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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