NAOC Open IR
出现在Ⅳμ爆发上的快变分量
陈晓娟; 纪树臣
1997
Source Publication云南天文台台刊
ISSN1001-7526
Volume000Issue:003Pages:58
Abstract概述了1988年12月16日出现在微波Ⅳ型大爆发上的快变分量观测特征,以及由MHD调制磁流管的磁场强度,而产生了12.5min和1.2min的长短准周期振荡,呈部分高能电子被磁场俘获,做同步加速回旋辐射,产生了微波Ⅳ型爆发,另一部分能电子以一定入射角喷注磁拱上,形成螺距角各为异性的空心束分布,其电子回旋不稳定性导致spike辐射。最后,用慢波模式计算了三个频率上的1.2min的准周期振荡,结果表明
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/39733
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
陈晓娟,纪树臣. 出现在Ⅳμ爆发上的快变分量[J]. 云南天文台台刊,1997,000(003):58.
APA 陈晓娟,&纪树臣.(1997).出现在Ⅳμ爆发上的快变分量.云南天文台台刊,000(003),58.
MLA 陈晓娟,et al."出现在Ⅳμ爆发上的快变分量".云南天文台台刊 000.003(1997):58.
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