Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6125
DC FieldValueLanguage
dc.contributor.authorallBizzarri, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.date.accessioned2010-09-28T06:30:14Zen
dc.date.available2010-09-28T06:30:14Zen
dc.date.issued2010-09en
dc.identifier.urihttp://hdl.handle.net/2122/6125en
dc.descriptionAn edited version of this paper was published by AGU. Copyright (2010) American Geophysical Union.en
dc.description.abstractHealing of faults is an important process in earthquake source physics since it accounts for a rapid restrengthening of the fault traction and for a consequent short slip duration, as indicated by slip inversions of seismic data. In this paper we show that a laboratory‐derived constitutive model, with an explicit dependence on the temperature developed by frictional heat, can provide a suitable explanation for the generation of self‐healing slip pulses. The model requires neither special modifications at low or high speeds nor the introduction of heterogeneities in the material properties, as previously proposed. We also demonstrate through numerical experiments of 3‐D ruptures that the temperature evolution can discriminate between crack‐like and slip pulses mode of propagation. In particular, we find that for a moderate level of strain localization (slipping zone width larger than 20 mm) ruptures behave as classical enlarging cracks.en
dc.language.isoEnglishen
dc.publisher.nameAGUen
dc.relation.ispartofGeophysical Research Lettersen
dc.relation.ispartofseries/37(2010)en
dc.subjectTemperatureen
dc.subjectNumerical modelsen
dc.titlePulse‐like dynamic earthquake rupture propagation under rate‐, state‐ and temperature‐dependent frictionen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumberL18307en
dc.identifier.URLhttp://www.bo.ingv.it/~bizzarrien
dc.subject.INGV04. Solid Earth::04.06. Seismology::04.06.03. Earthquake source and dynamicsen
dc.identifier.doi10.1029/2010GL044541en
dc.description.obiettivoSpecifico3.1. Fisica dei terremotien
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorBizzarri, A.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, 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 Bologna, Bologna, Italia-
crisitem.author.orcid0000-0001-8313-4124-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Article published / in press
Files in This Item:
File Description SizeFormat Existing users please Login
2010GL044541.pdf657.11 kBAdobe PDF
Show simple item record

WEB OF SCIENCETM
Citations 50

13
checked on Feb 10, 2021

Page view(s)

87
checked on Apr 17, 2024

Download(s)

20
checked on Apr 17, 2024

Google ScholarTM

Check

Altmetric