摘要
利用光学、射电、软X射线和硬X射线观测资料,对1986年2月系列太阳爆发中最大的两个耀斑作相似与相异性的分析,解释它们近地空间效应的区别,对该系列太阳爆发事件和叠加在一起的地球事件作认证研究.
Using observational data in optical, radio, soft and hard X-ray bands, the similarity and differences between the two top intense solar bursts of the solar activity sequence in early February 1986 are analysed, and the differences between the effects caused by these solar activities are interpreted. A relation identification of these solar-terrestrial events shows that a synthetic method for the event identification would be usable and a model study of solar corona with inhomogeneous structures and of interplanetary medium with inhomogeneous statures would be very necessary for a further investigation of coupling of solar-terrestrial disturbance events.
出处
《空间科学学报》
CAS
CSCD
北大核心
1998年第4期289-295,共7页
Chinese Journal of Space Science
基金
国家基金!49391400-2