中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Short-Term Periodicity in Solar Mean Magnetic Field during Activity Maximum and Minimum Periods

文献类型:期刊论文

作者Ye, N.; Zhu, F. R.; Zhou, X. M.; Jia, H. Y.
刊名SOLAR PHYSICS
出版日期2012-08-01
卷号279页码:411-418
关键词Magnetic Fields Periodicity Solar Active Region
ISSN号0038-0938
DOI10.1007/s11207-012-0032-7
文献子类Article
英文摘要The short-term periodicity in the solar mean magnetic field (SMMF) observed at the Wilcox Solar Observatory during the last four activity cycles is investigated by using Lomb-Scargle periodograms. Our results show that the SMMF has main periods of about 27, 13.5, and 9 days in both the maximum and minimum years of each activity cycle. The SMMF has the most dominant period of about 27 days during the activity maxima. However, during the activity minimum years the 13.5-day periodicity is the most significant, except for the minimum of 1984 -aEuro parts per thousand 1986. These results indicate that the distribution of active regions in the activity maximum years is quite different from that in the minimum years.
WOS关键词CORONAL HOLES ; TIME-SERIES ; SPACED DATA ; SUN ; EVOLUTION ; WIND
语种英语
WOS记录号WOS:000306440800005
出版者SPRINGER
源URL[http://119.78.100.186/handle/113462/48659]  
专题中国科学院近代物理研究所
通讯作者Zhu, F. R.
作者单位SW Jiaotong Univ, Inst Modern Phys, Chengdu, Peoples R China
推荐引用方式
GB/T 7714
Ye, N.,Zhu, F. R.,Zhou, X. M.,et al. Short-Term Periodicity in Solar Mean Magnetic Field during Activity Maximum and Minimum Periods[J]. SOLAR PHYSICS,2012,279:411-418.
APA Ye, N.,Zhu, F. R.,Zhou, X. M.,&Jia, H. Y..(2012).Short-Term Periodicity in Solar Mean Magnetic Field during Activity Maximum and Minimum Periods.SOLAR PHYSICS,279,411-418.
MLA Ye, N.,et al."Short-Term Periodicity in Solar Mean Magnetic Field during Activity Maximum and Minimum Periods".SOLAR PHYSICS 279(2012):411-418.

入库方式: OAI收割

来源:近代物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。