4.7 Article

Non-dimensional energy dissipation rate near the turbulent/non-turbulent interfacial layer in free shear flows and shear free turbulence

Journal

JOURNAL OF FLUID MECHANICS
Volume 875, Issue -, Pages 321-344

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2019.462

Keywords

jets

Funding

  1. JSPS KAKENHI [18K13682, 18H01367]
  2. Fundacao para a ciencia e Tecnologia (FCT) [PTDC/EMS-ENE/6129/2014]
  3. Collaborative Research Project on Computer Science with High-Performance Computing in Nagoya University
  4. Fundação para a Ciência e a Tecnologia [PTDC/EMS-ENE/6129/2014] Funding Source: FCT

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The non-dimensional dissipation rate C-epsilon = epsilon L/u('3), where epsilon, L and u' are the viscous energy dissipation rate, integral length scale of turbulence and root-mean-square of the velocity fluctuations, respectively, is computed and analysed within the turbulent/non-turbulent interfacial (TNTI) layer using direct numerical simulations of a planar jet, mixing layer and shear free turbulence. The TNTI layer that separates the turbulent and non-turbulent regions exists at the edge of free shear turbulent flows and turbulent boundary layers, and comprises both the viscous superlayer and turbulent sublayer regions. The computation of C-epsilon is made possible by the introduction of an original procedure, based on local volume averages within spheres of radius r, combined with conditional sampling as a function of the location with respect to the TNTI layer. The new procedure allows for a detailed investigation of the scale dependence of several turbulent quantities near the TNTI layer. An important achievement of this procedure consists in permitting the computation of the turbulent integral scale within the TNTI layer, which is shown to be approximately constant. Both the non-dimensional dissipation rate and turbulent Reynolds number Re-lambda vary in space within the TNTI layer, where two relations are observed: C-epsilon similar to Re-lambda(-1) and C-epsilon similar to Re-lambda(-2). Specifically, whereas the viscous superlayer and part of the turbulent sublayer display C epsilon similar to Re-lambda(-2), the remaining of the turbulent sublayer exhibits C epsilon similar to Re-lambda(-1), which is consistent with non-equilibrium turbulence

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