The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events

MA Yuan; XIE Rui-xiang

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Publications of the Yunnan Observatory > 2001 > 0(1): 26-31.

MA Yuan, XIE Rui-xiang. The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events[J]. Publications of the Yunnan Observatory, 2001, (1): 26-31.

Citation:

MA Yuan, XIE Rui-xiang. The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events[J]. Publications of the Yunnan Observatory, 2001, (1): 26-31.

Citation:

MA Yuan, XIE Rui-xiang. The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events[J]. Publications of the Yunnan Observatory, 2001, (1): 26-31.

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The Characteristics of Duration and Frequency of Millisecond Fast Spike Radiation Events

MA Yuan^1,2,
XIE Rui-xiang^1,2

1.
Yunnan Observatory, The Chinese Academy of Sciences, Kunming 650011
2.
China National Astronomical Observatories, The Chinese Academy of Sciences

More Information

Received Date: April 02, 2000
Revised Date: July 05, 2000
Published Date: January 14, 2001

Graphical Abstract

Abstract

Abstract

The observational observed results obtained with the Metric Wave Radio Spectrograph at the Yunnan Observatory during the solar activities of cycle 22 are introduced in this article. The statistic analyse of the duration and frequency of the 1557 individual spikes are carried out. The observational characteristics of the solar fast fine structures and their qualitative mechanism are presented.
- solar radio burst,
- fine structures