pith. sign in

arxiv: nlin/0404016 · v2 · submitted 2004-04-08 · 🌊 nlin.CD · astro-ph· physics.ao-ph· physics.flu-dyn

Diffusion of passive scalar in a finite-scale random flow

classification 🌊 nlin.CD astro-phphysics.ao-phphysics.flu-dyn
keywords flowdecaylambdarandomscalarvariancebox-scaledelta
0
0 comments X
read the original abstract

We consider a solvable model of the decay of scalar variance in a single-scale random velocity field. We show that if there is a separation between the flow scale k_flow^{-1} and the box size k_box^{-1}, the decay rate lambda ~ (k_box/k_flow)^2 is determined by the turbulent diffusion of the box-scale mode. Exponential decay at the rate lambda is preceded by a transient powerlike decay (the total scalar variance ~ t^{-5/2} if the Corrsin invariant is zero, t^{-3/2} otherwise) that lasts a time t~1/\lambda. Spectra are sharply peaked at k=k_box. The box-scale peak acts as a slowly decaying source to a secondary peak at the flow scale. The variance spectrum at scales intermediate between the two peaks (k_box<<k<<k_flow) is ~ k + a k^2 + ... (a>0). The mixing of the flow-scale modes by the random flow produces, for the case of large Peclet number, a k^{-1+delta} spectrum at k>>k_flow, where delta ~ lambda is a small correction. Our solution thus elucidates the spectral make up of the ``strange mode,'' combining small-scale structure and a decay law set by the largest scales.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.