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dc.contributor.authorReinaud, Jean Noel
dc.contributor.authorDritschel, David Gerard
dc.date.accessioned2019-07-21T23:41:28Z
dc.date.available2019-07-21T23:41:28Z
dc.date.issued2019-03-25
dc.identifier.citationReinaud , J N & Dritschel , D G 2019 , ' The stability and nonlinear evolution of quasi-geostrophic toroidal vortices ' , Journal of Fluid Mechanics , vol. 863 , pp. 60-78 . https://doi.org/10.1017/jfm.2018.1013en
dc.identifier.issn0022-1120
dc.identifier.otherPURE: 256888764
dc.identifier.otherPURE UUID: 8fdd4ac8-a5af-423c-8752-57e71cb27180
dc.identifier.otherORCID: /0000-0001-5449-6628/work/53214493
dc.identifier.otherScopus: 85060366607
dc.identifier.otherWOS: 000458502400001
dc.identifier.otherORCID: /0000-0001-6489-3395/work/64697796
dc.identifier.urihttps://hdl.handle.net/10023/18145
dc.description.abstractWe investigate the linear stability and nonlinear evolution of a three-dimensional toroidal vortex of uniform potential vorticity under the quasi-geostrophic approximation. The torus can undergo a primary instability leading to the formation of a circular array of vortices, whose radius is approximately the same as the major radius of the torus. This occurs for azimuthal instability mode numbers m ≥ 3, on sufficiently thin tori. The number of vortices corresponds to the azimuthal mode number of the most unstable mode growing on the torus. This value of m depends on the ratio of the torus’ major radius to its minor radius, with thin tori favouring high mode m values. The resulting array is stable when m = 4 and m = 5 and unstable when m = 3 and m ≥ 6. When m = 3 the array has barely formed before it collapses towards its centre with the ejection of filamentary debris. When m = 6 the vortices exhibit oscillatory staggering, and when m ≥ 7 they exhibit irregular staggering followed by substantial vortex migration, e.g. of one vortex to the centre when m = 7. We also investigate the effect of an additional vortex located at the centre of the torus. This vortex alters the stability properties of the torus as well as the stability properties of the circular vortex array formed from the primary toroidal instability. We show that a like-signed central vortex may stabilise a circular m-vortex array with m ≥ 6.
dc.format.extent19
dc.language.isoeng
dc.relation.ispartofJournal of Fluid Mechanicsen
dc.rightsCopyright © 2018, Cambridge University Press. This work has been made available online in accordance with the publisher's policies. This is the author created accepted version manuscript following peer review and as such may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1017/jfm.2018.1013en
dc.subjectQuasi-geostrophic flowsen
dc.subjectVortex instabilityen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectT-NDASen
dc.subjectBDCen
dc.subjectR2Cen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe stability and nonlinear evolution of quasi-geostrophic toroidal vorticesen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.contributor.institutionUniversity of St Andrews. Scottish Oceans Instituteen
dc.contributor.institutionUniversity of St Andrews. Marine Alliance for Science & Technology Scotlanden
dc.identifier.doihttps://doi.org/10.1017/jfm.2018.1013
dc.description.statusPeer revieweden
dc.date.embargoedUntil2020-01-22


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