High-wavenumber steady solutions of two-dimensional Rayleigh--B\'enard convection between stress-free boundaries

Abstract

Recent investigations show that steady solutions share many features with turbulent Rayleigh--B\'enard convection (RBC) and form the state space skeleton of turbulent dynamics. Previous computations of steady roll solutions in two-dimensional (2D) RBC between no-slip boundaries reveal that for fixed Rayleigh number RaRa and Prandtl number PrPr, the heat-flux-maximizing solution is always in the high-wavenumber regime. In this study, we explore the high-wavenumber steady convection roll solutions that bifurcate supercritically from the motionless conductive state for 2D RBC between stress-free boundaries. Our computations confirm the existence of a local heat-flux-maximizing solution in the high-wavenumber regime. To elucidate the asymptotic properties of this solution, we perform computations over eight orders of magnitude in the Rayleigh number, 108≀Ra≀1016.510^{8} \le Ra \le 10^{16.5}, and two orders of magnitude in the Prandtl number, 10βˆ’1≀Pr≀103/210^{-1} \leq Pr \leq 10^{3/2}. The numerical results indicate that as Raβ†’βˆžRa\to\infty, the local heat-flux-maximizing aspect ratio Ξ“locβˆ—β‰ƒRaβˆ’1/4\Gamma^*_{loc}\simeq Ra^{-1/4}, the Nusselt number Nu(Ξ“locβˆ—)≃Ra0.29Nu(\Gamma^*_{loc})\simeq Ra^{0.29}, and the Reynolds number Re(Ξ“locβˆ—)≃Prβˆ’1Ra2/5Re(\Gamma^*_{loc})\simeq Pr^{-1}Ra^{2/5}, with all prefactors depending on PrPr. Moreover, the interior flow of the local NuNu-maximizing solution can be well described by an analytical heat-exchanger solution, and the connection to the high-wavenumber asymptotic solution given by Blennerhassett & Bassom is discussed. With a fixed aspect ratio 0.06≀Γ≀π/50.06\le\Gamma\le\pi/5 at Pr=1Pr=1, however, our computations show that as RaRa increases, the steady rolls converge to the semi-analytical asymptotic solutions constructed by Chini & Cox, with scalings Nu∼Ra1/3Nu\sim Ra^{1/3} and Re∼Prβˆ’1Ra2/3Re\sim Pr^{-1}Ra^{2/3}. Finally, a phase diagram is delineated to gain a panorama of steady solutions in the high-Rayleigh-number-wavenumber plane

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