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Large Scale Convection in Stars : Towards a Model for the Action of Coherent Structures
Published online by Cambridge University Press: 12 April 2016
Abstract
We show that, representing the descending fluid in a convection zone by a porous medium, the differential rotation of the (rising) fluid is very close to that in an axisymmetric model of the convection zone with anisotropic viscosity.
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- Part I Convection and turbulence as the basis of magnetic activity
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- Copyright © Springer-Verlag 1991