Title of article
Computing turbulent flows driven by Rayleigh-Taylor and Richtmyer-Meshkov instabilities
Author/Authors
Zhou، Y. C. نويسنده , , Rubinstein، R. نويسنده , , Eliason، D. نويسنده , , Cabot، W. نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2003
Pages
-378
From page
379
To page
0
Abstract
We develop a two-scale turbulence model for turbulent mix induced by Rayleigh-Taylor and Richtmyer-Meshkov instabilities. In this model, the large scales are dominated by production by instability mechanisms, while small scales satisfy Kolmogorov dynamics. The model allows transfer rates in the two spectral regions to be unequal. Constraints on model coefficients that permit relaxation to a unique self-similar state in free decay and self-similar growth are derived.
Keywords
turbulence , Supernovae , general , instabilities , stars
Journal title
Astronomy and Astrophysics
Serial Year
2003
Journal title
Astronomy and Astrophysics
Record number
76602
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