Subcritical convection of liquid metals in a rotating sphere using a quasi-geostrophic model
Celine Guervilly, Philippe Cardin

TL;DR
This study investigates nonlinear convection in a rapidly rotating sphere with liquid metal properties, revealing two distinct convection branches, subcritical behavior at low Ekman numbers, and the influence of Prandtl number on convection dynamics.
Contribution
It introduces a quasi-geostrophic numerical model to identify and analyze two convection branches, including a novel subcritical strong branch at low Ekman numbers, in liquid metal-like conditions.
Findings
Two convection branches identified: weak supercritical and strong subcritical.
Subcritical convection occurs at Ekman numbers around 10^{-8}.
Hysteresis and nonlinear oscillations are observed near convection onset.
Abstract
We study nonlinear convection in a rapidly rotating sphere with internal heating for values of the Prandtl number relevant for liquid metals (). We use a numerical model based on the quasi-geostrophic approximation, in which variations of the axial vorticity along the rotation axis are neglected, whereas the temperature field is fully three-dimensional. We identify two separate branches of convection close to onset: (i) a well-known weak branch for Ekman numbers greater than , which is continuous at the onset (supercritical bifurcation) and consists of thermal Rossby waves, and (ii) a novel strong branch at lower Ekman numbers, which is discontinuous at the onset. The strong branch becomes subcritical for Ekman numbers of the order of . On the strong branch, the Reynolds number of the flow is greater than , and a strong zonal flow with…
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