Dissipation and enstrophy in isotropic turbulence: Resolution effects and scaling in direct numerical simulations
نویسندگان
چکیده
Existing experimental and numerical data suggest that the turbulence energy dissipation and enstrophy i.e., the square of vorticity possess different scaling properties, while available theory suggests that there should be no differences at sufficiently high Reynolds numbers. We have performed a series of direct numerical simulations with up to 20483 grid points where advanced computational power is used to increase the Reynolds number up to 650 on the Taylor scale or to resolve the small scales better down to 1 /4 of a Kolmogorov scale . Our primary goal is to assess the differences and similarities between dissipation and enstrophy. Special attention is paid to the effects of small-scale resolution on the quality and reliability of the data, in view of recent theoretical work V. Yakhot and K. R. Sreenivasan, “Anomalous scaling of structure functions and dynamic constraints on turbulence simulations,” J. Stat. Phys. 121, 823 2005 which stipulates the resolution needed to obtain a moment of a given order. We also provide error estimates as a function of small-scale resolution. Probability density functions of dissipation and enstrophy at high Reynolds number reveal the presence of extreme events several thousands times of the mean. The extreme events in dissipation and enstrophy fields appear to scale alike, substantially overlap in space, and are nearly statistically isotropic, while fluctuations of moderate amplitudes, at least for the present Reynolds numbers, show persistent differences. Conditional sampling shows that intense dissipation is likely to be accompanied by similarly intense enstrophy, but intense enstrophy is not always accompanied by intense dissipation. © 2008 American Institute of Physics. DOI: 10.1063/1.2907227
منابع مشابه
Lognormal turbulence dissipation in global ocean models
Data from turbulent numerical simulations of the global ocean demonstrate that the dissipation of kinetic energy obeys a nearly lognormal distribution at surprisingly large horizontal scales. As the horizontal scales of resolved turbulence are larger than the ocean is deep, the KolmogorovYaglom theory for intermittency in 3D homogeneous, isotropic turbulence cannot apply: instead the downscale ...
متن کاملGeometry of enstrophy and dissipation, grid resolution effects and proximity issues in turbulence
We perform a multi-scale non-local geometrical analysis of the structures extracted from the enstrophy and kinetic energy dissipation-rate, instantaneous fields of a numerical database of incompressible homogeneous isotropic turbulence decaying in time obtained by DNS in a periodic box. Three different resolutions are considered: 256, 512 and 1024 grid points, with kmaxη̄ approximately 1, 2 and ...
متن کاملEvidence for the double cascade scenario in two-dimensional turbulence.
Statistical features of homogeneous, isotropic, two-dimensional turbulence is discussed on the basis of a set of direct numerical simulations up to the unprecedented resolution 32768(2). By forcing the system at intermediate scales, narrow but clear inertial ranges develop both for the inverse and for direct cascades where the two Kolmogorov laws for structure functions are simultaneously obser...
متن کاملThe effect of small-scale forcing on large-scale structures in two-dimensional flows
The effect of small scale forcing on large scale structures in β-plane twodimensional (2D) turbulence is studied using long-term direct numerical simulations (DNS). We find that nonlinear effects remain strong at all times and for all scales and establish an inverse energy cascade that extends to the largest scales available in the system. The large scale flow develops strong spectral anisotrop...
متن کاملRevisiting Batchelor’s theory of two-dimensional turbulence
Recent mathematical results have shown that a central assumption in the theory of two-dimensional turbulence proposed by Batchelor (Phys. Fluids, vol. 12, 1969, p. 233) is false. That theory, which predicts a χ2/3k−1 enstrophy spectrum in the inertial range of freely-decaying turbulence, and which has evidently been successful in describing certain aspects of numerical simulations at high Reyno...
متن کامل