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dc.contributor.authorKlocker, Andreas
dc.contributor.authorMunday, David
dc.contributor.authorGayen, Bishakhdatta
dc.contributor.authorRoquet, Fabien
dc.contributor.authorLacasce, Joseph Henry
dc.date.accessioned2024-02-15T12:01:56Z
dc.date.available2024-02-15T12:01:56Z
dc.date.created2024-01-02T15:09:53Z
dc.date.issued2023
dc.identifier.citationTellus A: Dynamic Meteorology and Oceanography. 2023, 75 (1), 392-409.en_US
dc.identifier.issn0280-6495
dc.identifier.urihttps://hdl.handle.net/11250/3117971
dc.description.abstractIn contrast with the atmosphere, which is heated from below by solar radiation, the ocean is both heated and cooled from above. To drive a deep-reaching overturning circulation in this context, it is generally assumed that either intense interior mixing by winds and internal tides, or wind-driven upwelling is required; in their absence, the circulation is thought to collapse to a shallow surface cell. We demonstrate, using a primitive equation model with an idealized domain and no wind forcing, that the surface temperature forcing can in fact drive an interhemispheric overturning provided that there is an open channel unblocked in the zonal direction, such as in the Southern Ocean. With this geometry, rotating horizontal convection, in combination with asymmetric surface cooling between the north and south, drives a deep-reaching two-cell overturning circulation. The resulting vertical mid-depth stratification closely resembles that of the real ocean, suggesting that wind-driven pumping is not necessary to produce a deep-reaching overturning circulation, and that buoyancy forcing plays a more important role than is usually assumed.en_US
dc.language.isoengen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectHorisontell konveksjonen_US
dc.subjectHorizontal convectionen_US
dc.titleDeep-Reaching Global Ocean Overturning Circulation Generated by Surface Buoyancy Forcingen_US
dc.title.alternativeDeep-Reaching Global Ocean Overturning Circulation Generated by Surface Buoyancy Forcingen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.rights.holder© 2023 The Author(s)en_US
dc.description.versionpublishedVersionen_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.doi10.16993/tellusa.3231
dc.identifier.cristin2219172
dc.source.journalTellus A: Dynamic Meteorology and Oceanographyen_US
dc.source.volume75en_US
dc.source.issue1en_US
dc.source.pagenumber392-409en_US
dc.relation.projectNorges forskningsråd: 302743en_US
dc.relation.projectAndre: Australian Research Council Future Fellowship FT180100037en_US
dc.subject.nsiVDP::Meteorologi: 453en_US
dc.subject.nsiVDP::Meteorology: 453en_US


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