      0.80  Underthrust sediment  Surface slope
                                  8                        Taper angle  Subduction angle

                                     50     40     30     20      10     0
                                         Distance arcward from the deformation front (km)
                              (b)
                                            Well drained:         Poorly drained:
                                             Rapid fluid escape   Retarded fluid escape
                                             Low pore pressures   Elevated pore
                                                                  pressures

                                                 Wedge steepens       Wedge remains
                                     TIME                             shallow

                                             Steep stable geometry  Shallow stable geometry
                                                   Strong base           Weak base






            Figure 9.22  (a) Schematic view of a numerical model of fluid flow within an accretionary prism and (b) cross-sections

            showing relationships between factors influencing accretionary wedge taper angle (modified from Saffer & Bekins,

            2002, with permission from the Geological Society of America). Arrows in (a) represent approximate sediment velocities
            at the deformation front. Shading shows generalized porosity distribution, contours are modeled steady-state pore
            pressures (l).

            the deforming wedge, are greatly influenced by factors   wedges (Saffer & Bekins, 2006). Thick sedimentary sec-
            such as the convergence rate and the stratigraphy, lithol-  tions give rise to large prisms that are able to sustain

            ogy, mineralogy, and hydrologic properties of the   high pore fluid pressures and low stable taper angles
            incoming sediments (Saffer, 2003).           (Fig. 9.23a). The results also suggest that prisms com-
               The sensitivity of accretionary prisms to fl uctua-  posed mostly of low permeability fi ne-grained  sedi-
            tions in fl uid  flow and pore fluid pressure has been   ment, such as northern Antilles (Barbados) and eastern


            explored in detail using mechanical and numerical   Nankai (Ashizuri), will exhibit thin taper angles and
            models. By combining a model of groundwater fl ow   those characterized by a high proportion of high per-
            with critical taper theory (Fig. 9.22a), Saffer & Bekins   meability turbidites, such as Cascadia, Chile, and
            (2002) concluded that low permeability, high pore pres-  México, will have steep taper angles (Fig. 9.23b). This
            sure, and rapid convergence rates sustain poorly drained   sensitivity to the physical properties of accreted and
            systems and result in shallow tapers, whereas high per-  subducted sediment implies that any along-strike varia-
            meability, low pore pressure, and slow convergence   tion in sediment lithology or thickness strongly infl u-
            result in well-drained systems and steep taper geome-  ences the geometry and mechanical behavior of
            tries (Fig. 9.22b). These authors also showed that the   accretionary prisms. Similarly, any variation in incom-
            stratigraphic thickness and composition of the sedi-  ing sediment thickness or composition over time will
            ment that is incorporated into the wedge are among the   force the accretionary complex to readjust until a new

            most important factors governing pore fluid pressure in   dynamic balance is reached.
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