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Origin of stable remanent magnetization in LL6 chondrite, St. Severin

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dc.contributor.authorYu, Yongjae-
dc.contributor.authorDoh, Seong-Jae-
dc.contributor.authorKim, Wonnyon-
dc.contributor.authorMin, Kyoungwon-
dc.date.accessioned2021-09-07T09:57:33Z-
dc.date.available2021-09-07T09:57:33Z-
dc.date.created2021-06-19-
dc.date.issued2011-08-
dc.identifier.issn0031-9201-
dc.identifier.urihttps://scholar.korea.ac.kr/handle/2021.sw.korea/111908-
dc.description.abstractThermal demagnetization has been carried out on 20 mutually oriented chips to unravel the stable paleomagnetic record of LL6 St. Severin. Whereas the higher unblocking fractions (520-560 degrees C) of natural remanent magnetization (NRM) are directionally scattered, the lower unblocking fractions (<520 degrees C) are relatively well constrained along a great circle in a stereographic projection. Microscopic analysis revealed St. Severin to contain paramagnetic troilite and a ferromagnetic Fe-Ni system. A sharp unblocking around 560 degrees C during thermal demagnetization strongly indicates that tetrataenite is the sole NRM carrier in St. Severin. The absence of kamacite contribution on NRM and the presence of a scattered higher unblocking fraction (520-560 degrees C) of NRM imply a sequence of brecciation and a shock-induced metamorphism rather than a thermal origin of NRM. (C) 2011 Elsevier B.V. All rights reserved.-
dc.languageEnglish-
dc.language.isoen-
dc.publisherELSEVIER-
dc.subjectANALYTICAL ELECTRON-MICROSCOPY-
dc.subjectSTONY METEORITES-
dc.subjectORDERED FENI-
dc.subjectPARENT BODY-
dc.subjectCLASSIFICATION-
dc.subjectTETRATAENITE-
dc.subjectMAGNETISM-
dc.subjectSHOCK-
dc.subjectSUPERSTRUCTURE-
dc.subjectSYSTEMATICS-
dc.titleOrigin of stable remanent magnetization in LL6 chondrite, St. Severin-
dc.typeArticle-
dc.contributor.affiliatedAuthorDoh, Seong-Jae-
dc.identifier.doi10.1016/j.pepi.2011.06.004-
dc.identifier.scopusid2-s2.0-80053201256-
dc.identifier.wosid000296207900017-
dc.identifier.bibliographicCitationPHYSICS OF THE EARTH AND PLANETARY INTERIORS, v.187, no.3-4, pp.292 - 300-
dc.relation.isPartOfPHYSICS OF THE EARTH AND PLANETARY INTERIORS-
dc.citation.titlePHYSICS OF THE EARTH AND PLANETARY INTERIORS-
dc.citation.volume187-
dc.citation.number3-4-
dc.citation.startPage292-
dc.citation.endPage300-
dc.type.rimsART-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaGeochemistry & Geophysics-
dc.relation.journalWebOfScienceCategoryGeochemistry & Geophysics-
dc.subject.keywordPlusANALYTICAL ELECTRON-MICROSCOPY-
dc.subject.keywordPlusSTONY METEORITES-
dc.subject.keywordPlusORDERED FENI-
dc.subject.keywordPlusPARENT BODY-
dc.subject.keywordPlusCLASSIFICATION-
dc.subject.keywordPlusTETRATAENITE-
dc.subject.keywordPlusMAGNETISM-
dc.subject.keywordPlusSHOCK-
dc.subject.keywordPlusSUPERSTRUCTURE-
dc.subject.keywordPlusSYSTEMATICS-
dc.subject.keywordAuthorChondrite-
dc.subject.keywordAuthorMeteorite-
dc.subject.keywordAuthorSt. Severin-
dc.subject.keywordAuthorTetrataenite-
dc.subject.keywordAuthorTaenite-
dc.subject.keywordAuthorKamacite-
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