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dc.date.accessioned2018-08-08T12:17:51Z
dc.date.available2019-09-01T22:46:19Z
dc.date.created2018-01-03T09:45:14Z
dc.date.issued2017
dc.identifier.citationRenard, Francois Cordonnier, Benoit Kobchenko, Maya Kandula, Neelima Weiss, Jérôme Zhu, Wenlu . Microscale characterization of rupture nucleation unravels precursors to faulting in rocks. Earth and Planetary Science Letters. 2017, 476, 69-78
dc.identifier.urihttp://hdl.handle.net/10852/62747
dc.description.abstractPrecursory signals, manifestations of microscale damage that precedes dynamic faulting, are key to earthquake forecasting and risk mitigation. Detections of precursors have primarily relied on measurements performed using sensors installed at some distance away from the rupture area in both field and laboratory experiments. Direct observations of continuous microscale damage accumulated during fault nucleation and propagation are scarce. Using an X-ray transparent triaxial deformation apparatus, we show the first quantitative high resolution three-dimensional (3D) information about damage evolution of rocks undergoing brittle failure. The dynamic microtomography images documented a spectrum of damage characteristics and different fault growth patterns. The interplay between various deformation mechanisms can result in either a positive, negative, or constant net volume change. Consequently, changes in rock density and acoustic wave velocities before faulting are expected to vary in different tectonics settings, hence making failure forecasting intrinsically dependent on rock type at depth.en_US
dc.languageEN
dc.publisherElsevier Science
dc.titleMicroscale characterization of rupture nucleation unravels precursors to faulting in rocksen_US
dc.typeJournal articleen_US
dc.creator.authorRenard, Francois
dc.creator.authorCordonnier, Benoit
dc.creator.authorKobchenko, Maya
dc.creator.authorKandula, Neelima
dc.creator.authorWeiss, Jérôme
dc.creator.authorZhu, Wenlu
cristin.unitcode185,15,22,20
cristin.unitnameGEO Physics of Geological processes
cristin.ispublishedtrue
cristin.fulltextpreprint
cristin.qualitycode2
dc.identifier.cristin1534357
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Earth and Planetary Science Letters&rft.volume=476&rft.spage=69&rft.date=2017
dc.identifier.jtitleEarth and Planetary Science Letters
dc.identifier.volume476
dc.identifier.startpage69
dc.identifier.endpage78
dc.identifier.doihttp://dx.doi.org/10.1016/j.epsl.2017.08.002
dc.identifier.urnURN:NBN:no-65319
dc.type.documentTidsskriftartikkelen_US
dc.source.issn0012-821X
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/62747/1/2017_EPSL_Renard_InPress.pdf
dc.type.versionSubmittedVersion


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