NAOC Open IR
太阳射电爆发与高能质子加速过程
李春生; 傅其骏
1995
Source Publication天体物理学报
ISSN0253-2379
Volume015Issue:004Pages:350
Abstract根据近年来地面和空间观测资料的统计分析指出:(1)太阳质子事件(或质子耀斑)的发生同起伏剧烈的强微波爆发(包括脉冲和IVμ型爆发)或短分米波IV型爆发存在着紧密的共生关系(共生率趋近100%);(2)约有24%-30%的质子事件没有对应的II型爆发。这一结果否定了以前认为II型爆发中的激波加速是产生质子事件必要条件的看法,进而论证了产生强微波(脉冲或IVμ型)爆发的相对论性电子(≥500keV)与
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/43358
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
李春生,傅其骏. 太阳射电爆发与高能质子加速过程[J]. 天体物理学报,1995,015(004):350.
APA 李春生,&傅其骏.(1995).太阳射电爆发与高能质子加速过程.天体物理学报,015(004),350.
MLA 李春生,et al."太阳射电爆发与高能质子加速过程".天体物理学报 015.004(1995):350.
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