4.7 Article

The influence of the cell inclination on the heat transport and large-scale circulation in liquid metal convection

期刊

JOURNAL OF FLUID MECHANICS
卷 884, 期 -, 页码 -

出版社

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2019.935

关键词

Benard convection; convection in cavities; turbulent convection

资金

  1. Deutsche Forschungsgemeinschaft (DFG) [SPP 1881, Sh405/7]
  2. DFG [Sh405/4]

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Inclined turbulent thermal convection in liquid sodium is studied at large Rayleigh numbers Ra & 107 based on the results of both experimental measurements and high-resolution numerical simulations. For a direct comparison, the considered system parameters are set to be similar: Ra D 1 :67 107 in the direct numerical simulations (DNS), Ra D 1 :5 107 in the large-eddy simulations and Ra D 1 :42 107 in the experiments, while the Prandtl number of liquid sodium is very small (Pr 0:009). The cylindrical convection cell has an aspect ratio of one; one circular surface is heated, while the other one is cooled. Additionally, the cylinder is inclined with respect to gravity and the inclination angle varies from fi D 0ffi, which corresponds to Rayleigh-Benard convection (RBC), to fi D 90 ffi, as in a vertical convection (VC) set-up. Our study demonstrates quantitative agreement of the experimental and numerical results, in particular with respect to the global heat and momentum transport, temperature and velocity profiles, as well as the dynamics of the large-scale circulation (LSC). The DNS reveal that the twisting and sloshing of the LSC at small inclination angles periodically affects the instantaneous heat transport (up to 44% of the mean heat transport). The twisted LSC is associated with a weak heat transport, while the sloshing mode that brings together the hot and cold streams of the LSC is associated with a strong heat transport. The experiments show that the heat transport scales as Nu Ra0:22 in both limiting cases (RBC and VC) for Rayleigh numbers around Ra 107, while any inclination of the cell, 0 < fi 6 90ffi, leads to an increase of Nu.

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