Weakly nonlinear saturation of short-wave instabilities in a strained Lamb-Oseen vortex

Authors
Citation
D. Sipp, Weakly nonlinear saturation of short-wave instabilities in a strained Lamb-Oseen vortex, PHYS FLUIDS, 12(7), 2000, pp. 1715-1729
Citations number
26
Categorie Soggetti
Physics
Journal title
PHYSICS OF FLUIDS
ISSN journal
10706631 → ACNP
Volume
12
Issue
7
Year of publication
2000
Pages
1715 - 1729
Database
ISI
SICI code
1070-6631(200007)12:7<1715:WNSOSI>2.0.ZU;2-0
Abstract
A Lamb-Oseen vortex in a planar straining field is known to be subject to 3 D (three-dimensional) short-wave instabilities which are due to the resonan ce of the straining field and two stationary Kelvin waves characterized by the same axial wave number and by azimuthal wave numbers equal to -1 and +1 . The linear regime has been described by Moore and Saffman (1975). In this article, we extend this analysis to the weakly nonlinear regime. The emerg ing eigenmode is characterized by a complex amplitude A=\A\e(i phi), whose behavior is governed by an amplitude equation. It is shown that the unstabl e perturbation corresponds to an oscillation of the vortex in a plane incli ned at an angle phi, while the amplitude of these oscillations is proportio nal to \A\. The vortex centers are defined as the points where the velocity of the vortex is zero, which also corresponds to the points where the pres sure is minimum. We show that these instabilities saturate. The saturation amplitudes are evaluated numerically and expressed in terms of oscillation amplitudes of the vortex centers. If a denotes the internal radius of the v ortex and if the straining field is due to a counter-rotating vortex of sam e strength, located at a distance b, then the maximum amplitude Delta of th e vortex oscillations is Delta/b=6.1a(2)/b(2). This result is in agreement with those of the experiments of Leweke and Williamson (1998) for which a/b =0.2. It also shows that in aeronautical situations, for which a/b is small er, i.e., a/b < 0.1, the considered short-wave instability will saturate at very low amplitude. (C) 2000 American Institute of Physics. [S1070-6631(00 )02607-6].