Relationship between mantle convection currents and plate motions?

Introduction: Plate tectonics has been regarded as a scientific revolution. If so one might argue that it is incomplete. While we have a detailed understanding of how the plates behave, the relationship between plate motions and convection in the mantle is still vigorously debated. This is evident in the ongoing discussion about mantle plumes and hot spot trails. New information from seismic tomography and modeling capacities promise to provide insight in the near future. As we expand our knowledge in science we also expand the boundaries of the unknown. Convection is also a fundamentally important process that controls much of the dynamics of atmospheric, ocean, mantle and outer core systems.

Image to right depicting top to bottom mantle convection from http://geomag.usgs.gov/about.php .

Two basic simple models:

Possible driving forces for plate tectonics:


Basics of mantle convection: flowage in response to buoyancy forces.

Conduction vs. convection vs. advection. Advection is often assumed to be absent in the mantle, but is it? We won't have time to really address that here. Realize that the term advection is used in different ways.

Buoyancy is driven by gravity acting on density contrasts caused by thermal differences and by phase changes. Both are important in earth's mantle.

Importance of Clapeyron slope: For most mineral transformations the transformation pressure increases with increasing T (i.e. a positive Clapeyron slope). This means that in a colder mantle region the transformation can occur at a shallower level and in a hotter region it occurs at a deeper level. We already considered this in the context of the olivine to spinel transition in a subducting slab and the mechanism of trench pull. We can also consider thermal plumes. If there is a density increase in a colder region of convective downwelling, the phase transition will occur at a elevated level producing a negative buoyancy and enhancement of downwelling would be expected. By the same line of reasoning a hot spot a positive bouynacy force would exit. In this case a plume may be self perpetuating once it forms. Which is consistent with the long history of some mantle plumes (see below). In fact you could ask why would a mantle plume ever die? What is the slope for the 670 km, spinel to perovskite boundary?

Mantle viscosity: a most crucial parameter!!

viscosity

Shallow mantle viscosity dominated by olivine rheology.

Mantle material is of varying viscosity: lithosphere vs. asthenosphere, and upper vs. lower mantle. Is there a viscosity contrast across the 370 km phase change boundary?

Estimations of mantle viscosity from glacio-isostatic rebound:

Significance of the Rayleigh number in convection behavior:

Geometries of convection:

Hot spots:

Stratified vs. whole mantle convection:

Model simulations of mantle convection:

Viewing present patterns of convection:

Parting thoughts on the mechanisms:


Some References:


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