Diffusion of passive scalar in a finite-scale random flow
| dc.creator | Schekochihin, A. A. | |
| dc.creator | Haynes, P. H. | |
| dc.creator | Cowley, S. C. | |
| dc.date | 2004-04-08 | |
| dc.date | 2004-12-01 | |
| dc.date.accessioned | 2026-07-07T10:50:42Z | |
| dc.date.available | 2026-07-07T10:50:42Z | |
| dc.description | 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/λ. 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. | |
| dc.description | revtex4, 8 pages, 4 figures; final published version | |
| dc.identifier | https://arxiv.org/abs/nlin/0404016 | |
| dc.identifier | http://arxiv.org/abs/nlin/0404016 | |
| dc.identifier | Phys.Rev.E70:046304,2004 | |
| dc.identifier | doi:10.1103/PhysRevE.70.046304 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/184620 | |
| dc.subject | Chaotic Dynamics | |
| dc.subject | Astrophysics | |
| dc.subject | Atmospheric and Oceanic Physics | |
| dc.subject | Fluid Dynamics | |
| dc.title | Diffusion of passive scalar in a finite-scale random flow | |
| dc.type | text |