NAOC Open IR
日冕电子加速的诊断—多频射电高时间分辨率观测结果
谢瑞祥; 汪敏
1997
Source Publication云南天文台台刊
ISSN1001-7526
Volume000Issue:001Pages:18
Abstract一太阳耀斑的约含数千个微耀斑,每个微耀斑以热的,低频波和加速粒子的形成释放能量。耀斑期间大部分能量的释放是通过电子加速转移的 结果,然而电子加速是在耀斑前相开始,并在整个耀斑持续期间继续保持。本文介绍几个典型事件,包括射电尖峰脉冲辐射,类尖峰辐射和短时标漂移结构。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/43882
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
谢瑞祥,汪敏. 日冕电子加速的诊断—多频射电高时间分辨率观测结果[J]. 云南天文台台刊,1997,000(001):18.
APA 谢瑞祥,&汪敏.(1997).日冕电子加速的诊断—多频射电高时间分辨率观测结果.云南天文台台刊,000(001),18.
MLA 谢瑞祥,et al."日冕电子加速的诊断—多频射电高时间分辨率观测结果".云南天文台台刊 000.001(1997):18.
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