English

Multi-scale theory of rotating turbulence

Astrophysics 2009-11-13 v2 Fluid Dynamics

Abstract

We consider turbulence induced by an arbitrary forcing and derive turbulence amplitude and turbulent transport coefficients, first by using a quasi-linear theory and then by using a multi-scale renormalisation analysis. With an isotropic forcing, the quasi-linear theory gives that the turbulent transport coefficients, both parallel and perpendicular to the rotation vector, have the asymptotic scaling Ω1\Omega^{-1} for rapid rotation (i.e. when the rotation rate Ω\Omega is larger than the inverse of the correlation time of the forcing and the diffusion time), while the renormalisation analysis suggests a weaker dependence on Ω\Omega, with Ω1/2\Omega^{-1/2} scaling. The turbulence amplitude is found to scale as Ω0Ω1\Omega^0 - \Omega^{-1} in the rapid rotation limit depending on the property of the forcing. In the case of an anisotropic forcing, we find that non-diffusive fluxes of angular momentum scale as Ω2Ω1\Omega^{-2} - \Omega^{-1} for rapid rotation, depending on the temporal correlation of the forcing.

Keywords

Cite

@article{arxiv.astro-ph/0703079,
  title  = {Multi-scale theory of rotating turbulence},
  author = {Nicolas Leprovost and Eun-Jin Kim},
  journal= {arXiv preprint arXiv:astro-ph/0703079},
  year   = {2009}
}
R2 v1 2026-07-22T09:21:09.989Z