Direct numerical simulation of passive scalar in decaying compressible turbulence
Direct numerical simulation of passive scalar in decaying compressible turbulence
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DOI:
10.1360/03yw0029
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发表时间:
2004-01
期刊:
影响因子:
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通讯作者:
Xinliang Li;D. Fu;Yanwen Ma
中科院分区:
文献类型:
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作者:
Xinliang Li;D. Fu;Yanwen Ma
The passive scalars in the decaying compressible turbulence with the initial Reynolds number (defined by Taylor scale and RMS velocity) Re=72, the initial turbulent Mach numbers (defined by RMS velocity and mean sound speed) Mt=0.2–0.9, and the Schmidt numbers of passive scalar Sc=2–10 are numerically simulated by using a 7th order upwind difference scheme and 8th order group velocity control scheme. The computed results are validated with different numerical methods and different mesh sizes. The Batchelor scaling withk−1 range is found in scalar spectra. The passive scalar spectra decay faster with the increasing turbulent Mach number. The extended self-similarity (ESS) is found in the passive scalar of compressible turbulence.