English

A new method of identifying self-similarity in isotropic turbulence

Fluid Dynamics 2013-07-18 v1

Abstract

In order to analyse results for structure functions, Sn(r)S_n(r), we propose plotting the ratio Sn(r)/S3(r)|S_n(r)/S_3(r)| against the separation rr. This method differs from the extended self-similarity (ESS) technique, which plots Sn(r)S_n(r) against S3(r)S_3(r), where S3(r)rS_3(r) \sim r. Using this method in conjunction with pseudospectral evaluation of structure functions, for the particular case of S2(r)S_2(r) we obtain the new result that the exponent ζ2\zeta_2 decreases as the Taylor-Reynolds number increases, with ζ20.67±0.02\zeta_2 \to 0.67 \pm 0.02 as RλR_\lambda \to \infty. This supports the idea of finite-viscosity corrections to the K41 prediction for S2S_2, and is the opposite of the result obtained by ESS.

Keywords

Cite

@article{arxiv.1307.4575,
  title  = {A new method of identifying self-similarity in isotropic turbulence},
  author = {W. David McComb and Samuel R. Yoffe and Arjun Berera},
  journal= {arXiv preprint arXiv:1307.4575},
  year   = {2013}
}