English

Non-Fickian diffusion and tau approximation from numerical turbulence

Astrophysics 2009-11-10 v3 Chaotic Dynamics Fluid Dynamics

Abstract

Evidence for non-Fickian diffusion of a passive scalar is presented using direct simulations of homogeneous isotropic turbulence. The results compare favorably with an explicitly time-dependent closure model based on the tau approximation. In the numerical experiments three different cases are considered: (i) zero mean concentration with finite initial concentration flux, (ii) an initial top hat profile for the concentration, and (iii) an imposed background concentration gradient. All cases agree in the resulting relaxation time in the tau approximation relating the triple correlation to the concentration flux. The first order smoothing approximation is shown to be inapplicable.

Keywords

Cite

@article{arxiv.astro-ph/0306521,
  title  = {Non-Fickian diffusion and tau approximation from numerical turbulence},
  author = {Axel Brandenburg and Petri Käpylä and Amjed Mohammed},
  journal= {arXiv preprint arXiv:astro-ph/0306521},
  year   = {2009}
}

Comments

10 pages, 7 figs, Physics of Fluids (final version)

R2 v1 2026-07-22T08:25:15.965Z