Turning Ocean Mixing Upside Down

It is generally understood that small-scale mixing, such as is caused by breaking internal waves, drives upwelling of the densest ocean waters that sink to the ocean bottom at high latitudes. However, the observational evidence that the strong turbulent fluxes generated by small-scale mixing in the...

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Bibliographic Details
Main Authors: McDougall, Trevor J. (Author), Nikurashin, Maxim (Author), Ferrari, Raffaele (Contributor), Mashayekhi, Alireza (Contributor), Campin, Jean-Michel (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: American Meteorological Society, 2017-02-10T18:51:03Z.
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Online Access:Get fulltext
LEADER 02194 am a22002653u 4500
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042 |a dc 
100 1 0 |a McDougall, Trevor J.  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences  |e contributor 
100 1 0 |a Ferrari, Raffaele  |e contributor 
100 1 0 |a Mashayekhi, Alireza  |e contributor 
100 1 0 |a Campin, Jean-Michel  |e contributor 
700 1 0 |a Nikurashin, Maxim  |e author 
700 1 0 |a Ferrari, Raffaele  |e author 
700 1 0 |a Mashayekhi, Alireza  |e author 
700 1 0 |a Campin, Jean-Michel  |e author 
245 0 0 |a Turning Ocean Mixing Upside Down 
260 |b American Meteorological Society,   |c 2017-02-10T18:51:03Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/106899 
520 |a It is generally understood that small-scale mixing, such as is caused by breaking internal waves, drives upwelling of the densest ocean waters that sink to the ocean bottom at high latitudes. However, the observational evidence that the strong turbulent fluxes generated by small-scale mixing in the stratified ocean interior are more vigorous close to the ocean bottom boundary than above implies that small-scale mixing converts light waters into denser ones, thus driving a net sinking of abyssal waters. Using a combination of theoretical ideas and numerical models, it is argued that abyssal waters upwell along weakly stratified boundary layers, where small-scale mixing of density decreases to zero to satisfy the no density flux condition at the ocean bottom. The abyssal ocean meridional overturning circulation is the small residual of a large net sinking of waters, driven by small-scale mixing in the stratified interior above the bottom boundary layers, and a slightly larger net upwelling, driven by the decay of small-scale mixing in the boundary layers. The crucial importance of upwelling along boundary layers in closing the abyssal overturning circulation is the main finding of this work. 
520 |a National Science Foundation (U.S.) (Award OCE-1233832) 
520 |a Australian Research Council (Grant DE150100937) 
546 |a en_US 
655 7 |a Article 
773 |t Journal of Physical Oceanography