Linear Stability of Large, Elliptical Warm-Core Rings

摘要

An analytical solution for a confined, elliptical lens of light is perturbed to test the linear stability of elongated warm-core rings. The asymptotic expression of the solution when the eddy's radius is 'large' (three times the deformation radius or more) is used to suppress inertial oscillations and render the problem easily tractable. It is found that, in this large-scale limit, the eddy's stability is independent of its size and dependent only on its eccentricity. The critical threshold is a ration of semi-major to semi-minor axes equal to 1.8. More circular eddies are stable to all infinitesimal perturbations while more elongated ones are unstable to at least a mode 3 (egg shape). In the present, reduced-gravity formalism, baroclinic instability is absent, and the instability mechanism is purely of frontal nature (presence of a curved outcrop). With an active stratum, baroclinic processes can probably set instability at even more moderate eccentricities. It is suggested that the instability of elongated lenses of water is the reason that precludes their existence even in areas known for their intense ring activity. Key words: Elliptical rings; Ocean models; Linear stability; Warm-core rings; Circular Eddies; Eddies (Fluid mechanics). (Reprints)