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dc.contributor.authorBurgess, B. H.
dc.contributor.authorScott, R. K.
dc.date.accessioned2017-06-16T23:34:07Z
dc.date.available2017-06-16T23:34:07Z
dc.date.issued2017-01
dc.identifier.citationBurgess , B H & Scott , R K 2017 , ' Scaling theory for vortices in the two-dimensional inverse energy cascade ' Journal of Fluid Mechanics , vol. 811 , pp. 742-756 . https://doi.org/10.1017/jfm.2016.756en
dc.identifier.issn0022-1120
dc.identifier.otherPURE: 248699478
dc.identifier.otherPURE UUID: b56dcc32-9121-4cc3-a95e-16514daffd71
dc.identifier.otherScopus: 85027926454
dc.identifier.otherORCID: /0000-0001-9297-8003/work/54516628
dc.identifier.otherORCID: /0000-0001-5624-5128/work/55378725
dc.identifier.urihttp://hdl.handle.net/10023/11014
dc.descriptionB.H.B. is supported by the Natural Environment Research Council grant NE/M014983/1.en
dc.description.abstractWe propose a new similarity theory for the two-dimensional inverse energy cascade and the coherent vortex population it contains when forced at intermediate scales. Similarity arguments taking into account enstrophy conservation and a prescribed constant energy injection rate such that E∼t yield three length scales, lω, lE and lψ, associated with the vorticity field, energy peak and streamfunction, and predictions for their temporal evolutions, t1/2, t and t3/2, respectively. We thus predict that vortex areas grow linearly in time, A∼l2ω∼t, while the spectral peak wavenumber kE ≡ 2πl−1E ∼ t−1. We construct a theoretical framework involving a three-part, time-evolving vortex number density distribution, n(A) ∼ tαiA−ri,  i ∈ 1,2,3. Just above the forcing scale (i =1) there is a forcing-equilibrated scaling range in which the number of vortices at fixed A is constant and vortex ‘self-energy’ Evcm = (2D)−1∫ωv2A2n(A) dA is conserved in A-space intervals [μA0(t), A0(t)] comoving with the growth in vortex area, A0(t) ∼ t. In this range, α1 = 0 and n(A) ∼ A−3. At intermediate scales (i = 2) sufficiently far from the forcing and the largest vortex, there is a range with a scale-invariant vortex size distribution. We predict that in this range the vortex enstrophy Zvcm = (2D)−1∫ ωv2An(A)dA is conserved and n(A) ∼ t−1A−1. The final range (i = 3), which extends over the largest vortex-containing scales, conserves σvcm = (2D)−1∫ ωv2n(A)dA. If ωv2 is constant in time, this is equivalent to conservation of vortex number Nvcm =∫ n(A)dA. This regime represents a ‘front’ of sparse vortices, which are effectively point-like; in this range we predict n(A) ∼ tr3−1A−r3. Allowing for time-varying ωv2 results in a small but significant correction to these temporal dependences. High-resolution numerical simulations verify the predicted vortex and spectral peak growth rates, as well as the theoretical picture of the three scaling ranges in the vortex population. Vortices steepen the energy spectrum E(k) past the classical k−5/3 scaling in the range k ∈ [kf , kv], where kv is the wavenumber associated with the largest vortex, while at larger scales the slope approaches −5/3. Though vortices disrupt the classical scaling, their number density distribution and evolution reveal deeper and more complex scale invariance, and suggest an effective theory of the inverse cascade in terms of vortex interactions.en
dc.format.extent15en
dc.language.isoeng
dc.relation.ispartofJournal of Fluid Mechanicsen
dc.rights© 2016, 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 may differ slightly from the final published version. The final published version of this work is available at www.cambridge.org / https://doi.org/10.1017/jfm.2016.756en
dc.subjectTurbulence simulationen
dc.subjectTurbulence theoryen
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.titleScaling theory for vortices in the two-dimensional inverse energy cascadeen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1017/jfm.2016.756
dc.description.statusPeer revieweden
dc.date.embargoedUntil16-06-20


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