{"title":"Flux scaling in Rayleigh Bénard convection: a local boundary layer analysis","authors":"Prafulla P. Shevkar, Baburaj A. Puthenveettil","doi":"arxiv-2409.00930","DOIUrl":null,"url":null,"abstract":"We study the effect of shear due to the large scale flow (LSF) on the heat\nflux in Rayleigh B'enard convection for a range of near-plate Rayleigh numbers\n$8\\times 10^7 \\leq Ra_w \\leq 5\\times 10^{14}$, by studying its effect on the\nlocal boundary layers (BLs) on either sides of the plumes, which are much\nthinner than the global shear BL created by the LSF velocity $V_F$. Considering\nthese local BLs forced externally by the LSF, we obtain a fifth order algebraic\nequation for the local boundary layer thicknesses. Solving these equations\nnumerically using $Re$ relations for aspect ratios $\\Gamma=1$ and 0.5, we\nobtain the variation of the local BL thicknesses with the longitudinal distance\nfor various $Ra_w$. We find that the average shear acting on the edges of these\nlocal BLs ($\\overline{u|}_{z=\\delta}$) increases as $\\overline{u|}_{z=\\delta}\n\\sim Ra_w^{1/3}$ for $8\\times 10^7\\leq Ra_w \\leq 10^{12}$ at $\\Gamma=1$, and as\n$\\overline{u|}_{z=\\delta} \\sim Ra_w^{0.38}$ for $1\\times 10^{11}\\leq Ra_w \\leq\n5\\times 10^{14}$ at $\\Gamma=0.5$. We then estimate the average local thermal BL\nthickness to find the global Nusselt number $Nu$.We find that $Nu\\sim Ra_w^m$,\nwhere $m\\approx 0.327$ for $8\\times 10^7 \\leq Ra_w \\leq 1\\times 10^{12}$ at\n$\\Gamma=1$, and $m=0.33$ for $1\\times10^{11}\\leq Ra_w \\leq 5\\times10^{14}$ at\n$\\Gamma=0.5$. Inspite of the increasing shear on these BLs with increasing\n$Ra_w$, we then surprisingly obtain the classical 1/3 scaling of flux since the\nshear forcing acting on those BLs remains sub-dominant compared to the NCBL\nvelocities ($V_{bl}$) within these BLs, upto $Ra_w\\leq 5\\times10^{14}$.","PeriodicalId":501125,"journal":{"name":"arXiv - PHYS - Fluid Dynamics","volume":"200 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Fluid Dynamics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.00930","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We study the effect of shear due to the large scale flow (LSF) on the heat
flux in Rayleigh B'enard convection for a range of near-plate Rayleigh numbers
$8\times 10^7 \leq Ra_w \leq 5\times 10^{14}$, by studying its effect on the
local boundary layers (BLs) on either sides of the plumes, which are much
thinner than the global shear BL created by the LSF velocity $V_F$. Considering
these local BLs forced externally by the LSF, we obtain a fifth order algebraic
equation for the local boundary layer thicknesses. Solving these equations
numerically using $Re$ relations for aspect ratios $\Gamma=1$ and 0.5, we
obtain the variation of the local BL thicknesses with the longitudinal distance
for various $Ra_w$. We find that the average shear acting on the edges of these
local BLs ($\overline{u|}_{z=\delta}$) increases as $\overline{u|}_{z=\delta}
\sim Ra_w^{1/3}$ for $8\times 10^7\leq Ra_w \leq 10^{12}$ at $\Gamma=1$, and as
$\overline{u|}_{z=\delta} \sim Ra_w^{0.38}$ for $1\times 10^{11}\leq Ra_w \leq
5\times 10^{14}$ at $\Gamma=0.5$. We then estimate the average local thermal BL
thickness to find the global Nusselt number $Nu$.We find that $Nu\sim Ra_w^m$,
where $m\approx 0.327$ for $8\times 10^7 \leq Ra_w \leq 1\times 10^{12}$ at
$\Gamma=1$, and $m=0.33$ for $1\times10^{11}\leq Ra_w \leq 5\times10^{14}$ at
$\Gamma=0.5$. Inspite of the increasing shear on these BLs with increasing
$Ra_w$, we then surprisingly obtain the classical 1/3 scaling of flux since the
shear forcing acting on those BLs remains sub-dominant compared to the NCBL
velocities ($V_{bl}$) within these BLs, upto $Ra_w\leq 5\times10^{14}$.