摘要
1983年以来,我们在三厘米波段研制了太阳射电活动高时间分辨率记录系统,本文对该系统作了简单介绍。简述了1984年至1986年期间所观测到的部分毫秒级快速活动资料,并作了形态分析,发现快速事件具有多种多样的快速精细结构(简称FFS),它通常以密集尖蜂脉冲群的形态出现。对今后深入开展快速活动观测研究提出了进一步的设想,并正在实施中。
A brief introduction to a fast recording system of the solar radio activity (with good time resolution) at 3.2cm which was manufactured in 1983 is given in this paper. @ The present paper has made a preliminary analysis of the fast activity events which were observed from 1984 to 1986. It can be seen from these data that the fast events have a variety of fast fine structures. They appear among the clusters of crowded spikes usually. @ Future improvements and research of the fast radio activity have been proposed and prepared.
出处
《南京大学学报（自然科学版）》
CAS
CSCD
1989年第4期584-593,共10页
Journal of Nanjing University（Natural Science）
基金
中国科学院科学基金
