We carry out direct numerical simulations (DNSs) of minimal open-channel flow over riblets, which are streamwise-aligned grooves that modify the near-wall flow for drag reduction. Several riblet sizes and cross-sectional geometries are simulated, namely symmetric triangular, asymmetric triangular, blade and trapezoidal. With this unprecedented breadth and detail afforded by the DNS data, we are able to obtain more general insights into the flow physics of riblets. A generalization of the Fukagata–Iwamoto–Kasagi (FIK) identity is used to isolate the different contributions to skin friction drag changes. We show that, in the nonlinear regime of large riblet size, the dispersive contribution is comparable or larger than the turbulent one, repr...
Structures resulting from a Kelvin–Helmholtz instability have been shown to contribute to skin-frict...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...
© 2019 International Symposium on Turbulence and Shear Flow Phenomena, TSFP. All rights reserved. We...
© 2019 International Symposium on Turbulence and Shear Flow Phenomena, TSFP. All rights reserved. We...
We carry out direct numerical simulations of turbulent flow over riblets, streamwise- aligned groove...
We carry out direct numerical simulations of turbulent flow over riblets, streamwise- aligned groove...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. We carry out direct numerical simu...
We carry out direct numerical simulation of minimal openchannel flow over riblets. Several riblet g...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. We carry out direct numerical simu...
International audienceLarge Eddy Simulations of zero-pressure-gradient turbulent boundary layers ove...
We carry out direct numerical simulation of minimal open-channel flow over riblets. Several riblet g...
International audienceLarge Eddy Simulations of zero-pressure-gradient turbulent boundary layers ove...
© 2020 Sebastian EndrikatFlow passing over the surface of vehicles creates significant skin-friction...
Structures resulting from a Kelvin–Helmholtz instability have been shown to contribute to skin-fric...
Structures resulting from a Kelvin–Helmholtz instability have been shown to contribute to skin-frict...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...
© 2019 International Symposium on Turbulence and Shear Flow Phenomena, TSFP. All rights reserved. We...
© 2019 International Symposium on Turbulence and Shear Flow Phenomena, TSFP. All rights reserved. We...
We carry out direct numerical simulations of turbulent flow over riblets, streamwise- aligned groove...
We carry out direct numerical simulations of turbulent flow over riblets, streamwise- aligned groove...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. We carry out direct numerical simu...
We carry out direct numerical simulation of minimal openchannel flow over riblets. Several riblet g...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. We carry out direct numerical simu...
International audienceLarge Eddy Simulations of zero-pressure-gradient turbulent boundary layers ove...
We carry out direct numerical simulation of minimal open-channel flow over riblets. Several riblet g...
International audienceLarge Eddy Simulations of zero-pressure-gradient turbulent boundary layers ove...
© 2020 Sebastian EndrikatFlow passing over the surface of vehicles creates significant skin-friction...
Structures resulting from a Kelvin–Helmholtz instability have been shown to contribute to skin-fric...
Structures resulting from a Kelvin–Helmholtz instability have been shown to contribute to skin-frict...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...
© 2018 Australasian Fluid Mechanics Society. All rights reserved. Structures resulting from a Kelvin...