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Reynolds stress models of convection in convective cores

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type , Conference object 01 Aug 2006 English Publisher:Cambridge University Press (CUP)Journal:Proceedings of the International Astronomical Union, volume 2, pages 77-79 (issn: 1743-9213, eissn: 1743-9221, Copyright policy )
Authors: Roxburgh, Ian W.; Kupka, Friedrich;

doi: 10.1017/s1743921307000166

Reynolds stress models of convection in convective cores

Abstract

AbstractWe investigate the properties of non-local Reynolds stress models of turbulent convection in a spherical geometry. Regularity at the centre r=0 places constraints on the behaviour of 3rd order moments. Some of the down-gradient and algebraic closure models have inconsistent behaviour at r=0. A combination of down-gradient and algebraic closures gives a consistent prescription that can be used to model convection in stellar cores.

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Keywords

[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
2
Average
Average
Average
bronze