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A note on anisotropic convection and the rotation of stellar convective zones
Authors:Ian W. Roxburgh
Affiliation:(1) Queen Mary College, London, England
Abstract:The interaction of rotation and convection produces a latitude dependent anisotropic turbulent viscosity. When this friction is dominant, equilibrium of a convective outer layer of a star is achieved by an equatorial acceleration and a two-zone circulation, towards the equator at low surface latitudes.
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