Physics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pyuno..1s..135z&link_type=abstract
Publications of the Yunnan Observatory, Supplement 1989, Special issue 1, p. 135 - 140
Physics
Solar Microwave Bursts: Spectral Indices
Scientific paper
The microwave event on Nov. 10, 1988 have been analysed preliminarily. The variation of spectral index α with time appeared that α > 0 and α < 0 before and after the maximum of the burst at 11.1 cm wavelength respectively, and minus maximum near the peak of burst at 3.2 cm wavelength. Such characters of the variation of spectral indexes indicate that the microwave burst was due to gyro-synchrotron radiation of energetic electrons accelerated during the flare.
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