Direct Numerical Simulations of Turbulent Flow Over Various Riblet Shapes in Minimal-Span Channels
Web of Science
AuthorEndrikat, S; Modesti, D; MacDonald, M; Garcia-Mayoral, R; Hutchins, N; Chung, D
Source TitleFlow, Turbulence and Combustion
Document TypeJournal Article
CitationsEndrikat, S., Modesti, D., MacDonald, M., Garcia-Mayoral, R., Hutchins, N. & Chung, D. (2020). Direct Numerical Simulations of Turbulent Flow Over Various Riblet Shapes in Minimal-Span Channels. Flow, Turbulence and Combustion, 107 (1), https://doi.org/10.1007/s10494-020-00224-z.
Access StatusThis item is embargoed and will be available on 2021-11-20
ARC Grant codeARC/DP170102595
Riblets reduce skin-friction drag until their viscous-scaled size becomes large enough for turbulence to approach the wall, leading to the breakdown of drag-reduction. In order to investigate inertial-flow mechanisms that are responsible for the breakdown, we employ the minimal-span channel concept for cost-efficient direct numerical simulation (DNS) of rough-wall flows (MacDonald et al., J. Fluid Mech., vol. 816, 2017, pp. 5–42). This allows us to investigate six different riblet shapes and various viscous-scaled sizes for a total of 21 configurations. We verify that the small numerical domains capture all relevant physics by varying the box size and by comparing to reference data from full-span channel flow. Specifically, we find that, close to the wall in the spectral region occupied by drag-increasing Kelvin–Helmholtz rollers (García-Mayoral & Jiménez, J. Fluid Mech., vol. 678, 2011, pp. 317–347), the energy-difference relative to smooth-wall flow is not affected by the narrow domain, even though these structures have large spanwise extents. This allows us to evaluate the influence of the Kelvin–Helmholtz instability by comparing fluctuations of wall-normal and streamwise velocity, pressure and a passive scalar over riblets of different shapes and viscous-scaled sizes to those over a smooth wall. We observe that triangular riblets with a tip angle a = 30° and blades appear to support the instability, whereas triangular riblets with a = 60°–90° and trapezoidal riblets with a = 30° show little to no evidence of Kelvin–Helmholtz rollers.
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