Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10528
DC FieldValueLanguage
dc.contributor.authorallD'Amato, D.en
dc.contributor.authorallPace, B.en
dc.contributor.authorallDi Nicola, L.en
dc.contributor.authorallStuart, F. M.en
dc.contributor.authorallVisini, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Milano-Pavia, Milano, Italiaen
dc.contributor.authorallAzzaro, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBranca, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.authorallBarfod, D. N.en
dc.date.accessioned2017-03-24T08:48:12Zen
dc.date.available2017-03-24T08:48:12Zen
dc.date.issued2017en
dc.identifier.urihttp://hdl.handle.net/2122/10528en
dc.description.abstractThe eastern flank of the Mount Etna stratovolcano is affected by extension and is slowly sliding eastward into the Ionian Sea. The Pernicana fault system forms the border of the northern part of this sliding area. It consists of three E-W–oriented fault sectors that are seismically active and characterized by earthquakes up to 4.7 in magnitude (M) capable of producing ground rupture and damage located mainly along the western and central sectors, and by continuous creep on the eastern sector. A new topographic study of the central sector of the Pernicana fault system shows an overall bell-shaped profile, with maximum scarp height of 35 m in the center of the sector, and two local minima that are probably due to the complex morphological relation between fault scarp and lava flows. We determined the ages of lava flows cut by the Pernicana fault system at 12 sites using cosmogenic 3He and 40Ar/39Ar techniques in order to determine the recent slip history of the fault. From the displacementage relations, we estimate an average throw rate of ~2.5 mm/yr over the last 15 k.y. The slip rate appears to have accelerated during the last 3.5 k.y., with displacement rates of up to ~15 mm/yr, whereas between 3.5 and 15 ka, the throw rate averaged ~1 mm/yr. This increase in slip rate resulted in significant changes in seismicity rates, for instance, decreasing the mean recurrence time of M ≥ 4.7 earthquakes from ~200 to ~20 yr. Based on empirical relationships, we attribute the variation in seismic activity on the Pernicana fault system to factors intrinsic to the system that are likely related to changes in the volcanic system. These internal factors could be fault interdependencies (such as those across the Taupo Rift, New Zealand) or they could represent interactions among magmatic, tectonic, and gravitational processes (e.g., Kīlauea volcano, Hawaii). Given their effect on earthquake recurrence intervals, these interactions need to be fully assessed in seismic hazard evaluations.en
dc.language.isoEnglishen
dc.publisher.nameGeological Society of Americaen
dc.relation.ispartofGSA Bulletinen
dc.relation.ispartofseries3-4/129 (2017)en
dc.subjectEtnaen
dc.titleHolocene slip rate variability along the Pernicana fault system (Mt. Etna, Italy): Evidence from offset lava flows.en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber304-317en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.99. General or miscellaneousen
dc.identifier.doi10.1130/B31510.1en
dc.description.obiettivoSpecifico1V. Storia e struttura dei sistemi vulcanicien
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.relation.issn0016-7606en
dc.relation.eissn1943-2674en
dc.contributor.authorD'Amato, D.en
dc.contributor.authorPace, B.en
dc.contributor.authorDi Nicola, L.en
dc.contributor.authorStuart, F. M.en
dc.contributor.authorVisini, F.en
dc.contributor.authorAzzaro, R.en
dc.contributor.authorBranca, S.en
dc.contributor.authorBarfod, D. N.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Milano-Pavia, Milano, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Catania, Catania, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptDiSPUTer Università degli Studi “G. d’Annunzio”, Chieti-Pescara, Italy-
crisitem.author.deptIsotope Geosciences Unit, Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UK-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Pisa, Pisa, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia-
crisitem.author.orcid0000-0001-9582-6443-
crisitem.author.orcid0000-0001-8294-8687-
crisitem.author.orcid0000-0002-4971-4528-
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-
Appears in Collections:Article published / in press
Files in This Item:
File Description SizeFormat
GSA Bulletin-2016-D'Amato-B31510.1.pdf9.1 MBAdobe PDFView/Open
Show simple item record

WEB OF SCIENCETM
Citations

7
checked on Feb 10, 2021

Page view(s)

912
checked on Apr 17, 2024

Download(s) 50

417
checked on Apr 17, 2024

Google ScholarTM

Check

Altmetric