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Study of the Pallasite Radiation History by Track Analysis

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dc.contributor.authorAlexeev, V. A.
dc.contributor.authorBagulya, A. V.
dc.contributor.authorVolkov, A. E.
dc.contributor.authorGippius, A. A.
dc.contributor.authorGrachev, V. M.
dc.contributor.authorPolukhina, N. G.
dc.contributor.authorГрачев, Виктор Михайлович
dc.contributor.authorПолухина, Наталья Геннадьевна
dc.date.accessioned2024-11-21T12:08:46Z
dc.date.available2024-11-21T12:08:46Z
dc.date.issued2019
dc.description.abstractThis work was performed within the OLYMPIA experiment on the study of tracks of heavy and superheavy cosmic ray nuclei in olivine crystals from Marjalahti and Eagle Station pallasites. Depth distributions of the track formation rate for heavy cosmic ray nuclei in olivine crystals from pallasites of different pre-atmospheric sizes were obtained. The dependences obtained were used to analyze the data on the track density in olivine crystals from the Marjalahti pallasite. In three crystals, the track distribution with a high density gradient was detected, which indicates a complicated radiation history of the meteorite.
dc.format.extentС. 251-255;
dc.identifier.citationStudy of the Pallasite Radiation History by Track Analysis / Alexeev, VA [et al.] // Bulletin of the Lebedev Physics Institute. - 2019. - 46. - № 8. - P. 251-255;. - 10.3103/S1068335619080037
dc.identifier.doi10.3103/S1068335619080037
dc.identifier.urihttps://www.doi.org/10.3103/S1068335619080037
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dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000485900400003
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/18713
dc.relation.ispartofBulletin of the Lebedev Physics Institute
dc.titleStudy of the Pallasite Radiation History by Track Analysis
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue8
oaire.citation.volume46
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