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| Journal Article | FZJ-2026-03013 |
; ; ; ;
2024
Cambridge Univ. Press
Cambridge [u.a.]
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Please use a persistent id in citations: doi:10.1017/jfm.2024.853 doi:10.34734/FZJ-2026-03013
Abstract: We study the dynamics of thermal and momentum boundary regions in three-dimensionaldirect numerical simulations of Rayleigh–Bénard convection for the Rayleigh-numberrange $105 ≤ Ra ≤ 1011$ and $Pr = 0.7$. Using a Cartesian slab with horizontal periodicboundary conditions and an aspect ratio of 4, we obtain statistical homogeneity in thehorizontal x- and y-directions, thus approximating best an extended convection layerrelevant for most geo- and astrophysical flow applications. We observe upon canonical useof combined long-time and area averages, with averaging periods of at least 100 free-falltimes, that a global coherent mean flow is practically absent and that the magnitude ofthe velocity fluctuations is larger than the mean by up to 2 orders of magnitude. Thevelocity field close to the wall is a collection of differently oriented local shear-dominatedflow patches interspersed by extensive shear-free incoherent regions which can be aslarge as the whole cross-section, unlike for a closed cylindrical convection cell of aspectratio of the order 1. The incoherent regions occupy a 60 % area fraction for all Rayleighnumbers investigated here. Rather than resulting in a pronounced mean flow with smallfluctuations about such a mean, as found in small-aspect-ratio convection, the velocityfield is dominated by strong fluctuations of all three components around a non-existent orweak mean. We discuss the consequences of these observations for convection layers withlarger aspect ratios, including boundary layer instabilities and the resulting turbulent heattransport.
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