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摘要:
We study the relation between monthly average counting rates of the cosmic ray intensity (CRI) observed at Moscow Neutron Monitoring Station, solar flare index (SFI) and coronal index during the solar cycles 22 and 23, for the period 1986-2008. The long-term behaviour of various solar activity parameters: sunspot numbers (SSN), solar flare index (Hα flare index), coronal index (CI) in relation to the duration of solar cycles 22 and 23 is examined. We find that the correlation coefficient of CRI with the coronal index as well as Hα flare index is relatively large anti-correlation during solar cycle 22. However, the monthly mean values of sunspot number, Hα flare index, and coronal index are well positively correlated with each other. We have analyzed the statistical analysis of the above parameters using of linear model and second order polynomial fits model.
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篇名 Cosmic Ray Associated with Coronal Index and Solar Flare Index during Solar Cycle 22 - 23
来源期刊 天文学与天体物理学国际期刊(英文) 学科 地球科学
关键词 SOLAR Activity SUNSPOT Number CORONAL INDEX SOLAR FLARE INDEX COSMIC Ray Intensity
年,卷(期) 2017,(3) 所属期刊栏目
研究方向 页码范围 162-173
页数 12页 分类号 P1
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SOLAR
Activity
SUNSPOT
Number
CORONAL
INDEX
SOLAR
FLARE
INDEX
COSMIC
Ray
Intensity
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天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
333
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0
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