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224   CHAPTER 8



           8.3 THE DEEP                                 Brink, 2002). Both gravity data (ten Brink et al., 1993)

                                                        and wide-angle seismic reflection and refraction pro-

           STRUCTURE OF                                 files (DESERT Group, 2004; Mechie  et al., 2005)
                                                        support this conclusion by indicating that the Moho is
                                                        elevated only slightly (<2 km) under the Dead Sea
           CONTINENTAL                                  Basin. These characteristics suggest that, although
                                                        extension influences the surface morphology and

           TRANSFORMS                                   shapes of extensional basins that form along trans-
                                                        forms, it does not play a dominant role in shaping the
                                                        deep structure of the fault system (Section 8.6.2) like
           8.3.1  The Dead Sea Transform                it does in rift basins.

                                                          Seismic reflection and refraction data collected
                                                        across the Arava Fault (Fig. 8.3a) reveal the deep struc-
           The Dead Sea Transform forms part of the Arabia–  ture of the Dead Sea Transform. Beneath the surface
           Nubia plate boundary between the Red Sea and the   trace of the fault, the base of a 17- to 18-km-thick upper
           Bitlis suture zone in eastern Turkey (Fig. 8.3a). The   crust (seismic basement) is vertically offset by 3–5 km
           southern part of this plate boundary provides an impor-  (DESERT Group, 2004; Mechie et al., 2005). The fault
           tant example of a transtensional transform that has   descends vertically into the lower crust where it broad-
                                        −2
           formed in relatively cool (45–53 mW m ), strong conti-  ens downward into a zone of ductile deformation (Fig.
           nental lithosphere (Eckstein & Simmons, 1978; Galanis   8.11). The width of this lower crustal zone is con-
           et al., 1986).                               strained by a  ∼15-km-wide gap in a series of strong
             Since its inception in Middle Miocene times, approxi-  subhorizontal reflectors. These reflectors may repre-


           mately 105 km of left lateral strike-slip motion and ∼4 km   sent either compositional contrasts related to lateral
           of fault-perpendicular extension has occurred within the   displacements within a narrow zone or the effects of
           southern part of the plate boundary (Quennell, 1958;   localized horizontal flow (Al-Zoubi & ten Brink, 2002).

           Garfunkel, 1981). The component of extension was initi-  Below the gap, the Moho displays a small amount of
           ated during the Pliocene (Shamir et al., 2005). Horizontal   topography, suggesting that a narrow zone of deforma-
           velocities derived from GPS data (Section 5.8) suggest   tion beneath the Arava Fault may extend into the
           that relative motion between the Arabian and Nubian   mantle.
                                                   −1
           plates is occurring at the relatively slow rate of 4.3 mm a    These physical characteristics provide important
           (Mahmoud et al., 2005). Most of this motion is accom-  constraints on the dynamics of transform faults. The
           modated by faults that form a series of en echelon   results from the DESERT geophysical survey (DESERT
           step-overs within a narrow, 20- to 40-km-wide transform   Group, 2004; Mechie et al., 2005) suggest that the ∼105 km
           valley (Fig. 8.3a). Rhomb-shaped grabens, elongate pull-  of left lateral displacement between the Arabian and

           apart basins, and steep normal faults have formed where   Nubian plates (Fig. 8.12a) has resulted in a profile with a
           the fault segments step to the left. One of the largest of   significantly different crustal structure east and west of

           these extensional features is the Dead Sea Basin, which   the Arava Fault (Fig. 8.12b). The occurrence of exten-
           is ∼135 km long, 10–20 km wide, and fi lled with at least   sion and transtension between fault segments results in
           8.5 km of sediment (Fig. 8.3b).              localized subsidence and crustal flexure west of the fault

             Superficially the pull-apart basins and normal faults   and a minor, similar deflection of the Moho (Fig. 8.12c).


           along the transtensional Dead Sea Transform resemble   Erosion and sedimentation result in the present day
           features that characterize narrow intracontinental rift   structure of the plate boundary (Fig. 8.12d).
           basins (Section 7.2). Both types of basin typically are
           asymmetric, bounded by border faults, and display
           along-strike segmentations (Lazar et al., 2006). However,   8.3.2  The San Andreas Fault
           there are important differences between the two tec-
           tonic settings. Among the most significant of these is

           that, along transtensional transforms, the extension is   The San Andreas Fault formed in Oligocene times

           confined mostly to the crust and displays minimal   (Atwater, 1970, 1989) when the Pacifi c–Farallon spread-
           involvement of the upper mantle (Al-Zoubi & ten   ing ridge collided with the western margin of North
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