Hostname: page-component-5db58dd55d-pjp64 Total loading time: 0 Render date: 2026-06-07T01:12:40.987Z Has data issue: false hasContentIssue false

Turbulent drag reduction through oscillating discs – CORRIGENDUM

Published online by Cambridge University Press:  14 October 2018

Daniel J. Wise
Affiliation:
Department of Fluid Dynamics, A*Star Institute of High Performance Computing, Singapore
Paolo Olivucci
Affiliation:
Department of Mechanical Engineering, The University of Sheffield, S1 3JD Sheffield, UK
Pierre Ricco*
Affiliation:
Department of Mechanical Engineering, The University of Sheffield, S1 3JD Sheffield, UK
*
Email address for correspondence: p.ricco@sheffield.ac.uk

Abstract

Information

Type
Corrigendum
Copyright
© 2018 Cambridge University Press 
Figure 0

Figure 1. (a) Isosurfaces of $\langle u_{d}v_{d}\rangle ^{+}$ observed from the $y$$z$ plane at $x^{+}=0$, $x^{+}=160$, $x^{+}=320$ (from top to bottom). The plots show only $\langle u_{d}v_{d}\rangle ^{+}$ for $u_{d}<0$, $v_{d}>0$ as within the contour range the contributions from other contributions of $u_{d}$ and $v_{d}$ are negligible. (b) Wall-normal profiles of $u_{d,rms}^{+}$ (solid lines) and $\widehat{u_{d}v_{d}}^{+}$ (dashed lines). Profiles are shown for phases from the first half of the disc oscillation.

Figure 1

Figure 2. Reproduction of figure 14 on p. 557 of Wise & Ricco (2014). Note that the arrows of the interdisc structures now point upstream and upward in the wall-normal direction.

Figure 2

Figure 3. (a) $\mathscr{R}_{t}$, the contribution to drag reduction due to the modification to the turbulent Reynolds stresses, versus $\unicode[STIX]{x1D6FF}^{+}$, the penetration depth of the disc-flow boundary layer. (b) $\mathscr{R}_{d}$, contribution to drag reduction due to the disc-flow Reynolds stresses, versus $W^{2}T^{0.3}$. White circles: $W^{+}=3$, light grey: $W^{+}=6$, dark grey: $W^{+}=9$.