The effects of rotation on the global dynamics of turbulent convection

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Convection, Rotation, Turbulence

Scientific paper

3D numerical simulations of incompressible thermal convection in the presence of rotation have shown both a marked difference from (vortical plume interactions, mean thermal gradients, Ekman pumping, {\it etc}) and similarity to (boundary dependent hard- and soft-turbulent heat-transport scalings) its non-rotating counterpart. An understanding of these results should aid the development of proper parameterizations for solar structure and stellar evolution models.

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