Spatially localised doubly diffusive convection in an axisymmetric spherical shell
Paul M. Mannix, Cedric Beaume

TL;DR
This paper investigates the existence and properties of spatially localised doubly diffusive convection in an axisymmetric spherical shell using numerical simulations, revealing new localized solutions and bifurcation structures relevant to astrophysics.
Contribution
First numerical study of spatially localised doubly diffusive convection in spherical shells, identifying new solution families and bifurcation behaviors.
Findings
Multiple families of localised solutions ('convectons') identified.
Convection strength varies with latitude due to curved rolls.
Localised states arise via imperfect bifurcations, not periodic states.
Abstract
Doubly diffusive convection describes the fluid motion driven by the competition of temperature and salinity gradients diffusing at different rates. While the convective motions driven by these gradients usually occupy the entire domain, parameter regions exist where the convection is spatially localised. Although well-studied in planar geometries, spatially localised doubly diffusive convection has never been investigated in a spherical shell, a geometry of relevance to astrophysics. In this paper, numerical simulation is used to compute spatially localised solutions of doubly diffusive convection in an axisymmetric spherical shell. Several families of spatially localised solutions, named using variants of the word convecton, are found and their bifurcation diagram computed. The various convectons are distinguished by their symmetry and by whether they are localised at the poles or at…
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