Formation of eyes in large-scale cyclonic vortices
Ludivine Oruba, Peter Davidson, Emmanuel Dormy

TL;DR
This paper uses numerical simulations to investigate the formation of eye-like structures in large-scale cyclonic vortices, identifying key parameters and conditions that lead to eye formation.
Contribution
It provides new scaling laws and criteria for eye formation in rotating convection models inspired by tropical cyclones.
Findings
An eye forms at the vortex center with a reversed poloidal flow.
Flow velocity scales with ( extalpha g eta)^{1/2}H.
Conditions for eye formation depend on Re, Ro, and Ekman number bounds.
Abstract
We present numerical simulations of steady, laminar, axisymmetric convection of a Boussinesq fluid in a shallow, rotating, cylindrical domain. The flow is driven by an imposed vertical heat flux and shaped by the background rotation of the domain. The geometry is inspired by that of tropical cyclones and the global flow pattern consists of a shallow, swirling vortex combined with a poloidal flow in the r-z plane which is predominantly inward near the bottom boundary and outward along the upper surface. Our numerical experiments confirm that, as suggested by Oruba et al 2017, an eye forms at the centre of the vortex which is reminiscent of that seen in a tropical cyclone and is characterised by a local reversal in the direction of the poloidal flow. We establish scaling laws for the flow and map out the conditions under which an eye will, or will not, form. We show that, to leading…
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