Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8232
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dc.contributor.authorallGrezio, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.contributor.authorallWells, N. C.; Southampton Oceanography Centre, UKen
dc.contributor.authorallIvchenko, V. O.; Southampton Oceanography Centre, UKen
dc.contributor.authorallDe Cuevas, B. A.; Southampton Oceanography Centre, UKen
dc.date.accessioned2012-10-16T13:51:44Zen
dc.date.available2012-10-16T13:51:44Zen
dc.date.issued2005en
dc.identifier.urihttp://hdl.handle.net/2122/8232en
dc.description.abstractThree general-circulation models (FRAM, OCCAM and POP) are used to investigate the dynamics of the Antarctic Circumpolar Current (ACC) at the latitudes of the Drake Passage where the ACC is unbounded. In these general circulation models, bottom form stress balances the wind stress in the momentum budgets. In the vorticity budgets, the main balance is between wind curl and bottom pressure torque in FRAM, OCCAM and POP. Moreover, in the ACC belt all topographic features are regions of nonlinearity and bottom pressure torque variations, with the Drake Passage playing the largest role. Transient eddy Reynolds stresses (TERSs) play a different role in the three models. In the upper levels, TERSs accelerate the flow in the POP and FRAM models, but decelerate the flow in OCCAM. The behaviour of TERSs change throughout the whole water column in the ACC belt and Reynolds stresses have a dragging effect on the flow below the levels where the topography starts to obstruct the flow. The total volume transport in three models is very different. Additionally, the different spatial resolution, which results in a different level of eddy kinetic energy, has a significant influence on the transport.en
dc.language.isoEnglishen
dc.relation.ispartofQ. J. R. Meteorol. Soc.en
dc.relation.ispartofseries/131 (2005)en
dc.subjectEddies - Dynamical Budgetsen
dc.titleDynamical budgets of the Antarctic Circumpolar Current using ocean general-circulation modelsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber833-860en
dc.subject.INGV03. Hydrosphere::03.03. Physical::03.03.02. General circulationen
dc.identifier.doi10.1256/qj.03.213en
dc.description.obiettivoSpecifico3.7. Dinamica del clima e dell'oceanoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.contributor.authorGrezio, A.en
dc.contributor.authorWells, N. C.en
dc.contributor.authorIvchenko, V. O.en
dc.contributor.authorDe Cuevas, B. A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.contributor.departmentSouthampton Oceanography Centre, UKen
dc.contributor.departmentSouthampton Oceanography Centre, UKen
dc.contributor.departmentSouthampton Oceanography Centre, UKen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.deptSouthampton Oceanography Centre, UK-
crisitem.author.deptSouthampton Oceanography Centre, UK-
crisitem.author.deptSouthampton Oceanography Centre, UK-
crisitem.author.orcid0000-0001-6848-7589-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent03. Hydrosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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