Turbulence and laminar structures: can they co-exist?

被引:9
|
作者
Canuto, VM
机构
[1] NASA, Goddard Inst Space Studies, New York, NY 10025 USA
[2] Columbia Univ, Dept Appl Math & Phys, New York, NY 10027 USA
关键词
turbulence;
D O I
10.1046/j.1365-8711.2000.03786.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Schwarzschild first suggested that the laminar structures observed in the high Reynolds number Re = UL/nu approximate to O (10(12)) solar photosphere are the result of turbulence rather than a proof of its absence. He reasoned that, since turbulence generates large turbulent viscosities nu(t) much greater than nu, the 'effective' Reynolds number Re = UL/nu(t) approximate to O(1). Schwarzschild's argument is, however, incomplete, for it assumes that the entire role of the non-linear interactions is to 'enhance' viscosity. While this is not true in general, we present a proof of how and why it may occur, thus completing Schwarzschild's argument. We further discuss the fact that the same non-local turbulence models reproduce Large Eddy Simulation (LES) data for a variety of flows pertaining to astrophysics, geophysics and laboratory situations (in a fraction of the time).
引用
收藏
页码:985 / 988
页数:4
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