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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...
Autores principales: | , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
National Academy of Sciences
2020
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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. |
format | Online Article Text |
id | pubmed-7149414 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2020 |
publisher | National Academy of Sciences |
record_format | MEDLINE/PubMed |
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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