3-D shear wave velocity model of the lithosphere below the Sardinia-Corsica continental block based on Rayleigh-wave phase velocities

dc.contributor.authorMagrini, Fabrizioen
dc.contributor.authorDiaferia, Giovannien
dc.contributor.authorFadel, Islamen
dc.contributor.authorCammarano, Fabioen
dc.contributor.authorVan Der Meijde, Marken
dc.contributor.authorBoschi, Lapoen
dc.date.accessioned2025-12-17T10:40:55Z
dc.date.available2025-12-17T10:40:55Z
dc.date.issued2020-03-01en
dc.description.abstractRayleigh-wave dispersion curves from both ambient noise and teleseismic events allow us to provide the first high-resolution 3-D shear wave velocity (VS) model of the crust and upper mantle below the Sardinia-Corsica microplate, an important continental block for understanding the evolution of the central-western Mediterranean. For a wide range of periods (from 3 to ∼30 s), the phase velocities of the study area are systematically higher than those measured within the Italian peninsula, in agreement with a colder geotherm. Relative and absolute variations in the VS allow us to detect a very heterogeneous upper crust down to 8 km, as opposed to a relatively homogeneous middle and lower crust. The isosurface at 4.1 km s-1 is consistent with a rather flat Moho at a depth of 28.0 ± 1.8 km (2σ). The lithospheric mantle is relatively cold, and we constrain the thermal lithosphere-asthenosphere boundary at ∼100 km. We find our estimate consistent with a continental geotherm based on a surface heat flow of 60 mW m-2. Our results suggest that most of the lithosphere endured the complex history of deformation experienced by the study area and imply, in general, that deep tectonic processes do not easily destabilize the deeper portion of the continental lithosphere, despite leaving a clear surface signature.en
dc.description.sponsorshipOur many exchanges with Emanuel Kästle were very beneficial to this study. We are grateful to two anonymous reviewers and the editor Ian Bastow for carefully reading and commenting our manuscript. We also thank the University of Twente for funding the installation and maintenance of the LiSard stations. The Grant to Department of Science, Roma Tre University (MIUR-Italy Dipar-timenti di Eccellenza, ARTICOLO 1, COMMI 314-337 LEGGE 232/2016) is gratefully acknowledged.en
dc.description.statusPeer-revieweden
dc.format.extent12en
dc.identifier.issn0956-540Xen
dc.identifier.otherORCID:/0000-0003-2417-2686/work/171156795en
dc.identifier.scopus85085385851en
dc.identifier.urihttps://hdl.handle.net/1885/733795777
dc.language.isoenen
dc.rightsPublisher Copyright: © 2020 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Society.en
dc.sourceGeophysical Journal Internationalen
dc.subjectComposition and structure of the continental crusten
dc.subjectCrustal imagingen
dc.subjectSeismic noiseen
dc.subjectSeismic tomographyen
dc.title3-D shear wave velocity model of the lithosphere below the Sardinia-Corsica continental block based on Rayleigh-wave phase velocitiesen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage2130en
local.bibliographicCitation.startpage2119en
local.contributor.affiliationMagrini, Fabrizio; Geophysics, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationDiaferia, Giovanni; Roma Tre Universityen
local.contributor.affiliationFadel, Islam; University of Twenteen
local.contributor.affiliationCammarano, Fabio; Roma Tre Universityen
local.contributor.affiliationVan Der Meijde, Mark; University of Twenteen
local.contributor.affiliationBoschi, Lapo; University of Paduaen
local.identifier.citationvolume220en
local.identifier.doi10.1093/gji/ggz555en
local.identifier.pure0606e1d2-d521-4299-8c9b-8cc26eb43e88en
local.identifier.urlhttps://www.scopus.com/pages/publications/85085385851en
local.type.statusPublisheden

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