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 E33: Turbulent Convection I
5:10 PM–6:28 PM,
Sunday, November 18, 2018
Georgia World Congress Center
Room: B405
Chair: Jared Whitehead, Brigham Young University
Abstract ID: BAPS.2018.DFD.E33.6
Abstract: E33.00006 : Effects of fluid properties on sheared thermal convection*
6:15 PM–6:28 PM
Presenter:
Alexander Blass
(University of Twente)
Authors:
Alexander Blass
(University of Twente)
Xiaojue Zhu
(University of Twente)
Pier Tabak
(University of Twente)
Roberto Verzicco
(Univ of Roma)
Detlef Lohse
(University of Twente)
Richard Stevens
(University of Twente)
A series of direct numerical simulations of sheared thermal convection have been performed with a second-order finite difference code (van der Poel et al., Comp. & Fluids, 116:10-16, 2015), optimized for a GPU cluster (AFiD GPU (Zhu et al., Comp. Phys. Comm., 229:199-210, 2018)), with a Rayleigh number Ra = 1x106 and a wall Reynolds number Rew of 0 ≤ Rew ≤ 4000. We study the Prandtl number (Pr) dependency of flow structures in the regime of 0.22 ≤ Pr ≤ 4.6. Our findings show that a high Pr results in an increased dependency of Nusselt number and Rew. At Pr = 4.6 we find a dependency of Nu(Rew) ∝ 1x10-3 Rew in the shear dominated regime, while in the same regime for Pr = 0.22 and Pr = 0.46, Nu(Rew) seems to collapse at Nu(Rew) ∝ 1x10-4 Rew.
Additionally, we study the bulk Richardson number Rib - the ratio of buoyancy to mechanical forcing. For low Rib the flow settles in a regime dominated by the flow shearing, while a thermally dominated regime is present for high Rib. Various flow statistics have been plotted as a function of Rib-1 to determine whether the Richardson number is a good estimator of the flow behavior. We show that in the studied parameter space Rib-1 Ra0.31 predicts Nu within 10%.
*NWO-I SURFsara-Cartesius
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DFD.E33.6
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