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dc.contributor.authorRieder, Milan
dc.contributor.authorGuidotti, Charles V.
dc.contributor.authorSassi, Francesco P.
dc.contributor.authorWeiss, Zdeněk
dc.date.accessioned2007-11-19T10:08:52Z
dc.date.available2007-11-19T10:08:52Z
dc.date.issued1992
dc.identifier.citationEuropean journal of mineralogy. 1992, vol. 4, no. 4, p. 843-845.en
dc.identifier.issn0935-1221
dc.identifier.urihttp://hdl.handle.net/10084/64183
dc.language.isoenen
dc.publisherE. Schweizerbart'sche Verlagsbuchhandlungen
dc.relation.ispartofseriesEuropean journal of mineralogyen
dc.relation.urihttp://eurjmin.geoscienceworld.org/cgi/content/abstract/4/4/843en
dc.subjectmuscoviteen
dc.subjectgeobarometryen
dc.subjectpowder X-ray diffractionen
dc.titleMuscovites - d060 versus d(sub 331,060) spacing - its use for geobarometric purposesen
dc.typearticleen
dc.identifier.locationNení ve fondu ÚKen
dc.description.abstract-enThe phengite peak at d almost-equal-to 1.5 angstrom, formerly often labelled as 060, is a convolution of 331BAR and 060, whose intensities are in the ratio of about 2 : 1. Since both diffracting planes are practically perpendicular to (001), no preferred orientation can separate one diffraction peak from the other. By converting d331,060BAR to b, we introduce a systematic error. The correlation between d331,060BAR and the (Fe + Mg) content of muscovites remains valid as does the use of d331,060BAR for geobarometry within a given petrological and bulk-compositional context.en
dc.identifier.wosA1992JF89600012


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