AN ANALYSIS OF THE OBSERVATION OF SOLAR RADIO BURST AT THREE FREQUENCIES AT YUNNAN OBSERVATORY DURING THE SOLAR CYCLE 21

Ma Yuan; Yang Kai-ping; Luo Xian-han

doi:10.11728/cjss1991.01.059

Volume 11 Issue 1

Jan. 1991

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Ma Yuan, Yang Kai-ping, Luo Xian-han. AN ANALYSIS OF THE OBSERVATION OF SOLAR RADIO BURST AT THREE FREQUENCIES AT YUNNAN OBSERVATORY DURING THE SOLAR CYCLE 21[J]. Chinese Journal of Space Science, 1991, 11(1): 59-66. doi: 10.11728/cjss1991.01.059

Citation:

Ma Yuan, Yang Kai-ping, Luo Xian-han. AN ANALYSIS OF THE OBSERVATION OF SOLAR RADIO BURST AT THREE FREQUENCIES AT YUNNAN OBSERVATORY DURING THE SOLAR CYCLE 21[J]. Chinese Journal of Space Science, 1991, 11(1): 59-66. doi: 10.11728/cjss1991.01.059

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AN ANALYSIS OF THE OBSERVATION OF SOLAR RADIO BURST AT THREE FREQUENCIES AT YUNNAN OBSERVATORY DURING THE SOLAR CYCLE 21

doi: 10.11728/cjss1991.01.059 cstr: 32142.14.cjss1991.01.059

1.
Yunnan Observatory, Acadcmia Sinica, Kunming
2.
Department of Geophysics, Peking University

Received Date: 1989-12-11
Rev Recd Date: 1900-01-01
Publish Date: 1991-01-24

Abstract

Abstract

In this paper, the correlation between the duration and peak-flux-density of solar radio burst is analysed which is observed at 2902 MHz, 3653 MHz, 9375 MHz at Yunnan Observatory during the solar cycle 21, and the result shows that there is essentially a two-pronged distribution in all these three frequencies, and finally the relation between solar radio bursts and proton events is discussed.
- Solar radio burst,
- Proton event,
- Spotless flares