NAOC Open IR
太阳剩余磁场研究进展
宋文彬; 汪景琇
2005
Source Publication天文学进展
ISSN1000-8349
Volume023Issue:003Pages:205
Abstract太阳剩余磁场是指形成于太阳主序星阶段之前,深藏在太阳辐射核内部的原始磁场。由于太阳内部高电导率和准静态等因素,其剩余磁场耗散相当缓慢,而得以保留至今。太阳剩余磁场的存在不仅能够解释太阳活动的很多不对称性现象,如南北不对称性、活动经度与活动穴、低纬度冕洞和Maunder极小期等,还能通过改变自激发发电机模型的边值条件而影响整个太阳表面磁场的分布与演化。从观测结果和理论模型两方面评述了太阳剩余磁场的研究成果及最新进展,并简单讨论了进一步努力的方向。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46871
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
宋文彬,汪景琇. 太阳剩余磁场研究进展[J]. 天文学进展,2005,023(003):205.
APA 宋文彬,&汪景琇.(2005).太阳剩余磁场研究进展.天文学进展,023(003),205.
MLA 宋文彬,et al."太阳剩余磁场研究进展".天文学进展 023.003(2005):205.
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