Dg. Dritschel et Mdt. Juarez, THE INSTABILITY AND BREAKDOWN OF TALL COLUMNAR VORTICES IN A QUASI-GEOSTROPHIC FLUID, Journal of Fluid Mechanics, 328, 1996, pp. 129-160
We examine the linear stability of elliptical columns of uniform poten
tial vorticity subject to two-dimensional (horizontal) straining withi
n a rapidly rotating, stratified (quasi-geostrophic) fluid. We find th
at horizontal straining can promote the exponential growth of three-di
mensional disturbances when the vortex height-to-width aspect ratio ex
ceeds, qualitatively, three times the ratio of the Coriolis parameter
to the buoyancy frequency. This instability is not related to the usua
l baroclinic instability which operates on shallow vortex columns whos
e potential vorticity changes sign with height. The nonlinear developm
ent of these instabilities is investigated numerically using a high-re
solution contour surgery algorithm. Simulations are conducted for both
a Boussinesq (ocean-like) fluid and a compressible (atmospheric-like)
fluid having exponentially decreasing density with height. The simula
tions reveal a generic nonlinear development that results in a semi-el
lipsoidal baroclinic vortex dome at the lower surface and, in the case
of a Boussinesq fluid, another such dome at the upper surface. The re
lated problem of two interacting vortex columns is also examined. A ge
neric three-dimensional instability and nonlinear development occurs n
o matter how great the distance between the vortex columns, provided t
hat they are sufficiently tall. Our results may bear upon the observed
structure of many atmospheric and oceanic vortices, whose height-to-w
idth aspect ratios are consistent with our findings. Remarkably, even
strongly ageostrophic vortices, such as tropical cyclones, fit the pat
tern. Our results furthermore re-open questions about the long-time na
ture of freely decaying quasi-geostrophic turbulence, for which recent
simulations indicate a progressive two-dimensionalization by vortex a
lignment, while earlier simulations have indicated long-lived baroclin
ic vortices, not unlike what we find here.