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Direct numerical simulation of passive scalar in decaying compressible turbulence
Authors:Xinliang?Li  author-information"  >  author-information__contact u-icon-before"  >  mailto:lixl@lnm.imech.an.cn"   title="  lixl@lnm.imech.an.cn"   itemprop="  email"   data-track="  click"   data-track-action="  Email author"   data-track-label="  "  >Email author,Dexun?Fu,Yanwen?Ma
Affiliation:State Key Laboratory of Nonlinear Mechanics, Institute of Mechanics, Chinese Academy of Sciences, Beijing 100080, China
Abstract: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.
Keywords:passive scalar   decaying compressible turbulence   direct numerical simulation.
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