Abstract

Abstract The linear stability of steady frontal zones is considered using the primitive equations. The frontal zones chosen have uniform potential vorticity and form a sequence of “snapshots” of the deformation-induced front as it evolves toward frontal collapse. The stability for a given alongfront wavelength is determined by integrating a numerical model forward from an initial condition of the basic-state front plus white noise. Two classes of instabilities emerge. In one class, the modes are modified versions of familiar, synoptic-scale baroclinic waves. The other class consists of Kelvin–Helmholtz (KH) instabilities. These modes have wavelengths of order 1 km and exist only when the cross-frontal scale is of order 10 km or smaller. With e-folding times of a few minutes, the growth of KH waves may limit the cross-frontal scale of active, time-dependent frontal flows, although boundary layer processes are probably important, at least for surface fronts, before KH modes appear. No other instabilities ar...

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