Page 197 - Global Tectonics
P. 197

CONTINENTAL RIFTS AND RIFTED MARGINS  183



               Models of continental extension that emphasize   crustal buoyancy force are important at low strain rates,

            crustal buoyancy forces incorporate the effects of ductile   when thermal diffusion is relatively efficient (e.g. Fig.

            flow in the lower crust. Buck (1991) and Hopper & Buck   7.22h–j), and after long (>30 Myr) periods of time. In
            (1996) showed that the pressure difference between   addition, thermal buoyancy forces may dominate over
            areas inside and outside a rift could cause the lower crust   crustal buoyancy forces immediately after rifting when

            to flow into the zone of thinning if the crust is thick and   strain magnitudes are relatively low. This latter effect

            hot. Efficient lateral flow in a thick, hot, and weak lower   occurs because variations in crustal thicknesses are rela-

            crust works against crustal buoyancy forces by relieving   tively small at low stretching (β) factors. This study, and
            the stresses that arise from variations in crustal thick-  the work of Buck (1991) and Hopper & Buck (1996),
            ness. This effect may explain why the present depth of   suggests that shifts in the mode of extension are
            the Moho in some parts of the Basin and Range Prov-  expected as continental rifts evolve through time and
            ince, and therefore crustal thickness, remains fairly   the balance of thermal and crustal forces within the
            uniform despite the variable amounts of extension   lithosphere changes.
            observed in the upper crust (Section 7.3). In cases where
            low yield strengths and flow in the lower crust alleviate


            the effects of crustal buoyancy, the zone of crustal thin-  7.6.4 Lithospheric flexure
            ning can remain fixed as high strains build up near the

            surface. Buck (1991) and Hopper & Buck (1996) defi ned   Border faults that bound asymmetric rift basins with
            this latter style of deformation as core complex-mode   uplifted flanks are among the most common features in


            extension (Fig. 7.24c). Studies of flow patterns in ancient   continental rifts (Fig. 7.25). Some aspects of this char-
            lower crust exposed in metamorphic core complexes   acteristic morphology can be explained by the elastic
            (e.g. Klepeis et al., 2007) support this view.  response of the lithosphere to regional loads caused by
               The relative magnitudes of the thermal and crustal   normal faulting.

            buoyancy forces may be affected by two other param-  Plate flexure (Section 2.11.4) describes how the
                                                                                        5
            eters: strain rate and strain magnitude. Davis & Kusznir   lithosphere responds to long-term (>10  years) geo-
            (2002) showed that the strain delocalizing effects of the   logic loads. By comparing the flexure in the vicinity of

                            (a)                      Basin width
                                4    Rift flank uplift
                                   A                                             A
                              km  0

                               6





                            (b)
                                  A          flank  10– 100 km                   A
                                             Uplifted  10–60 km



                                                                         Monocline
                                                                         Border fault


            Figure 7.25  Generalized form of an asymmetric rift basin showing border fault in (a) cross-section and (b) plan view
            (after Ebinger et al., 1999, with permission from the Royal Society of London). Line of section (A–A′) shown in (b).
            Shading in (b) shows areas of depression.
   192   193   194   195   196   197   198   199   200   201   202