Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published September 2018 | Published
Journal Article Open

Restratification of Abyssal Mixing Layers by Submesoscale Baroclinic Eddies


For small-scale turbulence to achieve water mass transformation and thus affect the large-scale overturning circulation, it must occur in stratified water. Observations show that abyssal turbulence is strongly enhanced in the bottom few hundred meters in regions with rough topography, and it is thought that these abyssal mixing layers are crucial for closing and shaping the overturning circulation. If it were left unopposed, however, bottom-intensified turbulence would mix away the observed mixing-layer stratification over the course of a few years. It is proposed here that the homogenizing tendency of mixing may be balanced by baroclinic restratification. It is shown that bottom-intensified mixing, if it occurs on a large-scale topographic slope such as a midocean ridge flank, not only erodes stratification but also tilts isopycnals in the bottom few hundred meters. This tilting of isopycnals generates a reservoir of potential energy that can be tapped into by submesoscale baroclinic eddies. The eddies slide dense water under light water and thus restratify the mixing layer, similar to what happens in the surface mixed layer. This restratification is shown to be effective enough to balance the homogenizing tendency of mixing and to maintain the observed mixing-layer stratification. This suggests that submesoscale baroclinic eddies may play a crucial role in providing the stratification mixing can act on, thus allowing sustained water mass transformation. Through their restratification of abyssal mixing layers, submesoscale eddies may therefore directly affect the strength and structure of the abyssal overturning circulation.

Additional Information

© 2018 American Meteorological Society. Received: 20 April 2018; Final Form: 12 July 2018; Published online: 5 September 2018. I would like to thank the developers of Dedalus (dedalus-project.org), which was used for all computations presented in this paper. In particular, I would like to thank Keaton Burns, who also assisted with the setup and optimization of the computations. Chris Garrett and Carl Wunsch gave valuable feedback on the manuscript, and anonymous reviewers provided useful suggestions.

Attached Files

Published - jpo-d-18-0082.1.pdf


Files (1.4 MB)
Name Size Download all
1.4 MB Preview Download

Additional details

August 24, 2023
October 18, 2023