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  Aspect Ratio Dependence of Heat Transfer in a Cylindrical Rayleigh-Bénard Cell

Ahlers, G., Bodenschatz, E., Hartmann, R., He, X., Lohse, D., Reiter, P., et al. (2022). Aspect Ratio Dependence of Heat Transfer in a Cylindrical Rayleigh-Bénard Cell. Physical Review Letters, 128: 084501. doi:10.1103/PhysRevLett.128.084501.

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 Creators:
Ahlers, Guenter1, Author           
Bodenschatz, Eberhard1, Author                 
Hartmann, Robert2, Author
He, Xiaozhou1, Author           
Lohse, Detlef3, Author           
Reiter, Philipp1, Author           
Stevens, Richard J. A. M.2, Author
Verzicco, Roberto2, Author
Wedi, Marcel1, Author           
Weiss, Stephan1, Author           
Zhang, Xuan1, Author           
Zwirner, Lukas1, Author           
Shishkina, Olga1, Author           
Affiliations:
1Laboratory for Fluid Physics, Pattern Formation and Biocomplexity, Max Planck Institute for Dynamics and Self-Organization, Max Planck Society, ou_2063287              
2External Organizations, ou_persistent22              
3Max Planck Institute for Dynamics and Self-Organization, Max Planck Society, ou_2063285              

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 Abstract: While the heat transfer and the flow dynamics in a cylindrical Rayleigh-Benard (RB) cell are rather independent of the aspect ratio Gamma (diameter/height) for large Gamma, a small-Gamma cell considerably stabilizes the flow and thus affects the heat transfer. Here, we first theoretically and numerically show that the critical Rayleigh number for the onset of convection at given Gamma follows Ra-c,Ra-Gamma similar to Ra-c,Ra-infinity(1 + C Gamma(-2))(2), with C less than or similar to 1.49 for Oberbeck-Boussinesq (OB) conditions. We then show that, in a broad aspect ratio range (1/32) <= Gamma <= 32, the rescaling Ra -> Ra-l Ra[Gamma(2)/(C+Gamma(2))](3/2) collapses various OB numerical and almost-OB experimental heat transport data Nu(Ra,Gamma). Our findings predict the Gamma dependence of the onset of the ultimate regime Ra-u,Ra-Gamma similar to [Gamma(2)/(C+Gamma(2))](-3/2) in the OB case. This prediction is consistent with almost-OB experimental results (which only exist for Gamma = 1, 1/2, and 1/3) for the transition in OB RB convection and explains why, in small-Gamma cells, much larger Ra (namely, by a factor Gamma(-3)) must be achieved to observe the ultimate regime.

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Language(s): eng - English
 Dates: 2022-02-24
 Publication Status: Published online
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 Rev. Type: Peer
 Identifiers: DOI: 10.1103/PhysRevLett.128.084501
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Title: Physical Review Letters
Source Genre: Journal
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Pages: - Volume / Issue: 128 Sequence Number: 084501 Start / End Page: - Identifier: ISSN: 0031-9007
ISSN: 1079-7114