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dc.contributor.authorHeider, N.
dc.contributor.authorKenkmann, T.
dc.date.accessioned2021-02-12T20:56:23Z
dc.date.available2021-02-12T20:56:23Z
dc.date.issued2003-01-01
dc.identifier.citationHeider, N., & Kenkmann, T. (2003). Numerical simulation of temperature effects at fissures due to shock loading. Meteoritics & Planetary Science, 38(10), 1451-1460.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2003.tb00250.x
dc.identifier.urihttp://hdl.handle.net/10150/655753
dc.description.abstractThe localized appearance of specific shock features in target rocks and meteorites such as melt veins and high pressure polymorphs suggests that regions with a local increase in pressure and temperature exist as a shock wave propagates through an inhomogeneous rock. In this paper, we investigate the effect of planar fissures on the local temperature distribution using numerical simulations. Time-dependent parameters such as temperature, pressure, and displacement are evaluated. The simulation model is based on a shock equation of state for the involved materials, dunite and quartzite, and simulates geometries that were also used in shock-loading experiments. An artificial gap between the materials simulates an open fissure at the interface. A strong temperature increase occurs at a gap size of 0.1 mm, which potentially can cause melting in a thin layer at the interfaces. The temperature decreases with decreasing gap size. Temperature and pressure excursions at the interface are induced by the closure of the gap, which causes a second shock wave to superpose the primary wave. Open fissures and fractures, which occur ubiquitously in shallow-buried target rocks and projectiles, thus, act as local pressure and temperature amplyfiers and may be responsible for thin melt vein formation in shocked rocks.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectLithological interface
dc.subjectFissure
dc.subjectnumerical simulation
dc.subjectShock loading
dc.titleNumerical simulation of temperature effects at fissures due to shock loading
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume38
dc.source.issue10
dc.source.beginpage1451
dc.source.endpage1460
refterms.dateFOA2021-02-12T20:56:23Z


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