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dc.contributor.authorSalehipour, H.
dc.contributor.authorBouffard, D.
dc.contributor.authorCaulfield, C. P.
dc.contributor.authorNikurashin, M.
dc.contributor.authorPeltier, W. R.
dc.contributor.authorSmyth, W. D.
dc.contributor.authorMashayekhi, Alireza
dc.contributor.authorFerrari, Raffaele
dc.date.accessioned2018-10-01T14:02:42Z
dc.date.available2018-10-01T14:02:42Z
dc.date.issued2017-06
dc.date.submitted2016-12
dc.identifier.issn0094-8276
dc.identifier.urihttp://hdl.handle.net/1721.1/118296
dc.description.abstractTurbulent mixing produced by breaking of internal waves plays an important role in setting the patterns of downwelling and upwelling of deep dense waters and thereby helps sustain the global deep ocean overturning circulation. A key parameter used to characterize turbulent mixing is its efficiency, defined here as the fraction of the energy available to turbulence that is invested in mixing. Efficiency is conventionally approximated by a constant value near one sixth. Here we show that efficiency varies significantly in the abyssal ocean and can be as large as approximately one third in density stratified regions near topographic features. Our results indicate that variations in efficiency exert a first-order control over the rate of overturning of the lower branch of the meridional overturning circulation.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant OCE-1233832)en_US
dc.publisherAmerican Geophysical Union (AGU)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1002/2016GL072452en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceOther repositoryen_US
dc.titleEfficiency of turbulent mixing in the abyssal ocean circulationen_US
dc.typeArticleen_US
dc.identifier.citationMashayek, A. et al. “Efficiency of Turbulent Mixing in the Abyssal Ocean Circulation.” Geophysical Research Letters 44, 12 (June 2017): 6296–6306 © 2017 American Geophysical Unionen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorMashayekhi, Alireza
dc.contributor.mitauthorFerrari, Raffaele
dc.relation.journalGeophysical Research Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-09-21T18:53:00Z
dspace.orderedauthorsMashayek, A.; Salehipour, H.; Bouffard, D.; Caulfield, C. P.; Ferrari, R.; Nikurashin, M.; Peltier, W. R.; Smyth, W. D.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-1279-7593
dc.identifier.orcidhttps://orcid.org/0000-0002-3736-1956
mit.licensePUBLISHER_POLICYen_US


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