摘要
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.
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.
出处
《天文研究与技术》
CSCD
1990年第4期9-13,共5页
Astronomical Research & Technology
