Bénard convection in a slowly rotating penny-shaped cylinder subject to constant heat flux boundary conditions

• Published in: Journal of fluid mechanics Vol. 951; no. A5
• Main Authors: Soward, A.M., Oruba, L., Dormy, E.
• Format: Journal Article
• Language: English
• Published: Cambridge, UK Cambridge University Press 25.11.2022; Cambridge University Press (CUP)
• Subjects: Angular momentum; Angular velocity; Asymptotic methods; Asymptotic series; Atmospheric and Oceanic Physics; Boundary conditions; Boussinesq approximation; Boussinesq equations; Convection; Cylinders; Direct numerical simulation; Equations of motion; Fluid Dynamics; Heat; Heat flux; Heat transfer; JFM Papers; Methods; Momentum; Photosystem I; Physics; Prandtl number; Rayleigh number; Rotating cylinders; Symmetry; Velocity; rotating flows; atmospheric flows; Bénard convection
• DOI: 10.1017/jfm.2022.761
• ISSN: 0022-1120

We consider axisymmetric Boussinesq convection in a shallow cylinder of radius $L$ and depth $H (\ll L)$, which rotates with angular velocity $\varOmega$ about its axis of symmetry aligned to the vertical. Constant heat flux boundary conditions, top and bottom, are adopted, for which the onset of instability occurs on a long horizontal length scale provided that $\varOmega$ is sufficiently small. We investigate the nonlinear development by well-established two-scale asymptotic expansion methods. Comparisons of the results with the direct numerical simulations (DNS) of the primitive governing equations are good at sufficiently large Prandtl number $\sigma$. As $\sigma$ is reduced, the finite amplitude range of applicability of the asymptotics reduces in concert. Though the large meridional convective cell, predicted by the DNS, is approximated adequately by the asymptotics, the azimuthal flow fails almost catastrophically, because of significant angular momentum transport at small $\sigma$, exacerbated by the cylindrical geometry. To appraise the situation, we propose hybrid methods that build on the meridional streamfunction $\psi$ derived from the asymptotics. With $\psi$ given, we solve the now linear azimuthal equation of motion for the azimuthal velocity $v$ by DNS. Our ‘hybrid’ methods enable us to explain features of the flow at large Rayleigh number, found previously by Oruba et al. (J. Fluid Mech., vol. 812, 2017, pp. 890–904).