摘要
本文分析了云南天文台2902MHz、3653MHz和9375MHz 3台射电望远镜,1980年1月—1982年12月收到的太阳射电爆发的持续时间与极大流量密度的关系,发现3个波段均存在基本的两支分布,并讨论了射电爆发与质子事件、无黑子耀斑的关系.
In this paper, the correlation between the duration and peak-flux-density of solar radio burst is analysed which is observed at 2902 MHz, 3653 MHz, 9375 MHz at Yunnan Observatory during the solar cycle 21, and the result shows that there is essentially a two-pronged distribution in all these three frequencies, and finally the relation between solar radio bursts and proton events is discussed.
出处
《空间科学学报》
CAS
CSCD
北大核心
1991年第1期59-66,共8页
Chinese Journal of Space Science
关键词
太阳
射电
质子
无黑子耀斑
Solar radio burst, Proton event, Spotless flares
