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Reynolds Stresses Derived from Simulations

Published online by Cambridge University Press:  19 July 2016

P. Pulkkinen ,
I. Tuominen ,
A. Brandenburg ,
Å. Nordlund  and
R.F. Stein
P. Pulkkinen
Affiliation:
Dept. of Theoretical Physics, P.O. Box 9, FIN-00014 University of Helsinki, Finland
I. Tuominen
Affiliation:
Observatory and Astrophysics Laboratory, P.O. Box 14, FIN-00014 University of Helsinki, Finland
A. Brandenburg
Affiliation:
NORDITA, Blegdamsvej 17, DK-2100 Copenhagen ⊘, Denmark
Å. Nordlund
Affiliation:
Copenhagen University Observatory, ⊘ster Voldgade 3, DK-1350 Copenhagen K, Denmark
R.F. Stein
Affiliation:
Dept. of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA

Abstract

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Three-dimensional simulations of convection are studied with specific attention to the effects of rotation and latitude on different quantities. The latitude-dependence of the strength of convection is found to decrease with increasing strength of the turbulence. The λ-effect is, however, still present also in a more turbulent case.

Type
3. Numerical Simulations of Convection and Dynamo Processes
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 123 - 127
Copyright
Copyright © Kluwer 1993 

References

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