Nonlinear Evolution of a Baroclinic Wave and Imbalanced Dissipation

TL;DR

This paper investigates how unstable baroclinic waves in rotating stratified flows evolve nonlinearly, leading to interior turbulence and energy dissipation through secondary instabilities, with implications for oceanic and atmospheric dynamics.

Contribution

It demonstrates a local pathway to energy dissipation via interior turbulent cascades and analyzes the scaling of dissipation with Rossby number in a specific flow regime.

Findings

Dissipation rate peaks as frontogenesis slows down.

Energy spectrum shows a transition from $k^{-3}$ to $k^{-5/3}$ scaling.

Dissipation scales exponentially with Rossby number.

Abstract

We consider the nonlinear evolution of an unstable baroclinic wave in a regime of rotating stratified flow that is of relevance to interior circulation in the oceans and in the atmosphere---a regime characterized by small large-scale Rossby and Froude numbers, a small vertical to horizontal aspect ratio, and no bounding horizontal surfaces. Using high-resolution simulations of the non-hydrostatic Boussinesq equations and companion integrations of the balanced quasi-geostrophic equations, we present evidence for a local route to dissipation of balanced energy directly through interior turbulent cascades. Analysis of simulations presented in this study suggest that a developing baroclinic instability can lead to secondary instabilities that can cascade a small fraction of the energy forward to unbalanced scales. Mesoscale shear and strain resulting from the hydrostatic geostrophic baroclinic instability drive frontogenesis. The fronts in turn support ageostrophic secondary circulation and instabilities. These two processes acting together lead to a quick rise in dissipation rate which then reaches a peak and begins to fall slowly when frontogenesis slows down; eventually balanced and imbalanced modes decouple. Dissipation of balanced energy by imbalanced processes scales exponentially with Rossby number of the base flow. We expect that this scaling will hold more generally than for the specific setup we consider given the fundamental nature of the dynamics involved. A break is seen in the total energy spectrum at small scales: While a steep $k^{-3}$ geostrophic scaling (where $k$ is the three-dimensional wavenumber) is seen at intermediate scales, the smaller scales display a shallower $k^{-5/3}$ scaling, reminiscent of the atmospheric spectra of Nastrom & Gage. At higher Ro, the vertical shear spectrum has a minimum, like in some relevant obervations