Turbulence is an ineffective mixer when Schmidt numbers are large

Abstract

We solve the advection-diffusion equation for a stochastically stationary passive scalar $\theta$, in conjunction with forced 3D Navier-Stokes equations, using direct numerical simulations in periodic domains of various sizes, the largest being $8192^3$. The Taylor-scale Reynolds number varies in the range $140-650$ and the Schmidt number $Sc\equiv \nu /D$ in the range $1-512$, where $\nu$ is the kinematic viscosity of the fluid and $D$ is the molecular diffusivity of $\theta$. Our results show that turbulence becomes an ineffective mixer when $Sc$ is large. First, the mean scalar dissipation rate $⟨\chi ⟩=2D⟨|\nabla \theta {|}^2⟩$, when suitably non-dimensionalized, decreases as $1/\log Sc$. Second, 1D cuts through the scalar field indicate increasing density of sharp fronts on larger scales, oscillating with large excursions leading to reduced mixing, and additionally suggesting weakening of scalar variance flux across the scales. The scaling exponents of the scalar structure functions in the inertial-convective range appear to saturate with respect to the moment order and the saturation exponent approaches unity as $Sc$ increases, qualitatively consistent with 1D cuts of the scalar.

5 pages, 6 figures

References in corpus (4)

• Burgers Turbulence
• Vortex stretching and enstrophy production in high Reynolds number turbulence
• Self-attenuation of extreme events in Navier-Stokes turbulence
• Small-scale isotropy and ramp-cliff structures in scalar turbulence

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