Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10640
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dc.date.accessioned2017-11-21T13:19:58Zen
dc.date.available2017-11-21T13:19:58Zen
dc.date.issued2015en
dc.identifier.urihttp://hdl.handle.net/2122/10640en
dc.description.abstractThe Piano di Pezza fault is the central section of the 35 km long L’Aquila-Celano active normal fault-system in the central Apennines of Italy. Although palaeoseismic data document high Holocene vertical slip rates (∼1mm yr−1) and a remarkable seismogenic potential of this fault, its subsurface setting and Pleistocene cumulative displacement are still poorly known. We investigated for the first time the shallow subsurface of a key section of the main Piano di Pezza fault splay by means of high-resolution seismic and electrical resistivity tomography coupled with time-domain electromagnetic soundings (TDEM). Our surveys cross a ∼5-m-high fault scarp that was generated by repeated surfacerupturing earthquakes displacing Holocene alluvial fans. We provide 2-D Vp and resistivity images, which show significant details of the fault structure and the geometry of the shallow basin infill material down to 50m depth. Our data indicate that the upper fault termination has a sub-vertical attitude, in agreement with palaeoseismological trench evidence, whereas it dips ∼50◦ to the southwest in the deeper part.We recognize some low-velocity/low-resistivity regions in the fault hangingwall that we relate to packages of colluvial wedges derived from scarp degradation, which may represent the record of some Holocene palaeo-earthquakes.We estimate a ∼13–15m throw of this fault splay since the end of the Last Glacial Maximum (∼18 ka), leading to a 0.7–0.8mm yr−1 throw rate that is quite in accordance with previous palaeoseismic estimation of Holocene vertical slip rates. The 1-D resistivity models from TDEM soundings collected along the trace of the electrical profile significantly match with 2-D resistivity images. Moreover, they indicate that in the fault hangingwall, ∼200m away from the surface fault trace, the pre-Quaternary carbonate basement is at ∼90–100m depth. We therefore provide a minimal ∼150–160m estimate of the cumulative throw of the Piano di Pezza fault system in the investigated section. We further hypothesize that the onset of the Piano di Pezza fault activity may date back to the Middle Pleistocene (∼0.5 Ma), so this is a quite young active normal fault if compared to other mature normal fault systems active since 2–3 Ma in this portion of the central Apennines.en
dc.language.isoEnglishen
dc.relation.ispartofGeophysical Journal Internationalen
dc.relation.ispartofseries/203 (2015)en
dc.rightsCC0 1.0 Universalen
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/en
dc.subjectFault characterizationen
dc.subjectTDEMen
dc.subjectelectrcal resistivity methoden
dc.subjectseismic tomographyen
dc.subjectpaleoseismologyen
dc.subjectcontinental neotectonicsen
dc.titleShallow subsurface imaging of the Piano di Pezza active normal fault (central Italy) by high-resolution refraction and electrical resistivity tomography coupled with time-domain electromagnetic dataen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1482–1494en
dc.subject.INGV04.02. Exploration geophysicsen
dc.identifier.doi10.1093/gji/ggv399en
dc.description.obiettivoSpecifico2TR. Ricostruzione e modellazione della struttura crostaleen
dc.description.journalTypeJCR Journalen
dc.contributor.authorVillani, Fabioen
dc.contributor.authorTulliani, Valerioen
dc.contributor.authorSapia, Vincenzoen
dc.contributor.authorFierro, Elisaen
dc.contributor.authorCivico, Riccardoen
dc.contributor.authorPantosti, Danielaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
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 Roma2, Roma, Italia-
crisitem.author.deptAnglia Cathodic Protection Services Ltd-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptUniversità degli Studi di Camerino-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0001-7133-0136-
crisitem.author.orcid0000-0003-1958-2314-
crisitem.author.orcid0000-0002-5015-2155-
crisitem.author.orcid0000-0001-7308-9104-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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