Physical regimes and dimensional structure of rotating turbulence

被引:23
作者
Canuto, VM
Dubovikov, MS
机构
[1] NASA Goddard Institute for Space Studies, New York, NY, 10025
关键词
D O I
10.1103/PhysRevLett.78.666
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Numerical simulations of rotating turbulence have given rise to ''unexpected results'': An increasing Omega did not lead to the ''expected'' route to a 2D state. A recent model of turbulence leads to a new number N = K(nu Omega)(-1) (K and nu are turbulent kinetic energy and viscosity) so that DNS (direct numerical simulation) and LES (large eddy simulation) correspond to N < 1 and N > 1. In the first case, the energy cascade is suppressed, while in the second case there exists an inertial spectrum which is an equilibrium of quasi-2D-3D modes. With these ingredients, we reproduce DNS and LES data.
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页码:666 / 669
页数:4
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