Analytical model for large-scale turbulence

Details Analytical model for large-scale turbulence Analytical model for large-scale turbulence

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..54..430c&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 54, Feb. 4, 1985, p. 430-433.

Astronomy and Astrophysics

Astrophysics

44

Astrophysics, Convection, Turbulence, Turbulence Models, Closure Law, Mixing Length Flow Theory, Stellar Models

Scientific paper

The paper presents an analytical model for large-scale turbulence, based on a new closure which depends on the growth rate of the instability-generating turbulence. For convection in stars the results of the mixing-length theory are recovered, and for laboratory convection the N = R to the 1/3 power law is recovered. The present model can readily be extended to include magnetic fields and rotation.

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