Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/582
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dc.contributor.authorallPittarello, L.; Dipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
dc.contributor.authorallDi Toro, G.; Dipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
dc.contributor.authorallBizzarri, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.contributor.authorallHadizadeh, J.; Department of Geography and Geosciences, University of Louisville, Kentucky USAen
dc.contributor.authorallPennacchioni, G.; Dipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
dc.date.accessioned2005-12-01T13:58:44Zen
dc.date.available2005-12-01T13:58:44Zen
dc.date.issued2005-12-04en
dc.identifier.urihttp://hdl.handle.net/2122/582en
dc.description.abstractFracture energy EG (the energy used for expanding a rupture surface area) is the fraction of work during seismic faulting that is required for creation of (i) new surfaces in the slip zone, and (ii) damage zone in the wall rocks. Partitioning of the earthquake energy between EG and frictional heat EH, determines the features of the rupture propagation and the mechanical behavior of the fault. The cataclastic microstructures associated with pseudotachylyte (solidified clast-laden friction-induced melt produced during coseismic slip) veins might contain information about the partitioning. In this preliminary study we used microstructural observations on pseudotachylytes from the Gole Larghe Fault zone (Southern Alps, Italy) to determine both EH and EG. The EH for unit fault surface area is estimated from pseudotachylyte vein thickness 2w. The energy required to produce friction melt is EH = [(1- f) H+ cP(Tm-Thr)]r 2w where f is the volume ratio of lithic clasts within the pseudotachylyte, H is the latent heat of fusion, cP is the specific heat at constant pressure, (Tm-Thr) is the difference between initial melt temperature and host rock temperature and r is the density. The EG is estimated by multiplying the newly created grain surface per unit of fault area by the specific surface energy (J m-2). In fact the studied pseudotachylyte vein contains plagioclase clasts displaying a characteristic internal fragmentation not observed in the host rock. This indicates a direct association between newly created grain surfaces and the seismic rupture process via pseudotachylyte production. It follows that pseudotachylytes might yield information on the energy partitioning between EG and EH.en
dc.format.extent2367306 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofAGU Fall Meetingen
dc.subjectEarthquake dynamicsen
dc.subjectDynamics and mechanics of faultingen
dc.subjectFractures and faultsen
dc.subjectMicrostructuresen
dc.subjectStructural goelogyen
dc.titleSeismic energy partitioning inferred from pseudotachylyte-bearing faults (Gole Larghe Fault, Adamello batholith, Italy)en
dc.typePoster sessionen
dc.description.statusUnpublisheden
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.01. Earthquake geology and paleoseismologyen
dc.description.ConferenceLocationSan Francisco, CA, USAen
dc.relation.references1. Di Toro, G., Pennacchioni, G., 2004. Superheated friction-induced melts in zoned pseudotachylytes within the Adamello tonalites (Italian Southern Alps) J. Struct. Geol. 26, 1783–1801; 2. Di Toro, G., et al., 2005. Can pseudotachylytes be used to infer earthquake source parameters? An example of limitations in the study of exhumed faults, Tectonophysics, 402, 3-20; 3. Chester, J., et al., 2005. Fracture surface energy of the Punchbowl fault, San Andreas system , Nature, 437, 133-136; 4. Wilson, B., et al., 2005. Particle size and energetics of gouge from earthquake rupture zones, Nature, 434, 749-752 5. Brace, W.F., Walsh, J.B., 1962. Some direct measurements of the surface energy of quartz and orthoclase, Am. Min. 47, 1111-1122. 6. McGarr, A., 1999. On relating apparent stress to the stress causing earthquake slip, Journal of Geophysical Research 104, 3003–3011.en
dc.description.fulltextopenen
dc.contributor.authorPittarello, L.en
dc.contributor.authorDi Toro, G.en
dc.contributor.authorBizzarri, A.en
dc.contributor.authorHadizadeh, J.en
dc.contributor.authorPennacchioni, G.en
dc.contributor.departmentDipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
dc.contributor.departmentDipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.contributor.departmentDipartimento di Geologia, Paleontologia e Geofisica, Università di Padova, Italyen
item.openairetypePoster session-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniversità degli Studi di Padova-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.deptDipartimento di Geoscienze, Università di Padova, Padova, IT-
crisitem.author.orcid0000-0002-6618-3474-
crisitem.author.orcid0000-0001-8313-4124-
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-
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