Abstract
This paper presents a statistical summary of microwave fine structure (FS) events recorded by Beijing Astronomical Observatory at 2840 MHz in 1991. The statistical analysis shows that the time scales are between tens and hundreds of ms for more than 67% of the events and the amplitudes are less than 200 sfu in more than 85% of the cases. We discuss the time scale and intensity of FS events and the difference in the occurrence rate between the 21st and 22nd solar cycles.
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