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Study of a mathematical model with cylindric symmetry for convection in the upper layers of the mantle

F. Fannucci and S. Santini

Abstract: 

Two-dimensional numerical models of steady state convection show that convection cells of large aspect ratio are possible for variable viscosity convection in the upper mantle. Our model includes the effects of variable viscosity, viscous dissipation, heat flow through the bottom and the adiabatic gradient. The large aspect ratio of the convection cells is primarily due to the large viscosity contrast between the lithosphere and the asthenosphere.