Muscovites - d060 versus d(sub 331,060) spacing - its use for geobarometric purposes

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dc.contributor.author Rieder, Milan
dc.contributor.author Guidotti, Charles V.
dc.contributor.author Sassi, Francesco P.
dc.contributor.author Weiss, Zdeněk
dc.date.accessioned 2007-11-19T10:08:52Z
dc.date.available 2007-11-19T10:08:52Z
dc.date.issued 1992
dc.identifier.citation European journal of mineralogy. 1992, vol. 4, no. 4, p. 843-845. en
dc.identifier.issn 0935-1221
dc.identifier.uri http://hdl.handle.net/10084/64183
dc.language.iso en en
dc.publisher E. Schweizerbart'sche Verlagsbuchhandlung en
dc.relation.ispartofseries European journal of mineralogy en
dc.relation.uri http://eurjmin.geoscienceworld.org/cgi/content/abstract/4/4/843 en
dc.subject muscovite en
dc.subject geobarometry en
dc.subject powder X-ray diffraction en
dc.title Muscovites - d060 versus d(sub 331,060) spacing - its use for geobarometric purposes en
dc.type article en
dc.identifier.location Není ve fondu ÚK en
dc.description.abstract-en The 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.wos A1992JF89600012

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  • Publikační činnost VŠB-TUO / Publications of VŠB-TUO [1991]
    Kolekce obsahuje bibliografické záznamy publikační činnosti (článků) akademických pracovníků VŠB-TUO v časopisech (a v Lecture Notes in Computer Science) registrovaných ve Web of Science od roku 1990 po současnost.

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