NAOC Open IR
太阳微波射电快速精细结构亚类型的观测分析
汪敏; 谢瑞祥
1997
Source Publication空间科学学报
ISSN0254-6124
Volume017Issue:003Pages:234
Abstract通过分析“云南天文台4波段太阳射电快速同步观测系统”1990-01-1994-01取得的103个射电爆发,发现其中29个存在不同类型的快速精细结构。尤其是发现了几个少见的亚类FFS现象,本文仅介绍两个亚类型:窄带变周期脉动和宽带慢漂移长周期脉动。这些现象表明太阳射电FFS的多样性,它们发生在射电爆发的不同阶段(耀斑不同相),从而说明在耀斑演化中日冕非热电子的加速或注入可能贯穿于整个耀斑发展过程。由
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52125
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. 太阳微波射电快速精细结构亚类型的观测分析[J]. 空间科学学报,1997,017(003):234.
APA 汪敏,&谢瑞祥.(1997).太阳微波射电快速精细结构亚类型的观测分析.空间科学学报,017(003),234.
MLA 汪敏,et al."太阳微波射电快速精细结构亚类型的观测分析".空间科学学报 017.003(1997):234.
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