For thick rotating spherical shells and large Prandtl numbers, no-slip outer boundaries lower the critical Rayleigh number relative to stress-free boundaries, and internal heating moves onset away from the tangent cylinder.
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Influence of Boundary Conditions and Heating Modes on the Onset of Columnar Convection in Rotating Spherical Shells
For thick rotating spherical shells and large Prandtl numbers, no-slip outer boundaries lower the critical Rayleigh number relative to stress-free boundaries, and internal heating moves onset away from the tangent cylinder.