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SUBDUCTION ZONES  265



              (a) Accretionary forearc


                                                             V   fluid vents
                                 Accretionary
                                   prism                                                 Magmatic front
                              Trench axis  Trench slope  Trench slope  break  Thick forearc basin  Active

                     Trench        basin                                                    arc
                       fill


                                                                            Arc massif
                                Downgoing oceanic crust
                                                                                           Primary partial melts
                   20
                                           Subduction channel
                   10
                                          Lithosphere
                    km  10  30    50
              (b) Non-accretionary forearc

                                                                                        Magmatic  front
                             Exposed basement  Serpentinite                                Active
                   Seamount                   mud volcanoes      Thin forearc basin         arc

                          Empty trench



                                                                                           Primary partial melts
                           Subducted seamount  Downgoing oceanic crust
                   20
                   10

                    km  10  30    50      Lithosphere

                        Partially serpentinized mantle  Basaltic forearc crust  Undeformed sediments

                        Lithospheric mantle           Gabbroic forearc crust   Deformed sediments

            Figure 9.19  Diagrams contrasting the characteristic features of (a) accretionary, and (b) nonaccretionary, convergent
            margins (redrawn from Stern, 2002, by permission of the American Geophysical Union. Copyright © 2002 American

            Geophysical Union). V, fluid vents.



               Seismic reflection data and the ages of deformed   the arc by the addition of new wedges to the toe of the
            sediments suggest that the youngest faults in accretion-  prism. This process, called frontal accretion, causes older
            ary prisms occur at the deformation front and generally   thrusts to become more steeply dipping with time and
            become older away from the trench (Moore et al., 2001,   is responsible for the lateral growth of the prism. Lateral
            2005) (Fig. 9.20b). As shortening occurs, old thrust   growth requires that the most intense deformation
            wedges gradually move upwards and are rotated toward   occurs at the oceanward base of the sedimentary pile,
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