米波范围内的毫秒太阳射电爆发
Millisecond solar radio bursts in the metric wavelength range
摘要：
本文对度规IV型爆发中记录到的超短结构进行了研究和分类。SSS最重要的特性是其持续时间，在半功率范围为4-50 ms，比相应频率的尖峰短10倍。太阳起源的SSSs证实了一对一的对应关系的光谱记录的Artemis-IV 1和高时间分辨率的单频测量的TSRS 2。我们将SSS分为以下几类：1。宽带SSSs：它们被划分为两个子类，SSS-Pulses和Drifting SSSs; 2.窄带：它们表现为Spike-Like SSS或Patch-Like SSS; 3.复杂SSS：它们由吸收-发射段组成，并在形态上细分为雨滴爆发（窄带发射头和宽带吸收尾）和闪烁。
英文摘要：
A study and classification of super-short structures (SSSs) recorded during metric type IV bursts is presented. The most important property of SSSs is their duration, at half power ranging from 4-50 ms, what is up to 10 times shorter than spikes at corresponding frequencies. The solar origin of the SSSs is confirmed by one-to-one correspondence between spectral recordings of Artemis-IV1 and high time resolution single frequency measurements of the TSRS2. We have divided the SSSs in the following categories: 1. Broad-Band SSSs: They were partitioned in two subcategories, the SSS-Pulses and Drifting SSSs; 2. Narrow-band: They appear either as Spike-Like SSSs or as Patch-Like SSSs; 3. Complex SSS: They consist of the absorption-emission segments and were morphologically subdivided into Rain-drop Bursts (narrow-band emission head and a broad-band absorption tail) and Blinkers.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
