NASA NTRS · 19850041032
Analytical model for large-scale turbulence
Abstract
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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Canuto, V. M., Goldman, I.. 1985-02-04. Analytical model for large-scale turbulence. https://ntrs.nasa.gov/citations/19850041032
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