Cosmic Ray Intensity Variation During a Cme
| gdc.relation.journal | Planetary and Space Science | en_US |
| dc.contributor.author | Kandemir, Gulcın | |
| dc.contributor.author | Geçkinli, Melih | |
| dc.contributor.author | Fırat, Coşkun | |
| dc.contributor.author | Yılmaz, Melek | |
| dc.contributor.author | Özuğur, B | |
| dc.contributor.other | Molecular Biology and Genetics | |
| dc.contributor.other | 05. Faculty of Engineering and Natural Sciences | |
| dc.contributor.other | 01. Kadir Has University | |
| dc.date.accessioned | 2019-06-27T08:01:02Z | |
| dc.date.available | 2019-06-27T08:01:02Z | |
| dc.date.issued | 2002 | |
| dc.description.abstract | The 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.identifier.citationcount | 2 | |
| dc.identifier.doi | 10.1016/S0032-0633(02)00043-0 | en_US |
| dc.identifier.issn | 0032-0633 | en_US |
| dc.identifier.issn | 0032-0633 | |
| dc.identifier.scopus | 2-s2.0-0036526365 | en_US |
| dc.identifier.uri | https://hdl.handle.net/20.500.12469/220 | |
| dc.identifier.uri | https://doi.org/10.1016/S0032-0633(02)00043-0 | |
| dc.language.iso | en | en_US |
| dc.publisher | Pergamon-Elsevier Science Ltd | en_US |
| dc.relation.ispartof | Planetary and Space Science | |
| dc.rights | info:eu-repo/semantics/openAccess | en_US |
| dc.subject | Cosmic rays | en_US |
| dc.subject | CME | en_US |
| dc.subject | Solar modulation | en_US |
| dc.subject | Gamma rays | en_US |
| dc.subject | Solar flares | en_US |
| dc.title | Cosmic Ray Intensity Variation During a Cme | en_US |
| dc.type | Conference Object | en_US |
| dspace.entity.type | Publication | |
| gdc.author.institutional | Kandemir, Gülçin | en_US |
| gdc.author.institutional | Özuğur Uysal, Bengü | |
| gdc.bip.impulseclass | C5 | |
| gdc.bip.influenceclass | C5 | |
| gdc.bip.popularityclass | C5 | |
| gdc.coar.access | open access | |
| gdc.coar.type | text::conference output | |
| gdc.description.department | Fakülteler, Mühendislik ve Doğa Bilimleri Fakültesi, Bilgisayar Mühendisliği Bölümü | en_US |
| gdc.description.endpage | 636 | |
| gdc.description.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | en_US |
| gdc.description.scopusquality | Q2 | |
| gdc.description.startpage | 633 | en_US |
| gdc.description.volume | 50 | en_US |
| gdc.description.wosquality | Q3 | |
| gdc.identifier.openalex | W1989380484 | |
| gdc.identifier.wos | WOS:000178534600023 | en_US |
| gdc.oaire.diamondjournal | false | |
| gdc.oaire.impulse | 0.0 | |
| gdc.oaire.influence | 2.7737808E-9 | |
| gdc.oaire.isgreen | true | |
| gdc.oaire.keywords | Solar modulation | |
| gdc.oaire.keywords | Solar flares | |
| gdc.oaire.keywords | CME | |
| gdc.oaire.keywords | Gamma rays | |
| gdc.oaire.keywords | Cosmic rays | |
| gdc.oaire.popularity | 3.1581933E-9 | |
| gdc.oaire.publicfunded | false | |
| gdc.oaire.sciencefields | 0103 physical sciences | |
| gdc.oaire.sciencefields | 01 natural sciences | |
| gdc.oaire.sciencefields | 0105 earth and related environmental sciences | |
| gdc.openalex.fwci | 0.0 | |
| gdc.openalex.normalizedpercentile | 0.63 | |
| gdc.opencitations.count | 4 | |
| gdc.plumx.crossrefcites | 1 | |
| gdc.plumx.mendeley | 9 | |
| gdc.plumx.scopuscites | 2 | |
| gdc.scopus.citedcount | 2 | |
| gdc.wos.citedcount | 2 | |
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