A Kolmogorov-like exact relation for compressible polytropic turbulence

被引:39
作者
Banerjee, Supratik [1 ]
Galtier, Sbastien
机构
[1] Univ Paris Sud, Inst Astrophys Spatiale, F-91405 Orsay, France
关键词
compressible turbulence; homogeneous turbulence; turbulence theory; DENSITY POWER SPECTRUM; SOLAR-WIND; INTERSTELLAR TURBULENCE; THERMAL-INSTABILITY; MODEL; SIMULATIONS; DISSIPATION; STATISTICS; CASCADE; FLOWS;
D O I
10.1017/jfm.2013.657
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Compressible hydrodynamic turbulence is studied under the assumption of a polytropic closure. Following Kolmogorov, we derive an exact relation for some two-point correlation functions in the asymptotic limit of a high Reynolds number. The inertial range is characterized by: (i) a flux term implying in particular the enthalpy; and (ii) a purely compressible term l which may act as a source or a sink for the mean energy transfer rate. At subsonic scales, we predict dimensionally that the isotropic k(-513) energy spectrum for the density-weighted velocity field (rho(1/3)nu), previously obtained for isothermal turbulence, is modified by a polytropic contribution, whereas at supersonic scales 9 may impose another scaling depending on the polytropic index. In both cases, it is shown that the fluctuating sound speed is a key ingredient for understanding polytropic compressible turbulence.
引用
收藏
页码:230 / 242
页数:13
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