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                    40  CHAPTER 3



                                                              crust to a height z  and held open by a pressure
                          0        1000                                     magma
                                                              in its source region in excess of the local lithostatic
                               km                             pressure by an amount ∆P is given by
                                                                                   d
                                                              W = [(1 − ν)/µ]z magma  {∆P d
                                                                  + [z magma  g (ρ magma  − ρ crust )/π]}  (3.5)
                      North
                     America
                                                              where  ν and  µ are  Poisson’s ratio and  shear
                                                              modulus, respectively, two of the elastic propert-
                                                              ies of the host rocks. ∆P is the pressure at the inlet
                                                                                 d
                                                              to the dike at the base of the crust, and so the buoy-
                                                              ancy of all of the vertical extent H of the plume
                                              Africa
                                                              head providing magma contributes to this pressure,
                                                              i.e., in this case

                                                              ∆P =∆ρ gH                            (3.6)
                                                                 d    m
                                                                Table 3.2 shows the average widths of the dikes
                                                              that would contain the magma columns listed in
                                                              Table 3.1; the range, of order 100–200 m, seems
                                                              to be quite consistent with the field observations.
                                                              The great widths of these dikes means that magma
                                        South America
                                                              may flow through them very easily at relatively high
                                                              speed. This is probably directly linked to the forma-
                  Fig. 3.6 A reconstruction of the North American, South  tion of very large volume flood basalt flow fields
                  American and African plates as the Atlantic was opening.  on the continents and large igneous provinces on
                  Giant dike swarms radiated out from a hot spot, the position
                                                              the ocean floors.
                  of which is indicated by the star. Although they are present
                  on now widely separated continents, these dikes have
                  essentially identical compositions and emplacement ages,
                  confirming their common origin before the Atlantic formed.  3.7 Summary

                  (Adapted from fig. 6 published in Earth Science Reviews,
                  Vol. 39, Ernst, R.E., Head, J.W., Parfitt, E.A., Grosfils, E. &  • When a new convection cell forms in the mantle,
                  Wilson, L., Giant radiating dike swarms on Earth and Venus,  its rising upper part, a mantle plume, undergoes
                  1–58, copyright Elsevier (1995).)
                                                                partial melting due to the pressure reduction, and
                                                                the resulting body of low-density melt mixed with
                  only simple explanation of the sizes and geometr-  the residual solids constitutes a buoyant diapir
                  ies of these dikes is that they grow from very large  rising through the surrounding mantle rocks.
                  reservoirs of magma that have been extracted from  These rocks, although solid, act as a very viscous
                  the mantle but then trapped at or near the base of  fluid on the long time scales and slow defor-
                  the crust. Detailed measurements of the fabric and  mation rates involved.
                  magnetization of the dike rocks show that growth is  • In a similar way, melting due to the temperature
                  mainly upward immediately above and near to the  rise as wet sediments and ocean floor rocks are
                  reservoir, and mainly lateral in the more distant  carried down in a subduction zone can also
                  parts of the swarm.                           create a region of lower-density partial melt that
                    Are the widths of these giant dikes consistent  then forms a slowly rising diapir. Subduction
                  with what we would expect? The average width W  zone diapirs are expected to be much smaller
                  of a dike extending from the base of the continental  than mantle plume diapirs.
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