NAOC Open IR
晕状日冕物质抛射
汪景; 张军
2001
Source Publication天文学进展
ISSN1000-8349
Volume019Issue:002Pages:146
Abstract主要介绍晕状日冕物质抛射(halo CMEs)的产生机制,包括向量磁场演化是怎样触发halo CMEa的:halo CME与耀斑,暗条活动的相互关系怎样,是否有规律可循,暗条爆发,耀斑等活动现象是如何相互联系的,halo CME事件是由一个活动区域或一个活动事件驱动物,还是多个活动区或多个活动事件相互作用的结果,给出两个halo CME的日面起源的观测例证,提出相反极笥的磁场对消是CME日面源区磁场演化的主要特征。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47508
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
汪景,张军. 晕状日冕物质抛射[J]. 天文学进展,2001,019(002):146.
APA 汪景,&张军.(2001).晕状日冕物质抛射.天文学进展,019(002),146.
MLA 汪景,et al."晕状日冕物质抛射".天文学进展 019.002(2001):146.
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