Influence of the 11-Year Solar Cycle on Variations of Cosmic Ray Intensity
文献类型:期刊论文
作者 | Ma, L. H.; Han, Y. B.; Yin, Z. Q. |
刊名 | SOLAR PHYSICS
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出版日期 | 2009-03-01 |
卷号 | 255期号:1页码:187-191 |
关键词 | Cosmic ray intensity 11-year solar cycle Wavelet transform |
英文摘要 | The monthly cosmic ray intensity (CRI) time series from Climax, Huancayo, Moscow, Kiel, and Calgary are used to investigate the presence of the 11-year periodic component with special attention paid to the solar influence on these variations. The results show obvious 11-year temporal characteristics in CRI variations. We also find a close anticorrelation between the 11-year solar cycle and CRI variations and time delays of the CRI relative to solar activity. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000263649900014 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7485] ![]() |
专题 | 国家天文台_应用天文研究部 |
作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Ma, L. H.,Han, Y. B.,Yin, Z. Q.. Influence of the 11-Year Solar Cycle on Variations of Cosmic Ray Intensity[J]. SOLAR PHYSICS,2009,255(1):187-191. |
APA | Ma, L. H.,Han, Y. B.,&Yin, Z. Q..(2009).Influence of the 11-Year Solar Cycle on Variations of Cosmic Ray Intensity.SOLAR PHYSICS,255(1),187-191. |
MLA | Ma, L. H.,et al."Influence of the 11-Year Solar Cycle on Variations of Cosmic Ray Intensity".SOLAR PHYSICS 255.1(2009):187-191. |
入库方式: OAI收割
来源:国家天文台
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