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A numerical study of three-dimensional vortex ring instabilities: viscous corrections and early nonlinear stage

Published online by Cambridge University Press:  26 April 2006

Karim Shariff ,
Roberto Verzicco  and
Paolo Orlandi
Karim Shariff
Affiliation:
NASA-Ames Research Center, Moffett Field, CA 94035, USA
Roberto Verzicco
Affiliation:
Università di Roma ‘La Sapienza’ Dipartimento di Meccanica e Aeronautica, via Eudossiana n0 18, 00184 Roma, Italy
Paolo Orlandi
Affiliation:
Università di Roma ‘La Sapienza’ Dipartimento di Meccanica e Aeronautica, via Eudossiana n0 18, 00184 Roma, Italy
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Abstract

Finite-difference calculations with random and single-mode perturbations are used to study the three-dimensional instability of vortex rings. The basis of current understanding of the subject consists of a heuristic inviscid model (Widnall, Bliss & Tsai 1974) and a rigorous theory which predicts growth rates for thin-core uniform vorticity rings (Widnall & Tsai 1977). At sufficiently high Reynolds numbers the results correspond qualitatively to those predicted by the heuristic model: multiple bands of wavenumbers are amplified, each band having a distinct radial structure. However, a viscous correction factor to the peak inviscid growth rate is found. It is well described by the first term, 1 – α1(β)/Res, for a large range of Res. Here Res is the Reynolds number defined by Saffman (1978), which involves the curvature-induced strain rate. It is found to be the appropriate choice since then α1(β) varies weakly with core thickness β. The three most nonlinearly amplified modes are a mean azimuthal velocity in the form of opposing streams, an n = 1 mode (n is the azimuthal wavenumber) which arises from the interaction of two second-mode bending waves and the harmonic of the primary second mode. When a single wave is excited, higher harmonics begin to grow successively later with nonlinear growth rates proportional to n. The modified mean flow has a doubly peaked azimuthal vorticity. Since the curvature-induced strain is not exactly stagnation-point flow there is a preference for elongation towards the rear of the ring: the outer structure of the instability wave forms a long wake consisting of n hairpin vortices whose waviness is phase shifted π/n relative to the waviness in the core. Whereas the most amplified linear mode has three radial layers of structure, higher radial modes having more layers of radial structure (hairpins piled upon hairpins) are excited when the initial perturbation is large, reminiscent of visualization experiments on the formation of a turbulent ring at the generator.

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 279 , 25 November 1994 , pp. 351 - 375
Copyright
© 1994 Cambridge University Press

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