Journal of Fluid Mechanics



Papers

The quasi-geostrophic ellipsoidal vortex model


DAVID G. DRITSCHEL a1, JEAN N. REINAUD a1 and WILLIAM J. McKIVER a1
a1 School of Mathematics and Statistics, University of St Andrews, St Andrews, UK

Article author query
dritschel d   [Google Scholar] 
reinaud j   [Google Scholar] 
mckiver w   [Google Scholar] 
 

Abstract

We present a simple approximate model for studying general aspects of vortex interactions in a rotating stably-stratified fluid. The model idealizes vortices by ellipsoidal volumes of uniform potential vorticity, a materially conserved quantity in an inviscid, adiabatic fluid. Each vortex thus possesses 9 degrees of freedom, 3 for the centroid and 6 for the shape and orientation. Here, we develop equations for the time evolution of these quantities for a general system of interacting vortices. An isolated ellipsoidal vortex is well known to remain ellipsoidal in a fluid with constant background rotation and uniform stratification, as considered here. However, the interaction between any two ellipsoids in general induces weak non-ellipsoidal perturbations. We develop a unique projection method, which follows directly from the Hamiltonian structure of the system, that effectively retains just the part of the interaction which preserves ellipsoidal shapes. This method does not use a moment expansion, e.g. local expansions of the flow in a Taylor series. It is in fact more general, and consequently more accurate. Comparisons of the new model with the full equations of motion prove remarkably close.

(Received February 18 2003)
(Revised July 17 2003)



Metrics