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一个新型分米波太阳微耀斑现象的观测分析
汪敏; 谢瑞祥
1996
Source Publication天体物理学报
ISSN0253-2379
Volume016Issue:004Pages:421
Abstract本文介绍一组短分米波(1.42GHz)太阳微耀斑的射电和光学辐射特征,它们包含3个叠加在连续辐射背景上的射电快速精细结构(FFS),即准周期快速脉冲链(称微耀斑)它们的形态相似,强度大约在150-200sfu范围内,其寿命(半功率宽)大多为15-50ms,有18个分离的双峰结构,该事件产生的7646活动区中出现两处新浮现的几个小黑子,呈现复杂极性,可能存在多重交叉小磁流环多次重联的复杂状况,本文定
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/46256
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
汪敏,谢瑞祥. 一个新型分米波太阳微耀斑现象的观测分析[J]. 天体物理学报,1996,016(004):421.
APA 汪敏,&谢瑞祥.(1996).一个新型分米波太阳微耀斑现象的观测分析.天体物理学报,016(004),421.
MLA 汪敏,et al."一个新型分米波太阳微耀斑现象的观测分析".天体物理学报 016.004(1996):421.
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