The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events
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Abstract
The observational observed results obtained with the Metric Wave Radio Spectrograph at the Yunnan Observatory during the solar activities of cycle 22 are introduced in this article. The statistic analyse of the duration and frequency of the 1557 individual spikes are carried out. The observational characteristics of the solar fast fine structures and their qualitative mechanism are presented.
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