Reconciling the Observed Mid-Depth Exponential Ocean Stratification with Weak Interior Mixing and Southern Ocean Dynamics via Boundary-Intensified Mixing
Madeline D. Miller, Xiaoting Yang, Eli Tziperman

TL;DR
This paper demonstrates that boundary-intensified mixing, rather than interior mixing alone, explains the observed exponential deep ocean temperature profile, reconciling weak interior diffusivity with Southern Ocean dynamics.
Contribution
It introduces a boundary-focused mixing model that accounts for the exponential stratification, challenging the notion that interior mixing solely determines deep ocean profiles.
Findings
Boundary mixing leads to exponential temperature profiles.
Southern Ocean eddies link surface fluxes to deep stratification.
Interior mixing is insufficient alone to explain observed profiles.
Abstract
Munk (1966) showed that the deep (1000-3000 m) vertical temperature profile is consistent with a one-dimensional vertical advection-diffusion balance, with a constant upwelling and an interior diapycnal diffusivity of m s. However, typical observed diffusivities in the interior are m s. Recent work suggested that the deep stratification is set by Southern Ocean (SO) isopycnal slopes, fixed by SO eddies, that communicate the surface outcrop positions to the deep ocean. It is shown here, using an idealized ocean general circulation model, that SO eddies alone cannot lead to the observed exponential temperature profile, and that interior mixing must contribute. Strong diapycnal mixing concentrated near the ocean boundaries is shown to be balanced locally by upwelling. A one-dimensional Munk-like balance in these…
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