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dc.contributor.authorKandemir, Gulcın
dc.contributor.authorGeçkinli, Melih
dc.contributor.authorFırat, Coşkun
dc.contributor.authorYılmaz, Melek
dc.contributor.authorÖzuğur, B
dc.date.accessioned2019-06-27T08:01:02Z
dc.date.available2019-06-27T08:01:02Z
dc.date.issued2002
dc.identifier.issn0032-0633en_US
dc.identifier.urihttps://hdl.handle.net/20.500.12469/220
dc.identifier.urihttps://doi.org/10.1016/S0032-0633(02)00043-0
dc.description.abstractThe June 6 2000 coronal mass ejection was an exceptional full halo which made it possible to measure cosmic ray (CR) decrease with a simple experimental set-up. Variation in the local secondary cosmic ray density has been investigated by means of gamma rays. The experiment site was located in Istanbul (41.1N 29.0E). CR electrons and slow gamma rays have been eliminated. The CR density has dropped drastically starting on June 8 2000. The counts have been compared with the pre-shock levels and some other cases of CMEs. During strong solar modulation the local counts of secondary CR intensity values dropped down as much as 24%. (C) 2002 Elsevier Science Ltd. All rights reserved.en_US]
dc.language.isoengen_US
dc.publisherPergamon-Elsevier Science Ltden_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectCosmic raysen_US
dc.subjectCMEen_US
dc.subjectSolar modulationen_US
dc.subjectGamma raysen_US
dc.subjectSolar flaresen_US
dc.titleCosmic ray intensity variation during a CMEen_US
dc.typeconferenceObjecten_US
dc.identifier.startpage633en_US
dc.identifier.endpage636
dc.relation.journalPlanetary and Space Scienceen_US
dc.identifier.volume50en_US
dc.departmentFakülteler, Mühendislik ve Doğa Bilimleri Fakültesi, Bilgisayar Mühendisliği Bölümüen_US
dc.identifier.wosWOS:000178534600023en_US
dc.identifier.doi10.1016/S0032-0633(02)00043-0en_US
dc.identifier.scopus2-s2.0-0036526365en_US
dc.institutionauthorKandemir, Gülçinen_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US


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