Journal
NATURE COMMUNICATIONS
Volume 8, Issue -, Pages -Publisher
NATURE PUBLISHING GROUP
DOI: 10.1038/ncomms14197
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Funding
- US National Science Foundation [OCE-1233832]
- NSERC PDF award
- NERC [NE/E006000/1, NE/E005667/1, NE/E006663/1, NE/E005985/1, NE/E007058/1] Funding Source: UKRI
- Natural Environment Research Council [NE/E006663/1, NE/E007058/1, NE/E006000/1, NE/E005985/1, NE/E005667/1] Funding Source: researchfish
- Division Of Ocean Sciences
- Directorate For Geosciences [1233832, 1232962] Funding Source: National Science Foundation
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It is an open question whether turbulent mixing across density surfaces is sufficiently large to play a dominant role in closing the deep branch of the ocean meridional overturning circulation. The diapycnal and isopycnal mixing experiment in the Southern Ocean found the turbulent diffusivity inferred from the vertical spreading of a tracer to be an order of magnitude larger than that inferred from the microstructure profiles at the mean tracer depth of 1,500m in the Drake Passage. Using a high-resolution ocean model, it is shown that the fast vertical spreading of tracer occurs when it comes in contact with mixing hotspots over rough topography. The sparsity of such hotspots is made up for by enhanced tracer residence time in their vicinity due to diffusion toward weak bottom flows. The increased tracer residence time may explain the large vertical fluxes of heat and salt required to close the abyssal circulation.
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