Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/42077
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dc.contributor.authorHernández-Guerra, Alonsoen_US
dc.contributor.authorTalley, Lynne D.en_US
dc.contributor.otherHernandez-Guerra, Alonso-
dc.date.accessioned2018-10-04T16:43:56Z-
dc.date.available2018-10-04T16:43:56Z-
dc.date.issued2016en_US
dc.identifier.issn0079-6611en_US
dc.identifier.urihttp://hdl.handle.net/10553/42077-
dc.description.abstractThe meridional circulation and transports at 30°S in the Pacific and Indian Oceans for the years 2002–2003 and 2009 are compared, using GO-SHIP hydrographic section data with an inverse box model and several choices of constraints. Southward heat transport across the combined Indian-Pacific sections, reflecting net heating north of these sections, doubled from −0.7 ± 0.2 PW in 2002–2003 to −1.4 ± 0.1 PW in 2009 (negative sign is southward), with the increase concentrated in the Indian Ocean (∼0.6 PW compared with ∼0.2 PW in the Pacific), and was insensitive to model choices for the Indonesian Throughflow. Diagnosed net evaporation also more than doubled in the Indian Ocean, from 0.21–0.27 Sv in 2002–2003 to 0.51–0.58 in 2009, with a smaller but significant increase in net evaporation in the Pacific, from 0.06–0.08 Sv to 0.16–0.32 Sv. These increased heat and freshwater exports coincided with Indian Ocean warming, a shift in the Indian's shallow gyre overturning transport to lower densities, and an increase in southward Agulhas Current transport from 75 Sv in 2002 to 92 Sv in 2009. The Indian's deep overturn weakened from about 11 Sv in 2002 to 7 Sv in 2009. In contrast, the Pacific Ocean overturning circulation was nearly unchanged from 2003 to 2009, independent of model within the uncertainties. The East Australian Current transport decreased only slightly, from −52 Sv to −46 Sv. The southward Pacific Deep Water transport was at a higher density than the southward Indian Deep Water transport in both years and all models, similar to prior results. Estimated diapycnal diffusivity and velocity are strongly enhanced near the ocean bottom and are higher farther up in the water column in the Indian than in the Pacific, likely extending the reach of Indian Ocean overturning up to shallower depths than in the Pacific. The horizontal distribution of transports in the Pacific at all depths changed notably from 2003 to 2009, despite the stability of its meridional overturning structure. The 2009 horizontal structure resembles a “bowed gyre”; the hydrographic section data show that this disturbance extends to the abyss and disrupts the Deep Western Boundary Current structure in the Southwest Pacific Basin. Satellite altimetry suggests association with slow westward Rossby wave propagation generated in the eastern Pacific, with no apparent effect on the net overturning circulation. The Indian Ocean's upper ocean horizontal structure was stable between the two years even though its shallow gyre overturning transports changed significantly. On the other hand, northward abyssal transports concentrated in the central Indian Ocean (Crozet Basin) in 2002 shifted westward to the Mozambique and Madagascar Basins in 2009, although the Crozet Basin's Deep Western Boundary Current existed in both years.en_US
dc.languageengen_US
dc.relationVariabilidad Estacional de la Amoc: la Corriente de Canariasen_US
dc.relation.ispartofProgress in Oceanographyen_US
dc.sourceProgress in Oceanography [ISSN 0079-6611], v. 146, p. 89-120en_US
dc.subject2510 Oceanografíaen_US
dc.subject.otherTotal Geostrophic Circulation
dc.subject.otherLarge-Scale Circulation
dc.subject.otherFresh-Water Transports
dc.subject.otherAgulhas Current
dc.subject.otherLeeuwin Current
dc.subject.otherHydrographic Section
dc.subject.otherSouthern-Ocean
dc.subject.otherGlobal Heat
dc.subject.otherInterannual Variability
dc.subject.otherIndonesian Throughflow
dc.titleMeridional overturning transports at 30°S in the Indian and Pacific Oceans in 2002–2003 and 2009en_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.pocean.2016.06.005
dc.identifier.scopus84978961938-
dc.identifier.isi000382341800006-
dcterms.isPartOfProgress In Oceanography-
dcterms.sourceProgress In Oceanography[ISSN 0079-6611],v. 146, p. 89-120-
dc.contributor.authorscopusid56455072400-
dc.contributor.authorscopusid6701736545
dc.contributor.authorscopusid7004902765-
dc.description.lastpage120-
dc.description.firstpage89-
dc.relation.volume146-
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.identifier.wosWOS:000382341800006-
dc.contributor.daisngid660191-
dc.contributor.daisngid210519-
dc.identifier.investigatorRIDA-4747-2008-
dc.contributor.wosstandardWOS:Hernandez-Guerra, A
dc.contributor.wosstandardWOS:Talley, LD
dc.date.coverdateAgosto 2016
dc.identifier.ulpgces
dc.description.sjr1,922
dc.description.jcr3,391
dc.description.sjrqQ1
dc.description.jcrqQ1
dc.description.scieSCIE
item.grantfulltextnone-
item.fulltextSin texto completo-
crisitem.author.deptGIR IOCAG: Oceanografía Física-
crisitem.author.deptIU de Oceanografía y Cambio Global-
crisitem.author.deptDepartamento de Física-
crisitem.author.orcid0000-0002-4883-8123-
crisitem.author.parentorgIU de Oceanografía y Cambio Global-
crisitem.author.fullNameHernández Guerra, Alonso-
crisitem.project.principalinvestigatorHernández Guerra, Alonso-
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