NAOC Open IR
四频率太阳射电高时间分辨率观测特征:微耀斑能量释放的证据
宋谦; 谢瑞祥; 汪敏
1996
Source Publication天文学报
ISSN0001-5245
Volume037Issue:002Pages:187
Abstract作为微耀斑能量释放的证据。本文扼要介绍了云南天文台“四频率太阳射电高时间分辨率同步观测系统”(1.42,2.13,2.84和4.26GHz)1989年12月-1993月4月的观测事例,包含低强度的毫秒尖峰辐,类尖峰辐射,快速脉动现象,两种新的快速精细结构-微波Ⅲ型爆和微波类斑点结构。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/38600
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
宋谦,谢瑞祥,汪敏. 四频率太阳射电高时间分辨率观测特征:微耀斑能量释放的证据[J]. 天文学报,1996,037(002):187.
APA 宋谦,谢瑞祥,&汪敏.(1996).四频率太阳射电高时间分辨率观测特征:微耀斑能量释放的证据.天文学报,037(002),187.
MLA 宋谦,et al."四频率太阳射电高时间分辨率观测特征:微耀斑能量释放的证据".天文学报 037.002(1996):187.
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