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Type III bursts associated with millisecond spikes which occurred within the frequency range from 230 to 300 MHz
Ma Y(马媛)1,2; Xie RX(谢瑞祥)1,2; Zheng XM(郑向明)1,2; Ma, Y (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
Source PublicationSOLAR PHYSICS
2001-05
Volume200Issue:1-2Pages:157-166
DOI10.1023/A:1010374417115
Contribution Rank第1完成单位
Indexed BySCI
AbstractThe metric spectral data obtained at the Yunnan Observatory from July 1990 to December 1991 are analysed and some type III bursts associated with millisecond spikes are found. Their different morphologies reveal the relation between the type III bursts and the millisecond spikes. Based on the occurrence time and the characteristics of continuity and changes of the morphologies in the spikes and the type III bursts of two typical events, we verify that the acceleration region of the coronal electrons is located above the emitting region of the millisecond spikes and the type III bursts. The observations show that the interface frequency of a pair of type III bursts lies near 250 MHz. Finally the authors attempt to explain qualitatively the generating mechanism of the metric millisecond spike-type III bursts by means of the plasma hypothesis.
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0038-0938
URL查看原文
Archive Date2001-10-15
WOS IDWOS:000170067700011
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordSOLAR NARROW-BAND ; RADIO-EMISSION ; CORONA
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6043
Collection太阳物理研究组
Corresponding AuthorMa, Y (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
Affiliation1.Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P.R. China
2.National Astronomical Observatories, Chinese Academy of Sciences (NAOCAS), China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Ma Y,Xie RX,Zheng XM,et al. Type III bursts associated with millisecond spikes which occurred within the frequency range from 230 to 300 MHz[J]. SOLAR PHYSICS,2001,200(1-2):157-166.
APA Ma Y,Xie RX,Zheng XM,&Ma, Y .(2001).Type III bursts associated with millisecond spikes which occurred within the frequency range from 230 to 300 MHz.SOLAR PHYSICS,200(1-2),157-166.
MLA Ma Y,et al."Type III bursts associated with millisecond spikes which occurred within the frequency range from 230 to 300 MHz".SOLAR PHYSICS 200.1-2(2001):157-166.
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