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Dependence of scalar mixing on initial conditions in turbulent channel flow

Milind Singh, Emmanuel Germaine, Laurent Mydlarski, and Luca Cortelezzi
Phys. Rev. Fluids 8, 124605 – Published 19 December 2023

Abstract

Turbulent scalar mixing occurs within a wide variety of natural and engineering flows. Predicting and controlling the scalar concentration(s) within these flows can yield immediate benefits to numerous applications across many fields. To that end, a better understanding of the effects of scalar-field initial conditions on the evolution(s) of scalar fields is required to either promote or delay the rate at which mixing occurs. Direct numerical simulations are employed herein to simulate the evolution in time of the hydrodynamic and (passive) scalar fields within a fully developed turbulent channel flow. The effects of the scalar field initial conditions are studied by analyzing the evolution of the scalar field subject to three different initial conditions with interfaces oriented normal to the streamwise, wall-normal, and transverse directions. Particular emphasis is placed on the scalar variance and dissipation rate budgets, including the evolutions of their constituent terms. The fastest mixing occurs for the initial condition in which the interface is aligned normal to the mean velocity vector. The rapid mixing in this case is associated with higher rates of production and destruction of the scalar dissipation, as well as strong advection and stretching of the interface by the mean flow. In addition to better mixing arising from the stronger turbulence near the wall, enhanced mixing is correlated with having the edge of an interface along a channel wall, such that a large distortion of the initial interface arises from the combined effects of the no-slip condition at the channel walls with the advection of the interface by the mean flow in the region between the walls. To maximize this effect, it is recommended that scalar interfaces be aligned normal to the mean velocity vector to promote mixing within internal flows.

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  • Received 17 August 2023
  • Accepted 13 November 2023

DOI:https://doi.org/10.1103/PhysRevFluids.8.124605

©2023 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Milind Singh, Emmanuel Germaine, and Laurent Mydlarski

  • Department of Mechanical Engineering, McGill University, Montréal, Québec H3A 0C3, Canada

Luca Cortelezzi

  • Department of Aerospace Science and Technology, Politecnico di Milano, 20156 Milano, Italy

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Issue

Vol. 8, Iss. 12 — December 2023

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