Journal
PHYSICA D-NONLINEAR PHENOMENA
Volume 241, Issue 3, Pages 164-168Publisher
ELSEVIER
DOI: 10.1016/j.physd.2011.04.015
Keywords
Turbulence; Pressure fluctuations; Numerical simulations
Categories
Funding
- National Science Foundation [CBET-0553867]
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Using data from direct numerical simulations in the Reynolds number range 8 <= R-lambda <= 1000, where R-lambda is the Taylor microscale Reynolds number, we assess the Reynolds number scaling of the microscale and the integral length scale of pressure fluctuations in homogeneous and isotropic turbulence. The root-mean-square (rms) pressure (in kinematic units) is about 0.91 rho u'(2), where u' is the rms velocity in any one direction. The ratio of the pressure microscale to the (longitudinal) velocity Taylor microscale is a constant of about 0.74 for very low Reynolds numbers but increases approximately as 0.17R(lambda)(1/3) at high Reynolds numbers. We discuss these results in the context of the existing theory and provide plausible explanations, based on intermittency, for their observed trends. (C) 2011 Elsevier B.V. All rights reserved.
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