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Convection in Rotating Stars

Published online by Cambridge University Press:  15 February 2018

F.H. Busse
F.H. Busse*
Affiliation:
University of California, Los Angeles

Summary

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It is shown that many features of convection in rotating spheres and spherical shells can be understood on the basis Of plane layer models. The phenomenon of differential rotation generated by convection is emphasized. The potential applications and limitations of analytical and numerical models for problems of astrophysical interest are briefly discussed.

Type
V. Rotation and Magnetic Fields
Information
International Astronomical Union Colloquium , Volume 38: Problems of Stellar Convection , 1977 , pp. 156 - 175
Copyright
Copyright © 1976

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