PMO OpenIR  > 太阳活动的多波段观测研究团组
A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997
Huang, GL; Fu, QJ; Qin, ZH
1999
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
Volume266Issue:3Pages:389-398
AbstractThe most important feature of the microwave type III bursts on Nov. 4, 1997 is the periodically reversed drift rates, which may be contributed to a group of electron beams trapped by a huge magnetic tube (10(4) km). It is suggested that these electron beams are accelerated by the same mechanism, because there is a power law distribution with index 3.2 in the energetic spectrum of the beam. On the other hand, the energy release in each pulse is quasi-quantized, which is confirmed by the statistical correlation between the rising time and the burst flux. Both of these two results are based on the model of plasma instability responsible for the burst.
KeywordElectron-beams Radio Flare Pulsations
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordELECTRON-BEAMS ; RADIO ; FLARE ; PULSATIONS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000087108100004
Citation statistics
Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8315
Collection太阳活动的多波段观测研究团组
Affiliation1.Purple Mt Observ, Nanjing, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100864, Peoples R China
3.Beijing Astron Observ, Beijing, Peoples R China
4.Nanjing Univ, Dept Astron, Nanjing, Peoples R China
Recommended Citation
GB/T 7714
Huang, GL,Fu, QJ,Qin, ZH. A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997[J]. ASTROPHYSICS AND SPACE SCIENCE,1999,266(3):389-398.
APA Huang, GL,Fu, QJ,&Qin, ZH.(1999).A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997.ASTROPHYSICS AND SPACE SCIENCE,266(3),389-398.
MLA Huang, GL,et al."A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997".ASTROPHYSICS AND SPACE SCIENCE 266.3(1999):389-398.
Files in This Item:
File Name/Size DocType Version Access License
1999040A group of so(111KB) 开放获取LicenseView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Huang, GL]'s Articles
[Fu, QJ]'s Articles
[Qin, ZH]'s Articles
Baidu academic
Similar articles in Baidu academic
[Huang, GL]'s Articles
[Fu, QJ]'s Articles
[Qin, ZH]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Huang, GL]'s Articles
[Fu, QJ]'s Articles
[Qin, ZH]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 1999040A group of solar microwave type III bursts with reversed drift rates on Nov 4, 1997.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.