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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/8649
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dc.contributor.authorGałązka-Friedman, Jolanta-
dc.contributor.authorWoźniak, M.-
dc.contributor.authorDuda, P.-
dc.contributor.authorRzepecka, P.-
dc.contributor.authorJakubowska, M.-
dc.contributor.authorKarwowski, Łukasz-
dc.date.accessioned2019-03-26T07:45:02Z-
dc.date.available2019-03-26T07:45:02Z-
dc.date.issued2017-
dc.identifier.citationHyperfine Interactions, Vol. 238 no. 1 (2017), art. no. 67pl_PL
dc.identifier.issn0304-3843-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/8649-
dc.description.abstractThe aim of our studies was to check the usefulness of M¨ossbauer spectroscopy for preliminary classification of ordinary chondrites. M¨ossbauer spectra of 50 samples of ordinary chondrites (type LL, L and H) obtained at room temperature were analyzed. 35 M¨ossbauer spectra were obtained in our laboratory, the other spectra were taken from the literature. The conclusion of our study was, that the most useful way for the preliminary classification of the ordinary chondrites is the application of two types of plots based on the data obtained by M¨ossbauer spectroscopy. One type of these plots is a linear plot which was used for the identification of the samples which are unrepresentative. The second type of these plots is a plot of “spectral area of the olivine” vs “spectral area of the metallic phase”. This last one was used for the identification of two unknown meteorites.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectMossbauer spectral areapl_PL
dc.subjectordinary chondritespl_PL
dc.subjectBaszkowkapl_PL
dc.subjectClassification of meteoritespl_PL
dc.titleMossbauer spectroscopy - a useful method for classification of meteorites?pl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.identifier.doi10.1007/s10751-017-1439-1-
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