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Spikes in solar radio bursts at frequencies near 3 GHz
Wang, SJ; Yan, YH; Fu, QJ
2002-09-01
发表期刊SOLAR PHYSICS
卷号209期号:1页码:185-193
摘要Many solar microwave bursts presenting fine structures were recorded at high temporal resolution (8 ms) by the 2.6-3.8 GHz spectrometer of National Astronomical Observatories of China (NAOC). Here we present data that were recorded on 15 April 1998. After data processing, more than one hundred spikes were detected in the interval 07:59:29.622-07:59:50.362 UT. Some of the spikes were single, while others were grouped in clusters. We report the observational characteristics including lifetime, frequency bandwidth, drift rate and polarization degree, as well as duration of spike clusters. Afterwards we discuss the difference between the lifetime of the spikes presented here (near 3 GHz) and those reported formerly at frequency up to 1 GHz, the probable source density and dimension, the brightness temperature and some other characteristics.
收录类别SCI
语种英语
WOS记录号WOS:000178946700011
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8518
专题太阳物理研究部
作者单位Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Wang, SJ,Yan, YH,Fu, QJ. Spikes in solar radio bursts at frequencies near 3 GHz[J]. SOLAR PHYSICS,2002,209(1):185-193.
APA Wang, SJ,Yan, YH,&Fu, QJ.(2002).Spikes in solar radio bursts at frequencies near 3 GHz.SOLAR PHYSICS,209(1),185-193.
MLA Wang, SJ,et al."Spikes in solar radio bursts at frequencies near 3 GHz".SOLAR PHYSICS 209.1(2002):185-193.
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