A Great Radio Burst with Abundant Fast Fine-Structures

Details A Great Radio Burst with Abundant Fast Fine-Structures A Great Radio Burst with Abundant Fast Fine-Structures

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pyuno.......36w&link_type=abstract

Publications of the Yunnan Observatory, p. 36

Physics

Solar Radio Bursts, Fine Structure, Solar Physics, Sun, High Resolution, Abundance, Statistical Distributions

Scientific paper

A great solar radio burst was observed by the four-band high-time resolution synchronous observation system in Yunnan Obs. on July 30, 1990. In this burst, abundant ms-spikes were observed at 1. 42 GHz, 2. 00 GHz and 2.84 GHz 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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