Near-inertial echoes of ageostrophic instability in submesoscale filaments

Ocean submesoscales, flows with characteristic size around 10m--10km, are transitional between the larger, rotationally-constrained mesoscale and three-dimensional turbulence. In this paper we present simulations of a submesoscale ocean filament. The strong vertical transport associated with submesoscale fronts and filaments ventilates the deeper water and provides a route for the observed forward cascade of energy in the ocean. In our case, the filament is strongly sheared in both vertical and cross-filament directions and is unstable. Instability indeed dominates the early behaviour with a fast extraction of kinetic energy from the vertically sheared thermal wind. The filament is expected to be subject to instabilities, including symmetric and Kelvin-Helmholtz instabilities. An instability emerges with a circulation that does not match either, though symmetric modes become apparent later. The action of the instability is sufficiently rapid that the filament does not respond in a geostrophically balanced sense. Instead, it later exhibits vertically sheared near-inertial oscillations with higher amplitude as the initial minimum Richardson number decreases. Horizontal gradients strengthen only briefly as the fronts restratify. These unstable filaments can be generated by strong mixing events at pre-existing stable structures. The oscillations must also be considered when designing initial conditions for numerical experiments of submesoscale flows, where the initial state is intended to be balanced.
Comment: Submitted to Journal of Fluid Mechanics. 11 pages, 6 figures, 1 table. Supplementary data consists of one movie "Movie 1" available at https://youtu.be/0FUPSQWpfe4