NAOC Open IR
高纬度太阳活动的纬度漂移
高朋鑫; 李可军; 李启秀
2007
Source Publication科学通报
ISSN0023-074X
Volume052Issue:015Pages:1725
Abstract利用Carte Synoptique solar filament archive的暗条观测资料研究了高纬度太阳活动的纬度漂移.定量分析了高纬度活动的两种漂移:已知的太阳活动从中纬度(40°)向太阳两极的纬度漂移,以及新发现的从太阳两极向太阳中纬度的纬度漂移.在一个太阳活动周内从中纬度向太阳两极的纬度漂移的时间(约4.4a)比从太阳两极向太阳中纬度的纬度漂移的时间(约6.6a)要短约2.2a,这两种漂移的转换发生在太阳活动的极大期.将来,太阳活动发电机理论要考虑这种从太阳两极向太阳中纬度的纬度漂移.太阳活动延伸周是从太阳两极向太阳赤道的连续纬度漂移活动周的一部分.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/37851
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
高朋鑫,李可军,李启秀. 高纬度太阳活动的纬度漂移[J]. 科学通报,2007,052(015):1725.
APA 高朋鑫,李可军,&李启秀.(2007).高纬度太阳活动的纬度漂移.科学通报,052(015),1725.
MLA 高朋鑫,et al."高纬度太阳活动的纬度漂移".科学通报 052.015(2007):1725.
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