Type III burst pair.

Details Type III burst pair. Type III burst pair.

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..194..137z&link_type=abstract

Solar Physics, Vol. 194, No. 1, p. 137 - 145

Physics

Solar Radio Bursts: Pairs, Solar Radio Bursts: Morphology

Scientific paper

Presents a special solar radio burst detected on 5 January 1994 using the multi-channel (50) spectrometer (1.0 - 2.0 GHz) of the Beijing Astronomical Observatory. Sadly, the whole event could not be recorded since it had a broader bandwidth than the limit range of the instrument. The important part was obtained, however. The event is composed of a normal drift type III burst on the lower frequency side and a reverse drift type III burst appearing almost simultaneously on the high side. The authors call the burst type III a burst pair. It is a typical characteristic of two type III bursts that they are morphologically symmetric about some frequency from 1.64 GHz to 1.78 GHz on the dynamic spectra records, which indicates that there are two different electron beams from the same acceleration region travelling simultaneously in opposite directions (upward and downward). A magnetic reconnection mode is an interpretation of type III burst pair.

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