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Zhang Heqi, Yin Chunlin, Xu Aoao. SOME NEW STATISTICAL PROPERTIES OF SOLAR HARD X-RAY,GAMMA RAY BURSTS AND THIER ASTROPHYSICAL IMPLICATION FOR CHARGED PARTICLE ACCELERATION IN SOLAR FLARE[J]. Publications of the Yunnan Observatory, 1990, (4): 9-13.
Citation: Zhang Heqi, Yin Chunlin, Xu Aoao. SOME NEW STATISTICAL PROPERTIES OF SOLAR HARD X-RAY,GAMMA RAY BURSTS AND THIER ASTROPHYSICAL IMPLICATION FOR CHARGED PARTICLE ACCELERATION IN SOLAR FLARE[J]. Publications of the Yunnan Observatory, 1990, (4): 9-13.
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SOME NEW STATISTICAL PROPERTIES OF SOLAR HARD X-RAY,GAMMA RAY BURSTS AND THIER ASTROPHYSICAL IMPLICATION FOR CHARGED PARTICLE ACCELERATION IN SOLAR FLARE

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  • In this paper the SMM/GRS data obtained during the last solar maximum are studied. Some new statistical properties of hard X-ray and γ-ray bursts pointes out here will be significant in establishing the model of particle acceleration in solar flare. Much theoretical analyses for these results remain to be done in future.
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