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THE MECHANISM OF PLATE TECTONICS  397



            the core–mantle boundary. As Davies (1993) has aptly   being entirely passive. Meguin & Romanowicz (2000)
            put it, the plate mode is crucial in cooling the mantle,   and Montelli et al. (2004b) note that there is evidence
            by the creation of oceanic lithosphere, and the plume   in their mantle tomographic models for lateral fl ow in
            mode releases heat from the core. The heat released by   the upper mantle from the African upwelling to the
            the plate mode is thought to be much greater than that   Atlantic and Indian Ocean ridges, and from the Pacifi c

            released from the core as the mantle is heated internally   upwelling to the East Pacific Rise. If so this would com-

            by radioactivity. One might expect therefore that   plete the elusive route of the return flow from sub-
            the plate mode is dominant. These two very different   duction zones to mid-ocean ridges, or at least provide
            modes of convection need not necessarily be strongly   one such route.
            coupled. However it is noteworthy that the two major   The scale, or wavelength, of this gross pattern of
            upwellings at the present day, beneath southern Africa   convection in the mantle is greater than that predicted

            and the south central Pacific, are at the centers of the   by analogue experiments and early numerical models
                                                                                           6
            expanding ring of subduction zones around what was   assuming a Rayleigh number greater than 10 . It tran-
            Gondwana and the contracting ring of subduction   spires that this is because these models assumed uniform
            zones around the Pacific respectively, and hence distant   viscosity throughout the convecting layer. In the Earth’s

            from the cooling effect of the subducting slabs that   mantle the viscosity varies with both temperature
            appear to extend to the core–mantle boundary ((Plate   and pressure. For the relevant temperature gradient in
            12.2 (between pp. 244 and 245), Fig. 12.12). It is also   the mantle the effect of increasing pressure with depth
            striking that these two active upwellings do not corre-  almost certainly means that the viscosity of the

            spond directly to mid-ocean ridges. This is consistent   lower mantle is significantly greater than that of the
            with the interpretation of the upwelling beneath ridges   upper mantle. Bunge  et al.  (1997) investigated three-






                                           E Pacific

                                      MOR
                                                                        MOR



                                                                           African
                                                                           superswell
                            Pacific
                            superswell                Core



                                                                         MOR

                                                                      660 km
                                                                      discontinuity
                                                  W Pacific

            Figure 12.12  Cartoon showing an approximately equatorial section through the Earth and illustrating the
            possible relationship of subduction zones, superswells, plumes, and mid-ocean ridges (MOR) to the gross pattern of
            circulation in the mantle. Note that deep-seated or primary plumes, such as Afar, Reunion, Tristan, Hawaii, Easter, and

            Louisville, are peripheral to the superswells, and that secondary plumes are common above the Pacific superswell. The
            mid-ocean ridges are a passive response to the plate separation and not systematically related to the main convective
            pattern.
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