Effects of Rayleigh and Weber numbers on two-layer turbulent Rayleigh–Bénard convection

Journal Article (2024)
Author(s)

Andreas D. Demou (The Cyprus Institute)

Nicolò Scapin (KTH Royal Institute of Technology)

Marco Crialesi-Esposito (Università di Modena e Reggio Emilia)

Pedro Costa (TU Delft - Energy Technology, University of Iceland)

Filippo Spiga (NVIDIA)

Luca Brandt (Norwegian University of Science and Technology (NTNU), Politecnico di Torino, KTH Royal Institute of Technology)

DOI related publication
https://doi.org/10.1017/jfm.2024.805 Final published version
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Publication Year
2024
Language
English
Bibliographical Note
Green Open Access added to TU Delft Institutional Repository 'You share, we take care!' - Taverne project https://www.openaccess.nl/en/you-share-we-take-care Otherwise as indicated in the copyright section: the publisher is the copyright holder of this work and the author uses the Dutch legislation to make this work public.
Journal title
Journal of Fluid Mechanics
Volume number
996
Article number
A23
Downloads counter
210
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Abstract

This study presents direct numerical simulation results of two-layer Rayleigh–Bénard convection, investigating the previously unexplored Rayleigh–Weber parameter space 106≤Ra≤108 and 102≤We≤103. Global properties, such as the Nusselt and Reynolds numbers, are compared against the extended Grossmann–Lohse theory for two fluid layers, confirming a weak Weber number dependence for all global quantities and considerably larger Reynolds numbers in the lighter fluid. Statistics of the flow reveal that the interface fluctuates more intensely for larger Weber and smaller Rayleigh numbers, something also reflected in the increased temperature root mean square values next to the interface. The dynamics of the deformed two-fluid interface is further investigated using spectral analysis. Temporal and spatial spectrum distributions reveal a capillary wave range at small Weber and large Rayleigh numbers, and a secondary energy peak at smaller Rayleigh numbers. Furthermore, the maxima of the space–time spectra lie in an intermediate dispersion regime, between the theoretical predictions for capillary and gravity-capillary waves, showing that the gravitational energy of the interfacial waves is strongly altered by temperature gradients.

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