https://hal-polytechnique.archives-ouvertes.fr/hal-00996485Negretti, M. ElettaM. ElettaNegrettiLadHyX - Laboratoire d'hydrodynamique - X - École polytechnique - CNRS - Centre National de la Recherche ScientifiqueBillant, PaulPaulBillantLadHyX - Laboratoire d'hydrodynamique - X - École polytechnique - CNRS - Centre National de la Recherche ScientifiqueStability of a Gaussian pancake vortex in a stratified fluidHAL CCSD2013[PHYS.MECA.MEFL] Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph][SPI.MECA.MEFL] Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph]Roura, Denis2014-06-02 21:34:462020-11-23 10:28:022014-06-03 11:46:01enJournal articleshttps://hal-polytechnique.archives-ouvertes.fr/hal-00996485/document10.1017/jfm.2012.624application/pdf1Vortices in stably stratified fluids generally have a pancake shape with a small vertical thickness compared with their horizontal size. In order to understand what mechanism determines their minimum thickness, the linear stability of an axisymmetric pancake vortex is investigated as a function of its aspect ratio alpha, the horizontal Froude number F-h, the Reynolds number Re and the Schmidt number Sc. The vertical vorticity profile of the base state is chosen to be Gaussian in both radial and vertical directions. The vortex is unstable when the aspect ratio is below a critical value, which scales with the Froude number: alpha(c) similar to 1.1F(h) for sufficiently large Reynolds numbers. The most unstable perturbation has an azimuthal wavenumber either m = 0, vertical bar m vertical bar = 1 or vertical bar m vertical bar = 2 depending on the control parameters. We show that the threshold corresponds to the appearance of gravitationally unstable regions in the vortex core due to the thermal wind balance. The Richardson criterion for shear instability based on the vertical shear is never satisfied alone. The dominance of the gravitational instability over the shear instability is shown to hold for a general class of pancake vortices with angular velocity of the form (Omega) over tilde (r, z) = Omega(r)f(z) provided that r partial derivative Omega/partial derivative r < 3 Omega everywhere. Finally, the growth rate and azimuthal wavenumber selection of the gravitational instability are accounted well by considering an unstably stratified viscous and diffusive layer in solid body rotation with a parabolic density gradient.