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Convective motions as an indicator of solar structure

Published online by Cambridge University Press:  04 August 2017

R. Van der Borght  and
P. Fox
R. Van der Borght
Affiliation:
Monash University, Clayton (Vic.) Australia
P. Fox
Affiliation:
Monash University, Clayton (Vic.) Australia

Extract

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Most stars contain regions which are convectively unstable and one of the more daunting tasks facing astrophysics today is to find a satisfactory theoretical formulation of turbulent energy transport in stars. Various theories have been proposed, such as the mixing-length formalism and its extensions, and it would be most useful if one could test the accuracy of such models in view of their importance in the theory of stellar structure and evolution.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 71 - 74
Copyright
Copyright © Reidel 1984 

References

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