Generating wall-bounded turbulent inflows at high Reynolds numbers
Ronith Stanly, Timofey Mukha, Martin Karp, Stefano Markidis, Philipp Schlatter
TL;DR
The paper tackles the challenge of generating accurate inflow conditions for high-$Re$ wall-bounded turbulence without incurring prohibitive development lengths. It introduces a structure-based inflow method that decomposes cross-stream slices into inner and outer spectral components, upscales the outer content from a base Reynolds number to a higher target using spanwise wavenumber shifting, and reconstructs full velocity fields by combining scaled outer modes with inner information and adjusted timing and energy. Validation shows that inflow slices upscaled from $Re_ heta=2240$ and $4430$ to $Re_ heta=8000$ yield DNS results with skin-friction and shape-factor within $\\pm3.5\%$ and $\\\\\pm0.5\%$, and Reynolds stresses aligning by about $8\, δ_{99,0}$, representing an order-of-magnitude reduction in development length compared to other methods. The approach relies on measurable scaling laws of turbulent boundary layers and demonstrates robust performance in DNS of spatially developing TBLs, with potential applicability to pipes, channels, and atmospheric boundary layers.
Abstract
One of the main challenges in simulating high Reynolds number ($Re$) turbulent boundary layers (TBLs) is the long streamwise distance required for large-scale outer-layer structures to develop, making such simulations prohibitively expensive. We propose an inflow generation method for high $Re$ wall turbulence that leverages the known structure and scaling laws of TBLs, enabling shorter development lengths by providing rich input information. As observed from the inner-scaled pre-multiplied spectra of streamwise velocity, with an increase in $Re$ the outer region grows and occupies more of the spanwise wavenumber space in proportion to the increase in $Re$; while the inner region remains approximately the same. Exploiting this behavior, we generate high-$Re$ inflow conditions for a $\textit{target}$ $Re$ by starting from cross-stream velocity slices at a lower $\textit{base}$ $Re$. In spectral space, we identify the inner and outer region wavenumbers, and shift the outer-region components proportionally to the desired $Re$ increase. We closely examine the capability of this method by scaling a set of velocity slices at $Re_θ=2240$ and $4430$ to $Re_θ=8000$, and using them as inflow conditions for direct numerical simulations (DNS) of spatially developing TBLs growing from $Re_θ=8000-9000$. The skin friction coefficient and shape factor predicted by the new method, regardless of the $\textit{base}$ $Re$ tested, is within $\pm3.5\%$ and $\pm0.5\%$, respectively, of that of a precursor simulation right from the inlet. Reynolds stresses match very well after approximately $8~δ_{99_0}$. This gives an order of magnitude reduction in development length compared to other methods proposed in the literature.
