A group of solar microwave type III bursts with reversed drift rates on Nov. 4, 1997.

Details A group of solar microwave type III bursts with reversed drift rates on Nov. 4, 1997. A group of solar microwave type III bursts with reversed drift rates on Nov. 4, 1997.

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.266..389h&link_type=abstract

Astrophysics and Space Science, Vol. 266, No. 3, p. 389 - 398

Astronomy and Astrophysics

Astrophysics

2

Solar Microwave Bursts: Magnetic Flux Tubes

Scientific paper

The most important feature of the microwave type III bursts on November 4, 1997 is the periodically reversed drift rates, which may be contributed to a group of electron beams trapped by a huge magnetic tube (104km). It is suggested that these electron beams are accelerated by the same mechanism, because there is a power law distribution with index 3.2 in the energetic spectrum of the beam. On the other hand, the energy release in each pulse is quasi-quantized, which is confirmed by the statistical correlation between the rising time and the burst flux. Both of these two results are based on the model of plasma instability responsible for the burst.

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