A statistical study of solar microwave fine structure events.

Details A statistical study of solar microwave fine structure events. A statistical study of solar microwave fine structure events.

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..200f&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 2, p. 200 - 206

Astronomy and Astrophysics

Astrophysics

Solar Microwave Bursts: Fine Structure

Scientific paper

A summary of the statistical results of microwave fine structure (FS) events at 2840 MHz in 1991 is presented. Statistical analyses are made for the time scale, flux density, the peak flux of associated microwave bursts, the relation between FS and Hα flare and so on. They show that the time scales of more than 67% of FS events are between tens of millisecond and hundreds of millisecond, and the amplitudes of FS events of more than 85% are less than 200 sfu. A discussion on the time scale and intensity of FS, as well as on the difference of the occurrence rate of FS events in the 21st and 22nd solar activity cycle, has also been made.

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