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Stellar Convection

Published online by Cambridge University Press:  25 April 2016

Da Run Xiong*
Affiliation:
CCCAT (World Laboratory), PO Box 8730 Beijing 100080, and Purple Mountain Observatory, Nanjing, China

Abstract

Time-dependent convection theory and non-local convection theory are described. The difference between the convection theories results from the different treatment of the non-linear terms of the hydrodynamic equations. We have obtained a better understanding of the thermodynamic coupling between convection and oscillations in comparison to the dynamic coupling.

Type
Invited
Copyright
Copyright © Astronomical Society of Australia 1991

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