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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.
发表期刊SOLAR PHYSICS
2001-05
卷号200期号:1-2页码:157-166
DOI10.1023/A:1010374417115
产权排序第1完成单位
收录类别SCI
摘要The 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.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0038-0938
URL查看原文
归档日期2001-10-15
WOS记录号WOS:000170067700011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR NARROW-BAND ; RADIO-EMISSION ; CORONA
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6043
专题太阳物理研究组
通讯作者Ma, Y (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
作者单位1.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
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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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