Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acasn..27...38y&link_type=abstract
(Acta Astronomica Sinica, vol. 27, 1986, p. 38-46) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Dec. 1986, p. 3
Astronomy and Astrophysics
Astrophysics
Microwave Spectra, Radio Bursts, Solar Flares, Stellar Models, Thermal Emission, High Temperature Plasmas, Radiant Flux Density, Time Lag
Scientific paper
The parts of impulsive phase in the microwave bursts of May 13, 1981 at the different frequencies are similar to each other. Each time-profile of bursts is characterized by an approximately symmetrical structure around the peak. The durations of impulsive phase at different frequencies are nearly the same (about 25 min.). The total duration of each burst at different waves is also approximately the same. The middle part of the peak flux density spectrum is very flat. This is probably a new kind of bursts - a large gradual burst. The author suggests that the mechanism of the gradual bursts is caused by a thermal process.
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