NAOC Open IR
太阳射电爆发的起因:耀斑或/和日冕物质抛射
傅其骏1; 李春生2
1999
Source Publication紫金山天文台台刊
ISSN1000-3681
Volume018Issue:002Pages:161
Abstract本文分析了近二十年来的地面和空间太阳有关观测资料,得出太阳射电爆发的起因为耀斑和/或日冕物质抛射(CME)而不仅仅是耀斑,这将有利于更深刻地了解太阳射电爆发和共生高能现象的物理过程。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/42160
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.南京大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
傅其骏,李春生. 太阳射电爆发的起因:耀斑或/和日冕物质抛射[J]. 紫金山天文台台刊,1999,018(002):161.
APA 傅其骏,&李春生.(1999).太阳射电爆发的起因:耀斑或/和日冕物质抛射.紫金山天文台台刊,018(002),161.
MLA 傅其骏,et al."太阳射电爆发的起因:耀斑或/和日冕物质抛射".紫金山天文台台刊 018.002(1999):161.
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