English

Chaotic and turbulent mixing of passive scalar

Fluid Dynamics 2019-03-28 v1

Abstract

Spatio-temporal deterministic chaos at small Taylor-Reynolds numbers Reλ40Re_{\lambda} \lesssim 40 and distributed chaos at turbulent Reλ40Re_{\lambda} \gtrsim 40 in passive scalar dynamics have been studied using results of direct numerical simulations of homogeneous incompressible flows (with and without mean gradient of the passive scalar) for 8Reλ<7008 \leq Re_{\lambda} < 700 and of a reacting turbulent mixing layer. It is shown that the deterministic chaos in the passive scalar fluctuations at the small ReλRe_{\lambda} is characterized by exponential spatial (wavenumber) spectrum: E(k)exp(k/kc)E(k) \propto \exp-(k/k_c), whereas the distributed chaos at turbulent ReλRe_{\lambda} is characterized by stretched exponential spectrum E(k)exp(k/kβ)3/4E(k) \propto \exp-(k/k_{\beta})^{3/4}. The Birkhoff-Saffman invariant related to the momentum conservation and, due to the Noether theorem, to the spatial homogeneity has been used as a theoretical basis for this stretched exponential spectrum. Although the kck_c and kβk_{\beta} represent the large-scale structures a relevance of the Batchelor scale kbatk_{bat} has been established as well: the normalized values kc/kbatk_c/k_{bat} and kβ/kbatk_{\beta}/k_{bat} exhibit universality.

Keywords

Cite

@article{arxiv.1903.11523,
  title  = {Chaotic and turbulent mixing of passive scalar},
  author = {A. Bershadskii},
  journal= {arXiv preprint arXiv:1903.11523},
  year   = {2019}
}