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27. On meridional circulations in stellar convective zones
Published online by Cambridge University Press: 18 July 2016
Abstract
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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