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396   CHAPTER 12



                             N. America                                              South Africa
                (a)                         (b)                       (c)
                                 S. America                Hawaii



           410 discontinuity
           660 discontinuity

           D  discontinuity
                                     D  discontinuity            Large low-velocity
           D  anisotropy
                                     D  anisotropy                   structure
           Low-velocity scatterer    Melt inclusions              D  discontinuity
           Ultralow-velocity         Ultralow-velocity zone    Ultralow-velocity zone
           patches, plume
           genesis                           CMB                       CMB
                                 Underside-CMB sedimentation
           Core–mantle boundary
           (CMB)             Fluid outer core
                   CMB depression,
                 chemical reaction repository
           Figure 12.11  Sections through the Earth’s interior beneath regions centered on (a) central America, (b) Hawaii, and (c)
           South Africa, illustrating variations in the nature of the D″ layer (reproduced from Garnero, 2004, Science 304, 834–6,
           with permission from the AAAS).









           lateral and vertical variations within layer D″ may be
           caused by variations in chemical composition, mineral- 12.9 THE NATURE
           ogic phase changes and/or varying degrees of partial
           melting, in addition to temperature differences. Com- OF CONVECTION IN
           positional variations may be due to the mixing of
           molten iron from the core with the perovskite of the   THE MANTLE
           mantle to form new high-pressure minerals (Section
           2.8.6). It is thought that this is most likely to occur in
           the ULVZs where it is facilitated by higher tempera-

           tures, partial melting, and low viscosity. The result   The evidence for convective flow in the mantle, from
           would be a chemically distinct, high-density layer but   seismic tomography and studies of the regional eleva-
           with a low viscosity. A phase change in perovskite to a   tion and subsidence of the Earth’s surface, strongly
           denser and strongly anisotropic form is an interesting   suggests that there are two main driving forces for this
           possibility as some parts of the D″ layer exhibit a   convection. The negative buoyancy of cold subducting
           marked anisotropy. It is thought that this anisotropy   lithosphere would appear to determine the main sites
           may be induced by subducted slabs beneath down-  of downwelling, and the positive buoyancy of hot, low
           wellings and by shear fl ow beneath upwellings.  viscosity material originating in the lowermost, D″,
             It seems likely that the slabs of subducted lithosphere   layer of the mantle determines the upwellings. These
           that sink into the lower mantle affect the nature of the   two complementary modes of convection in the mantle
           D″ layer beneath them, most notably its temperature.   have been termed the plate and plume modes, respec-
           This in turn will modulate the flow of heat from the   tively (Davies, 1999). Both have their origins in thermal

           core which will influence convection in the core and the   boundary layers: the plate mode in the lithosphere

           nature of the Earth’s magnetic field, and determine   immediately beneath the Earth’s surface, and the plume


           where flow may occur within and above layer D″.  mode in the D″ layer of the mantle, immediately above
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