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130   CHAPTER 6



                             GDH1                PSM                HS

                 (a)
                      3                                                           HS
                                 Depth
                                                                           3
                      4
                   km
                      5                                                    2

                      6                                                    1
                                                                                      PSM  GDH1
                                                                           0

                 (b)
                    150
                                 Heat flow                                        HS  PSM
                   m Wm  2  100                                           .2



                     50                                                   .1
                                                                                          GDH1

                      0                                                    0
                        0            50          100          150                 Misfit
                                           Age (Myr)


           Fig. 6.9  Observed depth and heat flow data for oceanic ridges plotted as a function of lithospheric age, and
           compared to the predictions of three thermal models: HS, half space model; PSM, model of Parsons, Sclater and

           McKenzie; GDH1, global depth and heat flow model of Stein and Stein (redrawn from Stein & Stein, 1996, by permission
           of American Geophysical Union. Copyright © 1996 American Geophysical Union).


                            −1/2
                      q = 510t  for t ≤ 55 Ma           Blanketing by sediment does not appear to be the cause
               and q = 48 + 96exp(−t/36) for t > 55 Ma.  of the low heat flow because the troughs are within the

                                                        least sedimented areas of the ridge and also the young-

             The variation of heat flow with age predicted by all   est and therefore hottest. To explain these phenomena

           three thermal models is illustrated in Fig. 6.9b and com-  it was proposed that the pattern of heat flow is con-
           pared to observed heat flow values. It will be noted that   trolled by the circulation of seawater through the rocks

           observed values for younger lithosphere have not been   of the oceanic crust.
           plotted. This is because there are large variations in the   Although the penetration of water through the hard


           heat flux measured in young oceanic crust (Fig. 6.4).   rock of the sea fl oor at first seems unlikely, it has been
           The values obtained are typically less than those pre-  shown that thermal contraction can induce suffi cient
           dicted by the models and there is now thought to be   permeability for efficient convective flow to exist. The


           good reason for this. In particular, there is a large scatter   cracks are predicted to advance rapidly and cool a large

           in heat flow magnitude near the crests of ocean ridges.   volume of rock in a relatively short time, so that intense
           Thermal lows tend to occur in fl at-floored valleys and   localized sources of heat are produced at the surface.

           highs within areas of rugged topography (Lister, 1980).   Active geothermal systems that are driven by water
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