Aspect Ratio Dependence of Heat Transfer in a Cylindrical Rayleigh-Bénard Cell
Guenter Ahlers, Eberhard Bodenschatz, R.A. Hartmann, Xiaozhou He, Detlef Lohse, Philipp Reiter, Richard J. A. M. Stevens, Roberto Verzicco, Marcel Wedi, Stephan Weiss, Xuan Zhang, Lukas Zwirner, Olga Shishkina
Abstract
While the heat transfer and the flow dynamics in a cylindrical Rayleigh-B\'enard (RB) cell are rather independent of the aspect ratio $\mathrm{\ensuremath{\Gamma}}$ (diameter/height) for large $\mathrm{\ensuremath{\Gamma}}$, a small-$\mathrm{\ensuremath{\Gamma}}$ cell considerably stabilizes the flow and thus affects the heat transfer. Here, we first theoretically and numerically show that the critical Rayleigh number for the onset of convection at given $\mathrm{\ensuremath{\Gamma}}$ follows ${\mathrm{Ra}}_{c,\mathrm{\ensuremath{\Gamma}}}\ensuremath{\sim}{\mathrm{Ra}}_{c,\ensuremath{\infty}}(1+C{\mathrm{\ensuremath{\Gamma}}}^{\ensuremath{-}2}{)}^{2}$, with $C\ensuremath{\lesssim}1.49$ for Oberbeck-Boussinesq (OB) conditions. We then show that, in a broad aspect ratio range $(1/32)\ensuremath{\le}\mathrm{\ensuremath{\Gamma}}\ensuremath{\le}32$, the rescaling $\mathrm{Ra}\ensuremath{\rightarrow}{\mathrm{Ra}}_{\ensuremath{\ell}}\ensuremath{\equiv}\mathrm{Ra}[{\mathrm{\ensuremath{\Gamma}}}^{2}/(C+{\mathrm{\ensuremath{\Gamma}}}^{2}){]}^{3/2}$ collapses various OB numerical and almost-OB experimental heat transport data $\mathrm{Nu}(\mathrm{Ra},\mathrm{\ensuremath{\Gamma}})$. Our findings predict the $\mathrm{\ensuremath{\Gamma}}$ dependence of the onset of the ultimate regime ${\mathrm{Ra}}_{u,\mathrm{\ensuremath{\Gamma}}}\ensuremath{\sim}[{\mathrm{\ensuremath{\Gamma}}}^{2}/(C+{\mathrm{\ensuremath{\Gamma}}}^{2}){]}^{\ensuremath{-}3/2}$ in the OB case. This prediction is consistent with almost-OB experimental results (which only exist for $\mathrm{\ensuremath{\Gamma}}=1$, $1/2$, and $1/3$) for the transition in OB RB convection and explains why, in small-$\mathrm{\ensuremath{\Gamma}}$ cells, much larger Ra (namely, by a factor ${\mathrm{\ensuremath{\Gamma}}}^{\ensuremath{-}3}$) must be achieved to observe the ultimate regime.