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Multipolar vortices in two-dimensional incompressible flows

Published online by Cambridge University Press:  26 April 2006

Yves G. Morel  and
Xavier J. Carton
Yves G. Morel
Affiliation:
SHOM, LEGI/IMG, BP53X, 38041 Grenoble Cedex, France
Xavier J. Carton
Affiliation:
SHOM, GRGS, Centre National d’Etudes Spatiales, 18 Ave. Edouard Belin, 31055 Toulouse Cedex, France
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Abstract

In a two-dimensional incompressible fluid, the barotropic instability of isolated circular vortices can lead to multipole formation. The multipoles we study here are composed of a core vortex surrounded by two or more identical satellite vortices, of opposite-sign vorticity to the core, and the total circulation is zero. First, we present the generation of multipoles from unstable piecewise-constant monopoles perturbed on a monochromatic azimuthal mode. The stationary multipoles formed by this nonlinear evolution retain the same energy, circulation and angular momentum as the original monopoles, but possess a lower enstrophy. These multipolar steady states are then compared to multipolar equilibria of the Euler equation, obtained either analytically by a perturbation expansion or numerically via a relaxation algorithm. Finally the stability of these equilibria is studied. Quadrupoles (one core vortex bound to three satellites) prove relatively robust, whether initially perturbed or not, and resist severe permanent deformations (mode-2 shears or strains of amplitude up to 0.1ζ(max). Amplification of the mode-3 deformation proves more destructive. More complex multipoles degenerate in less than a turnover period into end-products of a lesser complexity, via vortex splitting, pairing or merging. We use the conservation of integral properties to classify the large variety of instability mechanisms along physical guidelines. To conclude, we synthetize the connections between these various vortex forms.

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 267 , 25 May 1994 , pp. 23 - 51
Copyright
© 1994 Cambridge University Press

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