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dc.contributor.authorStewart, Andrew L.
dc.contributor.authorFerrari, Raffaele
dc.contributor.authorThompson, Andrew F.
dc.date.accessioned2014-11-04T13:29:53Z
dc.date.available2014-11-04T13:29:53Z
dc.date.issued2014-03
dc.date.submitted2013-11
dc.identifier.issn0022-3670
dc.identifier.issn1520-0485
dc.identifier.urihttp://hdl.handle.net/1721.1/91277
dc.description.abstractIn the major ocean basins, diapycnal mixing upwells dense Antarctic Bottom Water, which returns southward and closes the deepest cell of the meridional overturning circulation (MOC). This cell ventilates the deep ocean and regulates the partitioning of CO[subscript 2] between the atmosphere and the ocean. The oceanographic community's conceptual understanding of the deep stratification and MOC has evolved from classic “abyssal recipes” arguments to a more recent appreciation of along-isopycnal upwelling in the Southern Ocean, consistent with a weakly mixed ocean interior. Both the deep stratification and the deep MOC are shown here to be sensitive to the form of the surface buoyancy forcing in a two-dimensional model that includes a circumpolar channel and northern basin. For a fixed surface buoyancy condition, the deep stratification is essentially prescribed, whereas for a fixed surface buoyancy flux, the deep stratification varies by orders of magnitude over the range of diapycnal diffusivity κ observed in the ocean. These cases also produce different scalings for the deep MOC with κ, in both weak and strong κ regimes. In addition, these scalings are shown to be sensitive not only to the type of surface boundary condition, but also to the latitudinal structure of the surface fluxes. This latter point is crucial as buoyancy budgets and dynamical features of the circulation are poorly constrained along the Antarctic margins. This study emphasizes the need for caution in the interpretation of simple conceptual models that, while useful, may not include all mechanisms that contribute to the MOC’s strength and structure.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Award OCE-1232962)en_US
dc.language.isoen_US
dc.publisherAmerican Meteorological Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1175/jpo-d-13-0206.1en_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.titleOn the Importance of Surface Forcing in Conceptual Models of the Deep Oceanen_US
dc.typeArticleen_US
dc.identifier.citationStewart, Andrew L., Raffaele Ferrari, and Andrew F. Thompson. “On the Importance of Surface Forcing in Conceptual Models of the Deep Ocean.” J. Phys. Oceanogr. 44, no. 3 (March 2014): 891–899. © 2014 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.orderedauthorsStewart, Andrew L.; Ferrari, Raffaele; Thompson, Andrew F.en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3736-1956
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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