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Preliminary Research on the Hot Spots of Energy Flares since Cycle 21

Published online by Cambridge University Press:  25 April 2016

Luo Baorong*
Affiliation:
Yunnan Observatory, Academia Sinica, PO Box 110 Kunming, China

Abstract

The time and spatial distributions of the ‘energy flare indices’ which have been observed since Cycle 21 are analysed and 13 hot spots of energy flares during this period are given in this article. These active regions of the ‘hot spots’ appear repeatedly where there erupted the energy flares accounting for 63.2 per cent of the total indices. The characteristics of the hot spots of the energy flares and the relationship between the hot spots and the evolution of the large-scale magnetic fields are also further discussed in this paper.

Type
Solar & Solar System
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Bai, T., 1988, Astrophys. J., 238, 860.Google Scholar
SESC, PRF of SCG, Nos. 66-748, (1976/12-1989/12).Google Scholar
NOAA, SCG, Part II, 1989, 544, 150.Google Scholar