Bulletin of the American Physical Society
71st Annual Meeting of the APS Division of Fluid Dynamics
Volume 63, Number 13
Sunday–Tuesday, November 18–20, 2018; Atlanta, Georgia
Session M39: Pipe Flow
8:00 AM–9:57 AM,
Tuesday, November 20, 2018
Georgia World Congress Center
Room: Ballroom 3/4
Chair: Xiaohua Wu, Royal Military College of Canada
Abstract ID: BAPS.2018.DFD.M39.3
Abstract: M39.00003 : Direct numerical simulation of pulsatile rough-wall turbulent pipe flow
8:26 AM–8:39 AM
Presenter:
Thomas Jelly
(University of Melbourne)
Authors:
Thomas Jelly
(University of Melbourne)
Rey Chin
(University of Adelaide)
Simon Illingworth
(University of Melbourne)
Jason Monty
(University of Melbourne)
Ivan Marusic
(University of Melbourne)
Andrew Ooi
(University of Melbourne)
Direct numerical simulations (DNS) of pulsatile rough-wall turbulent pipe flow have been performed at a friction Reynolds number of 540. The rough walls have a three-dimensional sinusoidal height distribution and were resolved explicitly using a body-fitted grid. Three geometrically-scaled surfaces with a common amplitude-to-wavelength ratio have been considered. An unsteady axial pressure gradient was imposed to simulate a current-dominated pulsatile flow in the very-high-frequency regime. The resulting flow field exhibits axial-azimuthal periodicity, as well as phase dependence in time, and permits instantaneous quantities to be decomposed into four separate parts: (i) a global-averaged component; (ii) a roughness-induced component; (iii) a pulsation-induced component and (iv) the remaining turbulent fluctuation. We compare statistics of (i)-(iv) against their non-pulsatile counterparts using past results related to the current work (Chan et al., J. Fluid Mech., 771:743-777, 2015). Whilst the pulsatile and non-pulsatile data collapse well in the outer region, clear differences are evident in the near-roughness region and the region below the roughness crests. These differences will be examined in the context of phase-averaged statistics (in both space and time).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DFD.M39.3
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