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Convergence issue of the k-ω SST turbulence model in Nalu-Wind #1286

@BumseokLee

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@BumseokLee

Hi,

I am reporting a convergence issue with the omega transport equation of the k-ω SST turbulence model in Nalu-Wind. I’ve attached non-linear residual plots for NASA’s canonical case: the subsonic NACA0012 airfoil at Re=6e6. I used the 2-D C meshes and flow conditions from NASA Langley’s Turbulence Modeling Resource (TMR) Website. The freestream Mach number of the case in NASA TMR was 0.15 but I reduced it to 0.1.

Screenshot 2024-08-19 at 9 43 45 AM Screenshot 2024-08-19 at 9 43 56 AM

In fact, this is not the only case that I’ve observed suspicious or inconsistent behavior in the omega transport equation. I’ve encountered similar issues (very large residuals or inconsistent convergence trend for a different number of Picard iterations) in other cases, including 2-D airfoils and 3-D blade simulations. In my tests, the sustaining terms didn’t resolve the issue.

Despite these behaviors, the residuals of the momentum (mean flow) and k still converge reasonably. Additionally, the predicted aerodynamic coefficients converge, showing good agreement with available experimental data or other numerical results. This might be due to the clipping functions of the model and/or the current implementation in Nalu-Wind.

Screenshot 2024-08-19 at 9 46 41 AM Screenshot 2024-08-19 at 9 46 52 AM

However, the magnitude of the residuals still looks concerning. The convergence stall of the omega could slow down the overall convergence of the turbulence model and, consequently, the mean flow as well. This issue could be particularly significant in highly unsteady flow simulations, such as IDDES FSI simulations, where sufficient iterations are not available between physical time steps. It could also affect laminar-turbulent transition simulations too because the transition model triggers the transition onset within the boundary layer using the k and omega values, making it highly sensitive to near-wall values. (That’s why I previously fixed the omega boundary condition at the wall, although it doesn’t seem to make a significant difference in fully turbulent simulations.)

I haven’t yet investigated where these large residuals occur, but I believe it is worthwhile to check. I am currently occupied with some other work in my projects, so I cannot attack this issue immediately. However, I can investigate this after completing my urgent work, probably around early or mid-September. If anyone is interested in this, you are welcome. I can share the mesh and input files, or you can directly start from the NASA mesh to reproduce the issue.

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