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DOI | 10.1073/pnas.1806823115 |
Radiative heating achieves the ultimate regime of thermal convection | |
Lepot S.; Aumaître S.; Gallet B. | |
发表日期 | 2018 |
ISSN | 0027-8424 |
起始页码 | 8937 |
结束页码 | 8941 |
卷号 | 115期号:36 |
英文摘要 | The absorption of light or radiation drives turbulent convection inside stars, supernovae, frozen lakes, and Earth’s mantle. In these contexts, the goal of laboratory and numerical studies is to determine the relation between the internal temperature gradients and the heat flux transported by the turbulent flow. This is the constitutive law of turbulent convection, to be input into large-scale models of such natural flows. However, in contrast with the radiative heating of natural flows, laboratory experiments have focused on convection driven by heating and cooling plates; the heat transport is then severely restricted by boundary layers near the plates, which prevents the realization of the mixing length scaling law used in evolution models of geophysical and astrophysical flows. There is therefore an important discrepancy between the scaling laws measured in laboratory experiments and those used, e.g., in stellar evolution models. Here we provide experimental and numerical evidence that radiatively driven convection spontaneously achieves the mixing length scaling regime, also known as the “ultimate” regime of thermal convection. This constitutes a clear observation of this regime of turbulent convection. Our study therefore bridges the gap between models of natural flows and laboratory experiments. It opens an experimental avenue for a priori determinations of the constitutive laws to be implemented into models of geophysical and astrophysical flows, as opposed to empirical fits of these constitutive laws to the scarce observational data. © 2018 National Academy of Sciences. All Rights Reserved. |
英文关键词 | Geophysical and astrophysical fluid dynamics; Thermal convection; Turbulence |
语种 | 英语 |
scopus关键词 | article; boundary layer; cooling; heat; heating; thermodynamics |
来源期刊 | Proceedings of the National Academy of Sciences of the United States of America
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/158965 |
作者单位 | Lepot, S., Service de Physique de l’Etat Condensé, Commissariat à l’Energie Atomique (CEA Saclay), CNRS UMR 3680, Université Paris-Saclay, Gif-sur-Yvette, 91191, France; Aumaître, S., Service de Physique de l’Etat Condensé, Commissariat à l’Energie Atomique (CEA Saclay), CNRS UMR 3680, Université Paris-Saclay, Gif-sur-Yvette, 91191, France, Laboratoire de Physique, Ecole Normale Supérieure de Lyon, UMR CNRS 5672, Lyon, 69007, France; Gallet, B., Service de Physique de l’Etat Condensé, Commissariat à l’Energie Atomique (CEA Saclay), CNRS UMR 3680, Université Paris-Saclay, Gif-sur-Yvette, 91191, France |
推荐引用方式 GB/T 7714 | Lepot S.,Aumaître S.,Gallet B.. Radiative heating achieves the ultimate regime of thermal convection[J],2018,115(36). |
APA | Lepot S.,Aumaître S.,&Gallet B..(2018).Radiative heating achieves the ultimate regime of thermal convection.Proceedings of the National Academy of Sciences of the United States of America,115(36). |
MLA | Lepot S.,et al."Radiative heating achieves the ultimate regime of thermal convection".Proceedings of the National Academy of Sciences of the United States of America 115.36(2018). |
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