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太阳射电精细结构事件的频率特性
FREQUENCY CHARACTERS OF FINE STRACTURE EVENT AT cm AND mm WAVELENGTH
【摘要】 本文分析了太阳射电短厘米、毫米波段准周期脉动现象(精细结构)的频率特性,得知该现象是由非热电子准周期注入的回旋同步辐射所致.
【Abstract】 Based on the analysis for frequency characterestics of solar radio quasi-periodic pulsation at short cm and mm wavelengths, it is found that the reahve bandwidth of such a kind of event is 5O%, and should be in wide bandwidth group. on the other hand, such a kind of phenomena occured bassically at the optical thin part or at about peak frequency of spectrum of related bulst. Thus, the fine structure may be cautal by gyro-synchrotron radiahon from quasi -periodic injechon of nonthermal electrons.
【关键词】 太阳耀斑;
短厘米;
毫米波;
精细结构事件;
【Key words】 Solar flare; Short cm-mm wavelength; Fine structure event;
【Key words】 Solar flare; Short cm-mm wavelength; Fine structure event;
【基金】 中国科学院天文委员会及太阳物理前沿课题
- 【文献出处】 空间科学学报 ,CHINESE JOURNAL OF SPACE SCIENCE , 编辑部邮箱 ,1997年01期
- 【分类号】P353.7
- 【被引频次】1
- 【下载频次】19