Breakdown of the large-scale wind in \Gamma=1/2 rotating Rayleigh-B\'enard flow
Richard J. A. M. Stevens, Herman J. H. Clercx, Detlef Lohse

TL;DR
This study investigates the flow structures in rotating Rayleigh-Bénard convection at aspect ratio 1/2, revealing that vertically-aligned vortices create a sinusoidal temperature pattern near the sidewall, unlike the random vortices at aspect ratio 1.
Contribution
The paper demonstrates through simulations that the spatial organization of vortices at aspect ratio 1/2 produces a sinusoidal temperature signature, clarifying flow differences from aspect ratio 1.
Findings
Vertically-aligned vortices form a sinusoidal temperature pattern at aspect ratio.
At aspect ratio, vortices are randomly distributed.
The flow structure transition explains heat transport behavior.
Abstract
Experiments and simulations of rotating Rayleigh-B\'enard convection in cylindrical samples have revealed an increase in heat transport with increasing rotation rate. This heat transport enhancement is intimately related to a transition in the turbulent flow structure from a regime dominated by a large-scale circulation (LSC), consisting of a single convection roll, at no or weak rotation to a regime dominated by vertically-aligned vortices at strong rotation. For a sample with an aspect ratio \Gamma = D/L = 1 (D is the sample diameter and L its height) the transition between the two regimes is indicated by a strong decrease in the LSC strength. In contrast, for \Gamma = 1/2 Weiss and Ahlers [J. Fluid Mech. {\bf{688}}, 461 (2011)] revealed the presence of a LSC-like sidewall temperature signature beyond the critical rotation rate. They suggested that this might be due to the formation…
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