Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/2407
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dc.contributor.authorallFuniciello, F.; Dipartimento di Scienze Geologiche, Universita` Roma Treen
dc.contributor.authorallMoroni, M.; Dipartimento di Idraulica, Trasporti e Strade, Universita` degli Studi di Roma ‘‘La Sapienza,’’ Rome, Italy.en
dc.contributor.authorallPiromallo, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallFaccenna, C.; Dipartimento di Scienze Geologiche, Universita` Roma Treen
dc.contributor.authorallCenedese, A.; Dipartimento di Idraulica, Trasporti e Strade, Universita` degli Studi di Roma ‘‘La Sapienza,’’ Rome, Italy.en
dc.contributor.authorallBui, H. A.; Dipartimento di Scienze Geologiche, Universita` Roma Treen
dc.date.accessioned2007-08-31T09:32:53Zen
dc.date.available2007-08-31T09:32:53Zen
dc.date.issued2006en
dc.identifier.urihttp://hdl.handle.net/2122/2407en
dc.description.abstractThree-dimensional dynamically consistent laboratory models are carried out to model the large-scale mantle circulation induced by subduction of a laterally migrating slab. A laboratory analogue of a slab–upper mantle system is set up with two linearly viscous layers of silicone putty and glucose syrup in a tank. The circulation pattern is continuously monitored and quantitatively estimated using a feature tracking image analysis technique. The effects of plate width and mantle viscosity/density on mantle circulation are systematically considered. The experiments show that rollback subduction generates a complex three-dimensional time-dependent mantle circulation pattern characterized by the presence of two distinct components: the poloidal and the toroidal circulation. The poloidal component is the answer to the viscous coupling between the slab motion and the mantle, while the toroidal one is produced by lateral slab migration. Spatial and temporal features of mantle circulation are carefully analyzed. These models show that (1) poloidal and toroidal mantle circulation are both active since the beginning of the subduction process, (2) mantle circulation is intermittent, (3) plate width affects the velocity and the dimension of subduction induced mantle circulation area, and (4) mantle flow in subduction zones cannot be correctly described by models assuming a two-dimensional steady state process. We show that the intermittent toroidal component of mantle circulation, missed in those models, plays a crucial role in modifying the geometry and the efficiency of the poloidal componenten
dc.language.isoEnglishen
dc.publisher.nameAguen
dc.relation.ispartofJ. Geophys. Res.en
dc.relation.ispartofseries/111 (2006)en
dc.subjectmantle flowen
dc.subjectsubductionen
dc.titleMapping mantle flow during retreating subduction: Laboratory models analyzed by feature trackingen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberB03402en
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.01. Continentsen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.06. Subduction related processesen
dc.identifier.doi10.1029/2005JB003792en
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorFuniciello, F.en
dc.contributor.authorMoroni, M.en
dc.contributor.authorPiromallo, C.en
dc.contributor.authorFaccenna, C.en
dc.contributor.authorCenedese, A.en
dc.contributor.authorBui, H. A.en
dc.contributor.departmentDipartimento di Scienze Geologiche, Universita` Roma Treen
dc.contributor.departmentDipartimento di Idraulica, Trasporti e Strade, Universita` degli Studi di Roma ‘‘La Sapienza,’’ Rome, Italy.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentDipartimento di Scienze Geologiche, Universita` Roma Treen
dc.contributor.departmentDipartimento di Idraulica, Trasporti e Strade, Universita` degli Studi di Roma ‘‘La Sapienza,’’ Rome, Italy.en
dc.contributor.departmentDipartimento di Scienze Geologiche, Universita` Roma Treen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDipartimento di Scienze Geologiche, Universita` degli Studi ‘‘Roma Tre,’’ Rome, Italy.-
crisitem.author.deptDipartimento di Idraulica, Trasporti e Strade, Università di Roma “La Sapienza, 00184 Rome, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptUniversità Roma Tre-
crisitem.author.deptDipartimento di Idraulica, Trasporti e Strade (DITS), Università degli Studi di Roma «La Sapienza», Roma, Italy-
crisitem.author.deptDipartimento di Scienze Geologiche, Universita` Roma Tre-
crisitem.author.orcid0000-0003-3478-5128-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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