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太阳射电快速事件的初析
引用本文:许富英 吴洪敖. 太阳射电快速事件的初析[J]. 天文学报, 1995, 36(2): 220-224
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
基金项目:中国科学院重大项目,天文委太阳物理学科组,紫金山天文台择优基金
摘    要:本文着重介绍了紫金山天文台在10cm波段上观测到的太阳射电快速结构事件资料,并对其进行了初步的分析.得到的一些结果如下:1.快速事件的宽度介于几十毫秒一几百毫秒的变化范围内;每秒出现的频数介于21-1之间;2.从spikes事件的形态上,也有着不同的结构特征;有的spike结构比较简单,基本上是一个个的单脉冲,而有的则比较复杂,即在每个spike尖峰上,还叠加有亚-精细结构。

关 键 词:太阳射电 精细结构事件 耀斑

A PRELIMINARY ANALYSIS FOR THE SOLAR RADIO FAST STRUCTURE EVENTS
Xu Fu-ying, Wu Hong-ao. A PRELIMINARY ANALYSIS FOR THE SOLAR RADIO FAST STRUCTURE EVENTS[J]. Acta Astronomica Sinica, 1995, 36(2): 220-224
Authors:Xu Fu-ying   Wu Hong-ao
Abstract:In this paper, we present some solar radio spike events at 10cm wavelength observed at Purple Mountain Observatory, and made a preliminary analysis for them.Some interesting results thus have been obtained as follows: 1. The widths of the spike events varied from tens of ms to hundredes of ms, and the occurrence rates of spike structure of the events ranged from 21-1 per second; 2. There are different characteristic structures on the morphology of the spike events. For instance, some events consist of single impulse with simple rise and fall time structure, while others are rather complex structures with subfine structure superposed on the peaks of the spike events.
Keywords:Solar radio emission  Fine structure event
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