The Diffusion Approximation in Turbulent Two-Particle Dispersion
arXiv:1306.6388 · doi:10.1103/PhysRevE.88.041001
Abstract
We solve an inverse problem for fluid particle pair-statistics: we show that a time sequence of probability density functions (PDF's) of separations can be exactly reproduced by solving the diffusion equation with a suitable time-dependent diffusivity. The diffusivity tensor is given by a time-integral of a conditional Lagrangian velocity structure-function, weighted by a ratio of PDF's. Physical hypotheses for hydrodynamic turbulence (sweeping, short memory, mean-field) yield simpler integral formulas, including one of Kraichnan and Lundgren. We evaluate the latter using a spacetime database from a numerical Navier-Stokes solution for driven turbulence. This diffusion theory reproduces PDF's well at rms separations, but growth rate of mean-square dispersion is overpredicted due to neglect of memory effects. More general applications of our approach are sketched.
5 pages, 4 figures
References in corpus (5)
- A public turbulence database cluster and applications to study Lagrangian evolution of velocity increments in turbulence
- Stochastic Flux-Freezing and Magnetic Dynamo
- Timescales of Turbulent Relative Dispersion
- Extreme events in the dispersions of two neighboring particles under the influence of fluid turbulence
- Geometry and violent events in turbulent pair dispersion
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