Abstract
Using direct numerical simulations of Rayleigh–Bénard convection (RBC), we perform a comparative study of the spectra and fluxes of energy and entropy, and the scaling of large-scale quantities for large and infinite Prandtl numbers in two (2D) and three (3D) dimensions. We observe close similarities between the 2D and 3D RBC, in particular, the kinetic energy spectrum E u (k)∼k −13/3, and the entropy spectrum exhibits a dual branch with a dominant k −2 spectrum. We showed that the dominant Fourier modes in 2D and 3D flows are very close. Consequently, the 3D RBC is quasi-two-dimensional, which is the reason for the similarities between the 2D and 3D RBC for large and infinite Prandtl numbers.
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Acknowledgements
The numerical simulations were performed at HPC and Newton clusters of IIT Kanpur, and at Param Yuva cluster of CDAC Pune. This work was supported by a research grant SERB /F/3279/2013-14 from Science and Engineering Research Board, India. The authors thank Supriyo Paul for useful comments and sharing his earlier results on 2D RBC. The authors also thank A Kumar for providing help in flow visualization.
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PANDEY, A., VERMA, M.K., CHATTERJEE, A.G. et al. Similarities between 2D and 3D convection for large Prandtl number. Pramana - J Phys 87, 13 (2016). https://doi.org/10.1007/s12043-016-1204-z
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DOI: https://doi.org/10.1007/s12043-016-1204-z