Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/16205
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dc.date.accessioned2023-02-21T11:09:38Z-
dc.date.available2023-02-21T11:09:38Z-
dc.date.issued2022-09-
dc.identifier.urihttp://hdl.handle.net/2122/16205-
dc.description.abstractMany vertical seismic velocity anomalies observed below different parts of the Eurasian plate are rooted in the transition zone between the upper and lower mantle (410–660 km), forming so-called secondary plumes. These anomalies are interpreted as the result of thermal effects of large-scale thermal upwelling (primary plume) in the lower mantle or deep dehydration of fluid-rich subducting oceanic plates. We present the results of thermo-mechanical numerical modelling to investigate the dynamics of such small-scale thermal and chemical (hydrous) anomalies rising from the lower part of the Earth’s upper mantle. Our objective is to determine the conditions that allow thermo-chemical secondary plumes of moderate size (initial radius of 50 km) to penetrate the continental lithosphere, as often detected in seismo-tomographic studies. To this end, we examine the effect of the following parameters: (1) the compositional deficit of the plume density due to the presence of water and hydrous silicate melts, (2) the width of the weak zone in the overlying lithosphere formed because of plume-induced magmatic weakening and/or previous tectonic events, and (3) a tectonic regime varied from neutral to extensional. In our models, secondary plumes of purely thermal origin do not penetrate the overlying plate, but flatten at its base, forming “mushroom”-shaped structures at the level of the lithosphere-asthenosphere boundary. On the contrary, plumes with enhanced density contrast due to a chemical (hydrous) component are shown to be able to pass upwards through the lithospheric mantle to shallow depths near the Moho when (1) the compositional density contrast is ≥ 100 kg m−3 and (2) the width of the lithospheric weakness zone above the plume is ≥ 100 km. An extensional tectonic regime facilitates plume penetration into the lithosphere but is not mandatory. Our findings can explain observations that have long remained enigmatic, such as the “arrow”-shaped zone of low seismic velocities below the Tengchong volcano in south-western China and the columnar (“finger”-shaped) anomaly within the lithospheric mantle discovered more than two decades ago beneath the Eifel volcanic fields in north-western Germany. It appears that a chemical component is a characteristic feature not only of conventional hydrous plumes located over presently downgoing oceanic slabs, but also of upper mantle plumes in other tectonic settings.en_US
dc.language.isoEnglishen_US
dc.publisher.nameElsevieren_US
dc.relation.ispartofEarth and Planetary Science Lettersen_US
dc.relation.ispartofseries/597 (2022)en_US
dc.rightsAttribution 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/us/*
dc.subjectplume-lithosphere interactionen_US
dc.subjectsecondary plumesen_US
dc.subjecthydrous plumesen_US
dc.subjectlithosphere rheologyen_US
dc.subjectmantle transition zoneen_US
dc.subjectnumerical modellingen_US
dc.titleFingerprinting secondary mantle plumesen_US
dc.typearticleen
dc.description.statusPublisheden_US
dc.type.QualityControlPeer-revieweden_US
dc.description.pagenumber117819en_US
dc.identifier.doi10.1016/j.epsl.2022.117819en_US
dc.description.obiettivoSpecifico1T. Struttura della Terraen_US
dc.description.journalTypeJCR Journalen_US
dc.relation.issn0012-821Xen_US
dc.contributor.authorCloetingh, Sierd-
dc.contributor.authorKoptev, Alexander-
dc.contributor.authorLavecchia, Alessio-
dc.contributor.authorKovács, István János-
dc.contributor.authorBeekman, Fred-
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Irpinia, Grottaminarda, Italiaen_US
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.orcid0000-0001-9472-7881-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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