| 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 | https://dx.doi.org/10.1127/ejm/4/4/0843 | 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 | note | 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.doi | 10.1127/ejm/4/4/0843 | |
| dc.identifier.wos | A1992JF89600012 | |