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dc.contributor.authorCarton, Xavier
dc.contributor.authorReinaud, Jean Noel
dc.contributor.authorVic, Armand
dc.contributor.authorGula, Jonathan
dc.date.accessioned2024-04-09T09:30:07Z
dc.date.available2024-04-09T09:30:07Z
dc.date.issued2024-04-06
dc.identifier300144553
dc.identifierce65946e-0e72-40a3-8d52-cca41a92aaf3
dc.identifier85189965479
dc.identifier.citationCarton , X , Reinaud , J N , Vic , A & Gula , J 2024 , ' The nonlinear evolution of two surface quasi-geostrophic vortices ' , Geophysical and Astrophysical Fluid Dynamics , vol. Latest Articles . https://doi.org/10.1080/03091929.2024.2330646en
dc.identifier.issn0309-1929
dc.identifier.otherORCID: /0000-0001-5449-6628/work/157578698
dc.identifier.urihttps://hdl.handle.net/10023/29619
dc.descriptionFunding: This work was supported by Ecole Normale Superieure de Rennes [PhD grant to Armand Vic].en
dc.description.abstractWe investigate numerically the evolution of a baroclinic vortex in a two-level surface quasi-geostrophic model. The vortex is composed of two circular patches of uniform buoyancy, one located at each level. We vary the vortex radii, the magnitude of buoyancy, and the vertical distance between the two levels. We also study different radial profiles of buoyancy for each vortex. This paper considers two main situations: firstly, initially columnar vortices with like-signed buoyancies. These vortices are contra-rotating, are linearly unstable and may break. Secondly, we consider initially tilted vortices with opposite-signed buoyancies, which may align vertically. Numerical experiments show that (1) identical contra-rotating vortices break into hetons when initially perturbed by low azimuthal modes; (2) unstable, vertically asymmetric, contra-rotating vortices can stabilise nonlinearly more often than vertically symmetric ones, and can form quasi-steady baroclinic tripoles; (3) co-rotating vortices can align when the two levels are close to each other vertically, and when the vortices are initially horizontally distant from each other by less than three radii; (4) for initially more distant vortices, two such vortices rotate around the plane center; (5) in all cases, the vortex boundaries are disturbed by Rossby waves. These results compare favorably to earlier results with internal quasi-geostrophic vortices. Further modelling efforts may extend the present study to fully three dimensional ocean dynamics.
dc.format.extent27
dc.format.extent1593684
dc.language.isoeng
dc.relation.ispartofGeophysical and Astrophysical Fluid Dynamicsen
dc.subjectTwo-level modelen
dc.subjectSurface quasi-geostrophyen
dc.subjectVortex stabilityen
dc.subjectBurger numberen
dc.subjectModal analysisen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQCen
dc.titleThe nonlinear evolution of two surface quasi-geostrophic vorticesen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doi10.1080/03091929.2024.2330646
dc.description.statusPeer revieweden


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