Intermittency of turbulent velocity and scalar fields using 3D local averaging

Abstract

An efficient approach for extracting 3D local averages in spherical subdomains is proposed and applied to study the intermittency of small-scale velocity and scalar fields in direct numerical simulations of isotropic turbulence. We focus on the inertial-range scaling exponents of locally averaged energy dissipation rate, enstrophy and scalar dissipation rate corresponding to the mixing of a passive scalar $\theta$ in the presence of a uniform mean gradient. The Taylor-scale Reynolds number $R_{\lambda }$ goes up to $1300$, and the Schmidt number $Sc$ up to $512$ (albeit at smaller $R_{\lambda }$). The intermittency exponent of the energy dissipation rate is $\mu \approx 0.23$, whereas that of enstrophy is slightly larger; trends with $R_{\lambda }$ suggest that this will be the case even at extremely large $R_{\lambda }$. The intermittency exponent of the scalar dissipation rate is ${\mu }_{\theta }\approx 0.35$ for $Sc=1$. These findings are in essential agreement with previously reported results in the literature. We further show that ${\mu }_{\theta }$ decreases monotonically with increasing $Sc$, either as $1/\log Sc$ or a weak power law, suggesting that ${\mu }_{\theta }\to 0$ as $Sc\to \infty$, reaffirming recent results on the breakdown of scalar dissipation anomaly in this limit.

7 pages, 5 figures

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• Universality of extreme events in turbulent flows
• Comparing velocity and passive scalar statistics in fluid turbulence at high Schmidt numbers and Reynolds numbers
• The spatio-temporal statistical structure of the turbulent dissipation field and its stochastic representation as a Gaussian Multiplicative Chaos