Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..12..156x&link_type=abstract
Acta Astrophys. Sin., Vol. 12, No. 2, p. 156 - 160
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
The narrow bandwidth of a solar radio spike is a characteristic parameter. Using this spike bandwidth not only the small-scale structure of spike source dimension can be calculated but also the theory of spike emission can be checked with the observations. Using the observational data with a frequency resolution of 0.5 MHz obtained at Yunnan Observatory, the authors got a bandwidth distribution of spikes in a frequency range from 230 MHz to 300 MHz, and derived the possible dimension of spike sources to be 151 km and the upper limitation to be 830 km.
Chen Jingying
Ma Yuan
Xia Zhiguo
Zheng Xiangmin
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