Show simple item record

Instabilities of interacting vortex rings generated by an oscillating disk

dc.creatorDeng, Jian
dc.creatorTeng, Lubao
dc.creatorCaulfield, Colm-cille Patrick
dc.creatorMao, Xuerui
dc.date.accessioned2016-08-26
dc.date.accessioned2018-11-24T23:19:23Z
dc.date.available2016-10-21T12:23:56Z
dc.date.available2018-11-24T23:19:23Z
dc.date.issued2016-09-14
dc.identifierhttps://www.repository.cam.ac.uk/handle/1810/260863
dc.identifier.urihttp://repository.aust.edu.ng/xmlui/handle/123456789/3437
dc.description.abstractWe propose a natural model to probe in a controlled fashion the instability of interacting vortex rings shed from the edge of an oblate spheroid disk of major diameter $\textit{c}$, undergoing oscillations of frequency $\textit{f}$$_{0}$ and amplitude $\textit{A}$. We perform a Floquet stability analysis to determine the characteristics of the instability modes, which depend strongly on the azimuthal (integer) wave number $\textit{m}$. We vary two key control parameters, the Keulegan-Carpenter number $\textit{K}$$_{c}$=$\textbf{2}$$_{π}$$\textit{A}$/$\textit{c}$ and the Stokes number $\textit{β}$=$\textbf{f}$$_{0}$$\textbf{c}$$^{2}$/$\textit{ν}$, where $\textit{ν}$ is the kinematic viscosity of the fluid. We observe two distinct flow regimes. First, for sufficiently small $\textit{β}$, and hence low frequency of oscillation corresponding to relatively weak interaction between sequentially shedding vortex rings, symmetry breaking occurs directly to a single unstable mode with $\textit{m}$=1. Second, for sufficiently large yet fixed values of $\textit{β}$, corresponding to a higher oscillation frequency and hence stronger ring-ring interaction, the onset of asymmetry is predicted to occur due to two branches of high $\textit{m}$ instabilities as the amplitude is increased, with $\textit{m}$=1 structures being dominant only for sufficiently large values of K$_{c}$. These two branches can be distinguished by the phase properties of the vortical structures above and below the disk. The region in ($\textit{K}$$_{c}$,$\textit{β}$) parameter space where these two high $\textit{m}$ instability branches arise can be described accurately in terms of naturally defined Reynolds numbers, using appropriately chosen characteristic length scales. We subsequently carry out direct numerical simulations of the fully three-dimensional flow to verify the principal characteristics of the Floquet analysis, in particular demonstrating that high wave-number symmetry-breaking generically occurs when vortex rings sequentially interact sufficiently strongly.
dc.languageen
dc.publisherAmerican Physical Society
dc.publisherPhysical Review E
dc.titleInstabilities of interacting vortex rings generated by an oscillating disk
dc.typeArticle


Files in this item

FilesSizeFormatView
Deng_et_al-2016-American_Physical_Society-AM.pdf1.864Mbapplication/pdfView/Open

This item appears in the following Collection(s)

Show simple item record