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dc.contributor.authorMckiver, William J.
dc.contributor.authorDritschel, David G.
dc.date.accessioned2017-02-04T00:32:51Z
dc.date.available2017-02-04T00:32:51Z
dc.date.issued2016-09
dc.identifier.citationMckiver , W J & Dritschel , D G 2016 , ' Balanced solutions for an ellipsoidal vortex in a rotating stratified flow ' , Journal of Fluid Mechanics , vol. 802 , pp. 333-358 . https://doi.org/10.1017/jfm.2016.462en
dc.identifier.issn0022-1120
dc.identifier.otherPURE: 245112796
dc.identifier.otherPURE UUID: afcaaef2-cd85-4d21-9592-d37c2422f6d1
dc.identifier.otherScopus: 84982712474
dc.identifier.otherWOS: 000381020500019
dc.identifier.otherORCID: /0000-0001-6489-3395/work/64697795
dc.identifier.urihttp://hdl.handle.net/10023/10227
dc.descriptionSupport for this research has come from the UK Engineering and Physical Sciences Research Council (grant number EP/H001794/1).en
dc.description.abstractWe consider the motion of a single ellipsoidal vortex with uniform potential vorticity in a rotating stratified fluid at finite Rossby number . Building on previous solutions obtained under the quasi-geostrophic approximation (at first order in ), we obtain analytical solutions for the balanced part of the flow at . These solutions capture important ageostrophic effects giving rise to an asymmetry in the evolution of cyclonic and anticyclonic vortices. Previous work has shown that, if the velocity field induced by an ellipsoidal vortex only depends linearly on spatial coordinates inside the vortex, i.e. , then the dynamics reduces markedly to a simple matrix equation. The instantaneous vortex shape and orientation are encapsulated in a symmetric matrix , which is acted upon by the flow matrix to provide the vortex evolution. Under the quasi-geostrophic approximation, the flow matrix is determined by inverting the potential vorticity to obtain the streamfunction via Poisson's equation, which has a known analytical solution depending on elliptic integrals. Here we show that higher-order balanced solutions, up to second order in the Rossby number, can also be calculated analytically. However, in this case there is a vector potential that requires the solution of three Poisson equations for each of its components. The source terms for these equations are independent of spatial coordinates within the ellipsoid, depending only on the elliptic integrals solved at the leading, quasi-geostrophic order. Unlike the quasi-geostrophic case, these source terms do not in general vanish outside the ellipsoid and have an inordinately complicated dependence on spatial coordinates. In the special case of an ellipsoid whose axes are aligned with the coordinate axes, we are able to derive these source terms and obtain the full analytical solution to the three Poisson equations. However, if one considers the homogeneous case, whereby the outer source terms are neglected, one can obtain an approximate solution having a compact matrix form analogous to the leading-order quasi-geostrophic case. This approximate solution proves to be highly accurate for the general case of an arbitrarily oriented ellipsoid, as verified through comparisons of the solutions with solutions obtained from numerical simulations of an ellipsoid using an accurate nonlinear balance model, even at moderate Rossby numbers.
dc.format.extent26
dc.language.isoeng
dc.relation.ispartofJournal of Fluid Mechanicsen
dc.rights© 2016, Cambridge University Press. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at journals.cambridge.org / https://dx.doi.org/10.1017/jfm.2016.462en
dc.subjectGeophysical and geological flowsen
dc.subjectGeostrophic turbulenceen
dc.subjectVortex dynamicsen
dc.subjectQA Mathematicsen
dc.subjectQC Physicsen
dc.subjectCondensed Matter Physicsen
dc.subjectMechanics of Materialsen
dc.subjectMechanical Engineeringen
dc.subjectT-NDASen
dc.subject.lccQAen
dc.subject.lccQCen
dc.titleBalanced solutions for an ellipsoidal vortex in a rotating stratified flowen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.contributor.institutionUniversity of St Andrews.School of Mathematics and Statisticsen
dc.contributor.institutionUniversity of St Andrews.Marine Alliance for Science & Technology Scotlanden
dc.contributor.institutionUniversity of St Andrews.Scottish Oceans Instituteen
dc.identifier.doihttps://doi.org/10.1017/jfm.2016.462
dc.description.statusPeer revieweden
dc.date.embargoedUntil2017-02-03


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