Direct Numerical Simulation of Passive Scalar in Decaying Compressible Turbulence
Li XL(李新亮); Fu DX(傅德薰); Ma YW(马延文)
刊名Science in China Series G-Physics Astronomy
2004
通讯作者邮箱lixl@lnm.imech.ac.cn
卷号47期号:1页码:52-63
ISSN号1672-1799
通讯作者Li, XL (reprint author), Chinese Acad Sci, Inst Mech, State Key Nonlinear Mech, Beijing 100080, Peoples R China.
中文摘要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 with k(-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.
学科主题力学
类目[WOS]Physics, Multidisciplinary
研究领域[WOS]Physics
收录类别SCI ; EI
语种英语
WOS记录号WOS:000188945900007
公开日期2007-06-15 ; 2007-12-05 ; 2009-06-23
内容类型期刊论文
源URL[http://dspace.imech.ac.cn/handle/311007/16345]  
专题力学研究所_力学所知识产出(1956-2008)
推荐引用方式
GB/T 7714
Li XL,Fu DX,Ma YW. Direct Numerical Simulation of Passive Scalar in Decaying Compressible Turbulence[J]. Science in China Series G-Physics Astronomy,2004,47(1):52-63.
APA 李新亮,傅德薰,&马延文.(2004).Direct Numerical Simulation of Passive Scalar in Decaying Compressible Turbulence.Science in China Series G-Physics Astronomy,47(1),52-63.
MLA 李新亮,et al."Direct Numerical Simulation of Passive Scalar in Decaying Compressible Turbulence".Science in China Series G-Physics Astronomy 47.1(2004):52-63.
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