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THE MECHANISM OF PLATE TECTONICS 385
However, as a result of advances in numerical simula- cooled from above, in which case there is a hot thermal
tions and analogue modeling, and constraints on the boundary layer at its base and a cold thermal bound-
pattern of convection supplied by seismic tomography ary layer at the top (Fig. 12.5a). However, it is possible
and past and present plate motions, it is now possible that one of these boundary layers may be weak or
to derive considerable information on the convective absent. In addition, the fl uid layer may be heated from
process. within (Fig. 12.5b,c). In Fig. 12.5b the lower boundary
Convection in a fluid involves heat transport by layer is missing and the fluid is heated internally. The
motion of the fluid caused by positive or negative cold dense fluid sinking from the top boundary layer
buoyancy of some of the fluid, that is, horizontal drives convection and the upwelling is passive rather
density contrasts or gradients within it. The latter are than buoyant; fluid has to move upwards to create
typically produced by more dense downwellings from space for the sinking cold fluid. The mantle is prob-
a cold boundary layer or less dense upwellings from ably more like Fig. 12.5c in that it is heated from below,
a hot boundary layer, but they may also be of com- by heat flowing from the core, and from within
positional origin. Indeed one tends to think of a con- by radioactivity. In Fig. 12.5 if the temperature of
vecting fluid layer as being heated from below and the lower boundary is fixed in each case then the
(a) COLD Temperature
HOT
(b) COLD Temperature
Internal heating
INSULATING
(c) COLD Temperature
Internal heating
HOT
Figure 12.5 Sketches of convecting fluid layers, and their associated temperature–depth profiles, illustrating the
varying nature of the lower thermal boundary layer depending on the way in which the fluid layer is heated (from
Davies, 1999. Copyright © Cambridge University Press, reproduced with permission).

