A Great Radio Burst With Abundant Fast Fine-Structures
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Abstract
A great solar radio burst was observed by the four-band high-time resolution synchrnous observation ststem in Yunnan Obs. on July 30, 1990. In this burst, abundant ms-spikes were observed at 1.42GHz, 2.00Hz and 2.84GHz respectively. The statistical distributions of the lifetimes and intensities of this ms-spikes are presented in this paper. The characteristics of this ms-spikes are also discussed.
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