English

Large-scale mean patterns in turbulent convection

Fluid Dynamics 2016-12-30 v1

Abstract

Large-scale patterns, which are well-known from the spiral defect chaos regime of thermal convection at Rayleigh numbers Ra<104Ra < 10^4, continue to exist in three-dimensional numerical simulations of turbulent Rayleigh-B\'{e}nard convection in extended cylindrical cells with an aspect ratio Γ=50\Gamma=50 and Ra>105Ra>10^5. They are uncovered when the turbulent fields are averaged in time and turbulent fluctuations are thus removed. We apply the Boussinesq closure to estimate turbulent viscosities and diffusivities, respectively. The resulting turbulent Rayleigh number RaRa_{\ast}, that describes the convection of the mean patterns, is indeed in the spiral defect chaos range. The turbulent Prandtl numbers are smaller than one with 0.2Pr0.40.2\le Pr_{\ast}\le 0.4 for Prandtl numbers 0.7Pr100.7 \le Pr\le 10. Finally, we demonstrate that these mean flow patterns are robust to an additional finite-amplitude side wall-forcing when the level of turbulent fluctuations in the flow is sufficiently high.

Keywords

Cite

@article{arxiv.1506.01560,
  title  = {Large-scale mean patterns in turbulent convection},
  author = {Mohammad S. Emran and Jörg Schumacher},
  journal= {arXiv preprint arXiv:1506.01560},
  year   = {2016}
}

Comments

13 pages, 7 figures

R2 v1 2026-06-22T09:47:15.916Z