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dc.contributor.author | Sungatullin R. | |
dc.contributor.author | Sungatullina G. | |
dc.contributor.author | Zakirov M. | |
dc.contributor.author | Tsel'movich V. | |
dc.contributor.author | Glukhov M. | |
dc.contributor.author | Bakhtin A. | |
dc.contributor.author | Osin Y. | |
dc.contributor.author | Vorob'ev V. | |
dc.date.accessioned | 2018-09-19T20:58:17Z | |
dc.date.available | 2018-09-19T20:58:17Z | |
dc.date.issued | 2017 | |
dc.identifier.issn | 1068-7971 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/143472 | |
dc.description.abstract | © 2017Magnetite microspheres from the Carboniferous deposits of the Usolka reference section were studied by probe microanalysis, with comparison of the distributions of chemical elements and microspheres. The presence of microspheres in sedimentary strata is considered to be an additional factor for stratigraphic correlation between sedimentary sections. The microspheres are shown to be of cosmic nature. The Late Paleozoic paleoclimatic changes (extreme cooling) and biotic crises were caused by the periodical Solar System motion in the Galaxy, cosmic-dust fallout, and meteorite bombardments of the Earth. | |
dc.relation.ispartofseries | Russian Geology and Geophysics | |
dc.subject | Carboniferous | |
dc.subject | chemical composition | |
dc.subject | cosmic bombardment | |
dc.subject | magnetite microspheres | |
dc.subject | paleoclimate | |
dc.subject | Urals foredeep | |
dc.title | Cosmic microspheres in the Carboniferous deposits of the Usolka section (Urals foredeep) | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 58 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 59 | |
dc.source.id | SCOPUS10687971-2017-58-1-SID85013170790 |