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太阳微波双峰事件的初步分析
引用本文:许富英,吴洪敖.太阳微波双峰事件的初步分析[J].空间科学学报,1999,19(2):97-101.
作者姓名:许富英  吴洪敖
作者单位:中国科学院紫金山天文台, 南京 210008
基金项目:国家自然科学重点基金!19833050,中国科学院“九五”重大项目
摘    要:本文对1989年1月-1990年6月期间的11个微波双峰事件进行了初步的分析,发现大部分双峰事件的两个峰随频率的演化呈现出竟争的趋势。这一观测特征,可由不同的非热电子分布、或相同非热电子分布,但在相同频率上不同光厚导致谱相交特征得到合理的解释,井可得到双峰事件中两个峰产生在不同源区的推论。 

关 键 词:太阳耀斑    微波事件    双峰结构
收稿时间:1998-06-25

A PRELIMINARY ANALYSIS OFSOLAR MICROWWE EVENTS WITHDOUBLE-PEAK STRVCTURES
XU Fuying ,WU Hongao.A PRELIMINARY ANALYSIS OFSOLAR MICROWWE EVENTS WITHDOUBLE-PEAK STRVCTURES[J].Chinese Journal of Space Science,1999,19(2):97-101.
Authors:XU Fuying  WU Hongao
Institution:Purple Mourstion Obsereatory, The Chinese Academy of Sciences, Nanjing 210008
Abstract:In this paper3 a preliminary analysis of eleven microwave eveals with donblepeak structures during the periods of Jan. 1989--Dec. 1990 are made. The resultsshown that the evolution of peak in most double-peak events with frequency exhibited a competition trend. Such a observing character may be interpreted resonablyby property of cross-spectra due to different distribution of nonthermal electronsor same distribution of nonthermal electrons but different optical thickness at samefrequency. Therefore, a deduction may be obtained that two peaks in the microwaveevents with double-peak structures originate from different source region, respectively.
Keywords:Solar flare  Microwave event  Double-peak structures
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