Abstract

We study direct numerical simulations of turbulence arising from the interaction of an initial background shear, a linear background stratification and an external body force. In each simulation the turbulence produced is spatially intermittent, with dissipation rates varying over orders of magnitude in the vertical. We focus analysis on the statistically quasi-steady states achieved by applying large-scale body forcing to the domain, and compare flows forced by internal gravity waves with those forced by vertically uniform vortical modes. By considering the turbulent energy budgets for each simulation, we find that the injection of potential energy from the wave forcing permits a reversal in the sign of the mean buoyancy flux. This change in the sign of the buoyancy flux is associated with large, convective density overturnings, which in turn lead to more efficient mixing in the wave-forced simulations. The inhomogeneous dissipation in each simulation allows us to investigate localised correlations between the kinetic and potential energy dissipation rates. These correlations lead us to the conclusion that an appropriate definition of an instantaneous mixing efficiency, (where and are the volume-averaged turbulent viscous dissipation rate and fluctuation density variance destruction rate respectively) in the wave-forced cases is independent of an appropriately defined local turbulent Froude number, consistent with scalings proposed for low Froude number stratified turbulence.

Highlights

  • Irreversible turbulent mixing has an important influence on many physical processes in the ocean

  • After the initial transient dynamics and a further adjustment period in each case that lasts until t ≈ 50, the turbulence characterised by EK and EP reaches a quasi-steady state

  • The turbulent potential energy EP is much larger in the wave-forced cases than in case H, and this coincides with a reduction in the turbulent kinetic energy (TKE) dissipation rate

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Summary

Introduction

Irreversible turbulent mixing has an important influence on many physical processes in the ocean. In the deep ocean this mixing is needed to close the meridional overturning circulation and it helps to set the abyssal stratification Ferrari 2014; Cessi 2019). Waterhouse et al (2014) highlight strong regional variability in mixing rates inferred from observations, both in abyssal regions and in the 898 A7-2. The spatial inhomogeneity of turbulent mixing in the ocean presents a key challenge in locally quantifying the vertical transport of important tracers such as heat, carbon and nutrients

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