Dissipation range of the energy spectrum in high Reynolds number turbulence
arXiv:2004.06274 · doi:10.1103/PhysRevFluids.5.092601
Abstract
We seek to understand the kinetic energy spectrum in the dissipation range of fully developed turbulence. The data are obtained by direct numerical simulations (DNS) of forced Navier-Stokes equations in a periodic domain, for Taylor-scale Reynolds numbers up to , with excellent small-scale resolution of for all cases (and additionally at with ), where is the maximum resolved wavenumber and is the Kolmogorov length scale. We find that, for a limited range of wavenumbers past the bottleneck in the range , the spectra for all display a universal stretched exponential behavior of the form , in rough accordance with recent theoretical predictions. The stretched exponential fit in the near dissipation range does not possess a unique exponent, which decreases with increasing . This region can be regarded as a crossover between the stretched exponential behavior and the far dissipation range , in which analytical arguments as well as DNS data with superfine resolution (S. Khurshid et al., Phys.~Rev.~Fluids 3, 082601, 2018) suggest a dependence. We remark on the connection to the multifractal model which hypothesizes a pseudo-algebraic law.
6 pages, 4 figures
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