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Classical 1/3 scaling of convection holds up to Ra = 10(15)

The global transport of heat and momentum in turbulent convection is constrained by thin thermal and viscous boundary layers at the heated and cooled boundaries of the system. This bottleneck is thought to be lifted once the boundary layers themselves become fully turbulent at very high values of th...

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Autores principales: Iyer, Kartik P., Scheel, Janet D., Schumacher, Jörg, Sreenivasan, Katepalli R.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: National Academy of Sciences 2020
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7149414/
https://www.ncbi.nlm.nih.gov/pubmed/32213591
http://dx.doi.org/10.1073/pnas.1922794117
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author Iyer, Kartik P.
Scheel, Janet D.
Schumacher, Jörg
Sreenivasan, Katepalli R.
author_facet Iyer, Kartik P.
Scheel, Janet D.
Schumacher, Jörg
Sreenivasan, Katepalli R.
author_sort Iyer, Kartik P.
collection PubMed
description The global transport of heat and momentum in turbulent convection is constrained by thin thermal and viscous boundary layers at the heated and cooled boundaries of the system. This bottleneck is thought to be lifted once the boundary layers themselves become fully turbulent at very high values of the Rayleigh number [Formula: see text] —the dimensionless parameter that describes the vigor of convective turbulence. Laboratory experiments in cylindrical cells for [Formula: see text] have reported different outcomes on the putative heat transport law. Here we show, by direct numerical simulations of three-dimensional turbulent Rayleigh–Bénard convection flows in a slender cylindrical cell of aspect ratio [Formula: see text] , that the Nusselt number—the dimensionless measure of heat transport—follows the classical power law of [Formula: see text] up to [Formula: see text]. Intermittent fluctuations in the wall stress, a blueprint of turbulence in the vicinity of the boundaries, manifest at all [Formula: see text] considered here, increasing with increasing [Formula: see text] , and suggest that an abrupt transition of the boundary layer to turbulence does not take place.
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spelling pubmed-71494142020-04-15 Classical 1/3 scaling of convection holds up to Ra = 10(15) Iyer, Kartik P. Scheel, Janet D. Schumacher, Jörg Sreenivasan, Katepalli R. Proc Natl Acad Sci U S A Physical Sciences The global transport of heat and momentum in turbulent convection is constrained by thin thermal and viscous boundary layers at the heated and cooled boundaries of the system. This bottleneck is thought to be lifted once the boundary layers themselves become fully turbulent at very high values of the Rayleigh number [Formula: see text] —the dimensionless parameter that describes the vigor of convective turbulence. Laboratory experiments in cylindrical cells for [Formula: see text] have reported different outcomes on the putative heat transport law. Here we show, by direct numerical simulations of three-dimensional turbulent Rayleigh–Bénard convection flows in a slender cylindrical cell of aspect ratio [Formula: see text] , that the Nusselt number—the dimensionless measure of heat transport—follows the classical power law of [Formula: see text] up to [Formula: see text]. Intermittent fluctuations in the wall stress, a blueprint of turbulence in the vicinity of the boundaries, manifest at all [Formula: see text] considered here, increasing with increasing [Formula: see text] , and suggest that an abrupt transition of the boundary layer to turbulence does not take place. National Academy of Sciences 2020-04-07 2020-03-25 /pmc/articles/PMC7149414/ /pubmed/32213591 http://dx.doi.org/10.1073/pnas.1922794117 Text en Copyright © 2020 the Author(s). Published by PNAS. https://creativecommons.org/licenses/by-nc-nd/4.0/ https://creativecommons.org/licenses/by-nc-nd/4.0/This open access article is distributed under Creative Commons Attribution-NonCommercial-NoDerivatives License 4.0 (CC BY-NC-ND) (https://creativecommons.org/licenses/by-nc-nd/4.0/) .
spellingShingle Physical Sciences
Iyer, Kartik P.
Scheel, Janet D.
Schumacher, Jörg
Sreenivasan, Katepalli R.
Classical 1/3 scaling of convection holds up to Ra = 10(15)
title Classical 1/3 scaling of convection holds up to Ra = 10(15)
title_full Classical 1/3 scaling of convection holds up to Ra = 10(15)
title_fullStr Classical 1/3 scaling of convection holds up to Ra = 10(15)
title_full_unstemmed Classical 1/3 scaling of convection holds up to Ra = 10(15)
title_short Classical 1/3 scaling of convection holds up to Ra = 10(15)
title_sort classical 1/3 scaling of convection holds up to ra = 10(15)
topic Physical Sciences
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7149414/
https://www.ncbi.nlm.nih.gov/pubmed/32213591
http://dx.doi.org/10.1073/pnas.1922794117
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