Cosmic ray intensity variation during a CME

G. Kandemir; M. Geçkinli; C. Firat; M. Yilmaz; B. Ozugur

doi:10.1016/S0032-0633(02)00043-0

Cosmic ray intensity variation during a CME

G. Kandemir^*, M. Geçkinli, C. Firat, M. Yilmaz, B. Ozugur

^*Bu çalışma için yazışmadan sorumlu yazar

Enerji Enstitüsü

Araştırma sonucu: ???type-name??? › Makale › bilirkişi

2 Atıf (Scopus)

Özet

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%.

Orijinal dil	İngilizce
Sayfa (başlangıç-bitiş)	633-636
Sayfa sayısı	4
Dergi	Planetary and Space Science
Hacim	50
Basın numarası	5-6
DOI'lar	https://doi.org/10.1016/S0032-0633(02)00043-0
Yayın durumu	Yayınlandı - Nis 2002

Belgeye Erişim

10.1016/S0032-0633(02)00043-0

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Link to publication in Scopus

Alıntı Yap

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title = "Cosmic ray intensity variation during a CME",

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%.",

keywords = "CME, Cosmic rays, Gamma rays, Solar flares, Solar modulation",

author = "G. Kandemir and M. Ge{\c c}kinli and C. Firat and M. Yilmaz and B. Ozugur",

year = "2002",

month = apr,

doi = "10.1016/S0032-0633(02)00043-0",

language = "English",

volume = "50",

pages = "633--636",

journal = "Planetary and Space Science",

issn = "0032-0633",

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number = "5-6",

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TY - JOUR

T1 - Cosmic ray intensity variation during a CME

AU - Kandemir, G.

AU - Geçkinli, M.

AU - Firat, C.

AU - Yilmaz, M.

AU - Ozugur, B.

PY - 2002/4

Y1 - 2002/4

N2 - 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%.

AB - 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%.

KW - CME

KW - Cosmic rays

KW - Gamma rays

KW - Solar flares

KW - Solar modulation

UR - http://www.scopus.com/inward/record.url?scp=0036526365&partnerID=8YFLogxK

U2 - 10.1016/S0032-0633(02)00043-0

DO - 10.1016/S0032-0633(02)00043-0

M3 - Article

AN - SCOPUS:0036526365

SN - 0032-0633

VL - 50

SP - 633

EP - 636

JO - Planetary and Space Science

JF - Planetary and Space Science

IS - 5-6

ER -

Cosmic ray intensity variation during a CME

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