Abstract
This article presents new information on the growth of a mixing layer originating from turbulent upstream conditions, obtained through large eddy simulation. The mixing layer develops from a turbulent high-speed side boundary layer and a laminar low-speed side boundary layer. Validation of the grid resolution, subgrid-scale model, and spanwise domain extent is performed. It is observed that the initially turbulent mixing layer undergoes three distinct phases in its evolution: a sub-shear region, where an internal shear layer develops immediately downstream of the splitter plate trailing edge and entrains the vorticity from the high-speed side boundary layer; a relaxation region, where the mixing layer develops to a point where the influence of the upstream conditions is forgotten; and a fully developed region, where the flow behaves in a self-preserving manner. The simulations display a discrepancy in downstream distances for the mean field, and turbulent stresses, to attain a self-preserving state, respectively, which is attributed to the spanwise integral length scale requiring a longer distance to attain an equilibrium value when compared to its streamwise and vertical counterparts. Large-scale, spanwise-orientated coherent structures are found to be a constituent part of the fully developed flow, and there is an absence of a spatially stationary streamwise structure in the initially turbulent mixing layer. The findings of the simulations are used to reconcile discrepancies found in experiments available in the archival literature.
| Original language | English |
|---|---|
| Article number | 115194 |
| Number of pages | 25 |
| Journal | Physics of Fluids |
| Volume | 36 |
| Issue number | 11 |
| Early online date | 21 Nov 2024 |
| DOIs | |
| Publication status | Published - Nov 2024 |
Bibliographical note
Copyright © 2024 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/).Funding
The research used TAURUS, the Aston University High Performance Computing facility. Aspects of the research were performed using ALICE, the University of Leicester High Performance Computing facility. The calculation on grid 3 was performed using the Sulis Tier 2 HPC platform hosted by the Scientific Computing Research Technology Platform at the University of Warwick. Sulis is funded by EPSRC Grant EP/T022108/1 and the HPC Midlands+ consortium.