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Some open questions concerning the modelling of non-locality in Reynolds stress type models of stellar convection.

Published online by Cambridge University Press:  01 August 2006

F. Kupka*
Affiliation:
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany email: fk@mpa-garching.mpg.de
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Abstract

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We discuss some benefits and pitfalls when combining conceptually different types of closure approximations into complete Reynolds stress models of stellar convection.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

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