What rotation rate maximizes heat transport in rotating Rayleigh-Bénard convection with Prandtl number larger than one?

Yantao Yang, Roberto Verzicco, Detlef Lohse, and Richard J. A. M. Stevens
Phys. Rev. Fluids 5, 053501 – Published 13 May 2020

Abstract

The heat transfer and flow structure in rotating Rayleigh-Bénard convection are strongly influenced by the Rayleigh (Ra), Prandtl (Pr), and Rossby (Ro) numbers. For Pr1 and intermediate rotation rates, the heat transfer is increased compared to the nonrotating case. We find that the regime of increased heat transfer is subdivided into low- and high-Ra-number regimes. For Ra5×108 the heat transfer at a given Ra and Pr is highest at an optimal rotation rate, at which the thicknesses of the viscous and thermal boundary layers are about equal. From the scaling relations of the thermal and viscous boundary layer thicknesses, we derive that the optimal rotation rate scales as 1/Roopt0.12Pr1/2Ra1/6. In the low-Ra regime the heat transfer is similar in a periodic domain and cylindrical cells with different aspect ratios, i.e., the ratio of diameter to height. This is consistent with the view that the vertically aligned vortices are the dominant flow structure. For Ra5×108 the above scaling for the optimal rotation rate does not hold anymore. It turns out that in the high-Ra regime, the flow structures at the optimal rotation rate are very different than for lower Ra. Surprisingly, the heat transfer in the high-Ra regime differs significantly for a periodic domain and cylindrical cells with different aspect ratios, which originates from the sidewall boundary layer dynamics and the corresponding secondary circulation.

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  • Received 17 September 2019
  • Accepted 13 April 2020

DOI:https://doi.org/10.1103/PhysRevFluids.5.053501

©2020 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Yantao Yang

  • SKLTCS and Department of Mechanics and Engineering Science, BIC-ESAT, College of Engineering, and Institute of Ocean Research, Peking University, Beijing 100871, China

Roberto Verzicco

  • Physics of Fluids Group, Department of Science and Technology, MESA+ Institute, Max Planck Center Twente for Complex Fluid Dynamics, J. M. Burgers Center for Fluid Dynamics, University of Twente, 7500 AE Enschede, Netherlands; Dipartimento di Ingegneria Industriale, University of Rome “Tor Vergata,” Via del Politecnico 1, Rome 00133, Italy; and Gran Sasso Science Institute, Viale F. Crispi 7, 67100 L'Aquila, Italy

Detlef Lohse

  • Physics of Fluids Group, Department of Science and Technology, MESA+ Institute, Max Planck Center Twente for Complex Fluid Dynamics and J. M. Burgers Center for Fluid Dynamics, University of Twente, 7500 AE Enschede, Netherlands and Max Planck Institute for Dynamics and Self-Organization, Am Faßberg 17, Göttingen, Germany

Richard J. A. M. Stevens

  • Physics of Fluids Group, Department of Science and Technology, MESA+ Institute, Max Planck Center Twente for Complex Fluid Dynamics and J. M. Burgers Center for Fluid Dynamics, University of Twente, 7500 AE Enschede, Netherlands

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Vol. 5, Iss. 5 — May 2020

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