NAOC Open IR
太阳耀斑的磁能释放机制
艾国祥1; 李醒2; 胡友秋2
1995
Source Publication科学通报
ISSN0023-074X
Volume000Issue:013Pages:1204
Abstract磁能是太阳耀斑的主要能源,但关于磁能的释放机制却众说纷纭.以往一些太阳耀斑模型或基于电流片的磁重联,或基于无力场的不稳定性,二者分别在磁能的储存和释放方面碰到困难.最近,胡友秋导出一类具奇异电流密度面(一种电流密度趋于无限但磁场连续的弱间断)的局地四极无力场解,证明该奇异电流密度面稳定,提出奇异电流密度面发展到一定程度出现的电阻耗散和不稳定性,有可能触发无力场的磁能释放,导致耀斑发生.本文采
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46734
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.中国科学技术大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
艾国祥,李醒,胡友秋. 太阳耀斑的磁能释放机制[J]. 科学通报,1995,000(013):1204.
APA 艾国祥,李醒,&胡友秋.(1995).太阳耀斑的磁能释放机制.科学通报,000(013),1204.
MLA 艾国祥,et al."太阳耀斑的磁能释放机制".科学通报 000.013(1995):1204.
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