Abstract

Internal tides power much of the observed small-scale turbulence in the ocean interior. To represent mixing induced by this turbulence in ocean climate models, the cascade of internal tide energy to dissipation scales must be understood and mapped. Here, we present a framework for estimating the geography of internal tide energy sinks. The mapping relies on the following ingredients: (i) a global observational climatology of stratification; (ii) maps of the generation of M2, S2 and K1 internal tides decomposed into vertical normal modes; (iii) simplified representations of the dissipation of low-mode internal tides due to wave-wave interactions, scattering by small-scale topography, interaction with critical slopes and shoaling; (iv) Lagrangian tracking of low-mode energy beams through observed stratification, including refraction and reflection. We thus obtain a global map of the column-integrated energy dissipation for each of the four considered dissipative processes, each of the three tidal constituents and each of the first five modes. Modes ≥6 are inferred to dissipate within the local water column at the employed half-degree horizontal resolution. Combining all processes, modes and constituents, we construct a map of the total internal tide energy dissipation, which compares well with observational inferences of internal wave energy dissipation. This result suggests that tides largely shape observed spatial contrasts of dissipation, and that the framework has potential in improving understanding and modelling of ocean mixing. However, sensitivity to poorly constrained parameters and simplifying assumptions entering the parameterized energy sinks calls for additional investigation. The attenuation of low-mode internal tides by wave-wave interactions needs particular attention.

Highlights

  • Ocean general circulation models (OGCMs) do not resolve the cascade of energy down to dissipation scales

  • For an ocean model to appropriately respond to changes in external forcing, irreversible mixing must be connected to the forcing via conservative and realistic tracking of energy (Eden et al, 2014)

  • We begin by illustrating the energy redistribution accomplished by the first-mode M2 internal tide

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Summary

Introduction

Ocean general circulation models (OGCMs) do not resolve the cascade of energy down to dissipation scales. They rely on parameterizations of the irreversible mixing accomplished by small-scale turbulence. This parameterized mixing is pivotal to model behaviour on climatic timescales because it is the principal source of density transformation away from boundaries (Iudicone et al, 2008). Ad hoc representations of irreversible mixing, such as the specification of diffusivities that are fixed in time, remain common in ocean modelling. For an ocean model to appropriately respond to changes in external forcing, irreversible mixing must be connected to the forcing via conservative and realistic tracking of energy (Eden et al, 2014)

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