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dc.contributor.authorMazloff, Matthew R.
dc.contributor.authorFerrari, Raffaele
dc.contributor.authorSchneider, Tapio
dc.date.accessioned2014-02-24T17:03:05Z
dc.date.available2014-02-24T17:03:05Z
dc.date.issued2013-06
dc.date.submitted2013-02
dc.identifier.issn0022-3670
dc.identifier.issn1520-0485
dc.identifier.urihttp://hdl.handle.net/1721.1/85074
dc.description.abstractThe Southern Ocean (SO) limb of the meridional overturning circulation (MOC) is characterized by three vertically stacked cells, each with a transport of about 10 Sv (Sv ≡ 10[superscript 6] m[superscript 3] s[superscript −1]). The buoyancy transport in the SO is dominated by the upper and middle MOC cells, with the middle cell accounting for most of the buoyancy transport across the Antarctic Circumpolar Current. A Southern Ocean state estimate for the years 2005 and 2006 with 1/6° resolution is used to determine the forces balancing this MOC. Diagnosing the zonal momentum budget in density space allows an exact determination of the adiabatic and diapycnal components balancing the thickness-weighted (residual) meridional transport. It is found that, to lowest order, the transport consists of an eddy component, a directly wind-driven component, and a component in balance with mean pressure gradients. Nonvanishing time-mean pressure gradients arise because isopycnal layers intersect topography or the surface in a circumpolar integral, leading to a largely geostrophic MOC even in the latitude band of Drake Passage. It is the geostrophic water mass transport in the surface layer where isopycnals outcrop that accomplishes the poleward buoyancy transport.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant OCE-1233832)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant OCE-1234473)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant OPP-0961218)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant MCA06N007)en_US
dc.language.isoen_US
dc.publisherAmerican Meteorological Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1175/jpo-d-12-069.1en_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.sourceAmerican Meteorological Societyen_US
dc.titleThe Force Balance of the Southern Ocean Meridional Overturning Circulationen_US
dc.typeArticleen_US
dc.identifier.citationMazloff, Matthew R., Raffaele Ferrari, and Tapio Schneider. “The Force Balance of the Southern Ocean Meridional Overturning Circulation.” J. Phys. Oceanogr. 43, no. 6 (June 2013): 1193–1208. © 2013 American Meteorological Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorFerrari, Raffaeleen_US
dc.relation.journalJournal of Physical Oceanographyen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsMazloff, Matthew R.; Ferrari, Raffaele; Schneider, Tapioen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3736-1956
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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