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Statistical Characteristics of Solar Proton Flares

Published online by Cambridge University Press:  12 April 2016

Jia-Long Wang
Jia-Long Wang*
Affiliation:
Beijing Astronomical Observatory Chinese Academy of Sciences Beijing 100080, China

Abstract

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An investigation of the statistical behaviour of solar flares responsible for the proton events detected at the earth orbit would be of significance for solar physics and sun-earth research. Based on the data given by Kunches (1992) and other relevant data, we study the statistical behaviour of solar proton flares. The asymmetry of distributions, special property of hard X-ray bursts and relation to the large scale mean magnetic field of the proton flares are given in this paper.

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 366 - 368
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Dennis, B.R. et al., 1991, NASA Technical Memorandum 4332, NASA, USA.Google Scholar
Dennis, B R. et al., 1992. NASA Technical Memorandum 4342, 4343, 4344, NASA USA.Google Scholar
Kunches, J. 1992, SESC PRF, 858, 25.Google Scholar
Wang, J.L., 1989, Publ. Yunnan Obs., Special Issue I, 330.Google Scholar