A preliminary analysis for the solar radio fast structure events.

Details A preliminary analysis for the solar radio fast structure events. A preliminary analysis for the solar radio fast structure events.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acasn..36..220x&link_type=abstract

Acta Astron. Sin., Vol. 36, No. 2, p. 220 - 224

Astronomy and Astrophysics

Astronomy

Solar Radio Bursts: Fine Structure

Scientific paper

The authors present some observations of solar radio spike events at 10 cm wavelength and made a preliminary analysis of them. Some interesting results thus have been obtained as follows: 1. The widths of the spike events varies from tens of ms to hundreds of ms, and the occurrence rates of spike structure of the events ranged from 21 - 1 per second. 2. There are different characteristic structures on the morphology of the spike events.

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