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27. On meridional circulations in stellar convective zones

Published online by Cambridge University Press:  18 July 2016

L. Biermann
L. Biermann*
Affiliation:
Max Planck Institut für Physik, Göttingen, Germany

Abstract

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It is shown in outline by a discussion of the equation of motion in all its components and by taking regard of the geometrical properties of turbulent exchange, that in general the state of pure rotation (without meridional circulations) is not a possible stationary state of motion for convective zones of stars.

Type
Part IV: Solar and Interplanetary Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 6: Electromagnetic Phenomena in Cosmical Physics , 1958 , pp. 248 - 257
Copyright
Copyright © Cambridge University Press 1958 

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