Application of riblets to separating turbulent boundary layers
ORAL
Abstract
We conduct direct numerical simulations of separating turbulent boundary layers (TBLs) over triangular riblets with tip angles 90o (T9) and 60o (T6). Our setup follows the separating TBL study of Wu et al. ( J. Fluid Mech., vol. 883, 2020, p. A45). An equilibrium zero pressure-gradient (ZPG) TBL is generated at a reference location, followed by imposition of a Gaussian suction profile to create a separation bubble. The ZPG TBLs over the riblets and the benchmark smooth case have matched momentum thickness Reynolds number Reθ0 = 583 (friction Reynolds number 224). We employ a well-validated spectral-element solver, and leverage its unstructured-grid nature to generate an optimal grid, based on the size of turbulent scales across the TBL. At the reference location, the T9 and T6 riblets respectively increase and reduce drag, with viscous-scaled spacings 52 and 13. We discover that for both riblet cases, the mean separation point occurs at a distance of 140θ0 downstream of the reference location, 18% shorter than the mean separation distance for the smooth case (170θ0). This outcome is related to the progressive enhancement of the Kelvin-Helmholtz (KH) rollers over the riblets, owing to the continuous rise in the adverse pressure-gradient. The KH rollers penetrate into the turbulent separation bubble, with significantly larger size and coherence compared to their counterparts upstream of the mean separation point.
*AR acknowledges the support from the Air Force Office of Scientific Research (AFOSR) under award number FA8655-24-1-7008, monitored by Dr. Douglas Smith and Dr. Barrett Flake. VK acknowledges his AI4S fellowship within the Generacion D initiative by Red.es, Ministerio para la Transformacion Digital y de la Funcion Publica, for talent attraction (C005/24-ED CV1), funded by NextGenerationEU through PRTR. WW acknowledges the support from the AFOSR Grant No. FA9550-25-1-0033, monitored by Dr. Gregg Abate. We thank EPSRC for the computational time made available on ARCHER2 via the UK Turbulence Consortium (EP/R029326/1), and the UKRI access to the HPC call 2024.
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Presenters
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Wen Wu
- University of Mississippi