NAOC Open IR
太阳光球磁通量南北不对称性研究
宋文彬1; 汪景琇1; 马霞2
2005
Source Publication天文学报
ISSN0001-5245
Volume046Issue:001Pages:19
Abstract运用统计方法系统研究了1978-2002年太阳光球磁通量南北不对称性变化特征,发现其与太阳活动周有关.不对称值在太阳活动极小年要明显高于太阳活动极大年,并且磁通量变化总是由上升段的北半球占优逐渐过渡到下降段的南半球占优.另外运用小波变换方法详细讨论了这种不对称性变化可能存在的周期信息.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51952
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.中国电子科技集团公司第十所
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
宋文彬,汪景琇,马霞. 太阳光球磁通量南北不对称性研究[J]. 天文学报,2005,046(001):19.
APA 宋文彬,汪景琇,&马霞.(2005).太阳光球磁通量南北不对称性研究.天文学报,046(001),19.
MLA 宋文彬,et al."太阳光球磁通量南北不对称性研究".天文学报 046.001(2005):19.
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