Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10356
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dc.contributor.authorallBonini, L.; Dipartimento di Matematica e Geoscienze, Università di Trieste, Italyen
dc.contributor.authorallBasili, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallToscani, G.; Dipartimento di Scienze della Terra e dell'Ambiente, Università di Pavia, Pavia, Italyen
dc.contributor.authorallBurrato, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallSeno, S.; Dipartimento di Scienze della Terra e dell'Ambiente, Università di Pavia, Pavia, Italyen
dc.contributor.authorallValensise, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.date.accessioned2016-10-06T10:50:57Zen
dc.date.available2016-10-06T10:50:57Zen
dc.date.issued2016-01-29en
dc.identifier.urihttp://hdl.handle.net/2122/10356en
dc.description.abstractWe use wet-clay analogue models to investigate how pre-existing discontinuities (i.e. structures inherited from previous tectonic phases) affect the evolution of a normal fault at the Earth's surface. To this end we first perform a series of three reference experiments driven by a 45° dipping master fault unaffected by pre-existing discontinuities to generate a mechanically isotropic learning set of models. We then replicate the experiment six times introducing a 60°-dipping precut in the clay cake, each time with a different attitude and orientation with respect to an initially-blind, 45°-dipping, master normal fault. In all experiments the precut intersects the vertical projection of the master fault halfway between the center and the right-hand lateral tip. All other conditions are identical for all seven models. By comparing the results obtained from the mechanically isotropic experiments with results from experiments with precuts we find that the surface evolution of the normal fault varies depending on the precut orientation. In most cases the parameters of newly-forming faults are strongly influenced. The largest influence is exerted by synthetic and antithetic discontinuities trending respectively at 30° and 45° from the strike of the master fault, whereas a synthetic discontinuity at 60° and an antithetic discontinuity at 30° show moderate influence. Little influence is exerted by a synthetic discontinuity at 45° and an antithetic discontinuity at 60° from the strike of the master fault. We provide a ranking chart to assess fault-to-discontinuity interactions with respect to essential surface fault descriptors, such as segmentation, vertical-displacement profile, maximum displacement, and length, often used as proxies to infer fault properties at depth. Considering a single descriptor, the amount of deviation induced by different precuts varies from case to case in a rather unpredictable fashion. Multiple observables should be taken into consideration when analyzing normal faults evolving next to pre-existing discontinuities.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofTectonophysicsen
dc.relation.ispartofseries/684 (2016)en
dc.subjectFault growthen
dc.subjectnormal faulten
dc.subjectpre-existing discontinuityen
dc.subjectwetclay analogue modelen
dc.titleThe effects of pre-existing discontinuities on the surface expression of normal faults: Insights from wet-clay analogue modelingen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber157-175en
dc.identifier.URLhttp://www.sciencedirect.com/science/article/pii/S0040195115006782en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.01. Earthquake geology and paleoseismologyen
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.09. Structural geologyen
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.11. Instruments and techniquesen
dc.identifier.doi10.1016/j.tecto.2015.12.015en
dc.description.obiettivoSpecifico2T. Tettonica attivaen
dc.description.journalTypeJCR Journalen
dc.description.fulltextpartially_openen
dc.relation.issn0040-1951en
dc.relation.eissn1879-3266en
dc.contributor.authorBonini, L.en
dc.contributor.authorBasili, R.en
dc.contributor.authorToscani, G.en
dc.contributor.authorBurrato, P.en
dc.contributor.authorSeno, S.en
dc.contributor.authorValensise, G.en
dc.contributor.departmentDipartimento di Matematica e Geoscienze, Università di Trieste, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentDipartimento di Scienze della Terra e dell'Ambiente, Università di Pavia, Pavia, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentDipartimento di Scienze della Terra e dell'Ambiente, Università di Pavia, Pavia, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptDipartimento di Scienze della Terra, Università di Pavia. Via Ferrata, 1 - 27100 Pavia, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptDipartimento di Scienze della Terra, Università di Pavia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0001-5613-7813-
crisitem.author.orcid0000-0002-1213-0828-
crisitem.author.orcid0000-0001-6588-7560-
crisitem.author.orcid0000-0001-7631-1903-
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.classification.parent04. Solid Earth-
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-
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