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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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Ahlers, Guenter1, Autor           
Bodenschatz, Eberhard1, Autor                 
Hartmann, Robert2, Autor
He, Xiaozhou1, Autor           
Lohse, Detlef3, Autor           
Reiter, Philipp1, Autor           
Stevens, Richard J. A. M.2, Autor
Verzicco, Roberto2, Autor
Wedi, Marcel1, Autor           
Weiss, Stephan1, Autor           
Zhang, Xuan1, Autor           
Zwirner, Lukas1, Autor           
Shishkina, Olga1, Autor           
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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 Zusammenfassung: 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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Sprache(n): eng - English
 Datum: 2022-02-24
 Publikationsstatus: Online veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1103/PhysRevLett.128.084501
 Art des Abschluß: -

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Titel: Physical Review Letters
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 128 Artikelnummer: 084501 Start- / Endseite: - Identifikator: ISSN: 0031-9007
ISSN: 1079-7114