Mantle Convection

The Navier–Stokes equation introduced in Chapter 7 provides the basis for understanding the behaviour of mantle convection. Because the mantle is highly viscous, the dominant contributions to the momentum balance come from viscous and buoyancy forces. This means that a scaling analysis from boundary layer theory can be used to compute mantle convection velocities from estimates of mantle viscosity and buoyancy forces. The peculiar geometry, or planform, of mantle convection cells, with subduction zones separated by distances several times the mantle depth, results from a strong increase in mantle viscosity with depth. The internal mantle temperature distribution departs considerably from the adiabat, because the mantle overturns slowly in a time comparable to the internal heat production time scale and the rate of secular cooling. The topography associated with cooling of the oceanic lithosphere and with hot spot swells gives a useful reference to constrain the ratio of internal mantle heating relative to the heat flux coming from the core, although the topography associated with plumes must be corrected for non-adiabatic effects. The Mesozoic and Cenozoic circulation of the mantle can be inferred from plate motion histories, although a limitation is the lack of information on initial conditions. Convective forces We start by providing a simple treatment of convection based on boundary layer theory, and we will see that this provides velocities of the size associated with plate motion (Figure 14.1).