中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
solarreleasetimeofsolarenergeticparticlesandassociatedaccelerationsourceincorona

文献类型:期刊论文

作者LE GuiMing1; TANG YuHua1; HAN YanBen2
刊名chinesesciencebulletin
出版日期2008
卷号53期号:2页码:161
ISSN号1001-6538
英文摘要Solar energetic particles (SEPs) are accelerated in corona at an early phase of solar energetic particle events (SEPE). The acceleration mechanism of SEPs in corona can only be inferred from an analysis of multi-band observational data, as the observation of SEPs is usually made around 1AU. In this context, people have investigated spectrums, charge state, solar release time (SRT), and multi-band data of SEPEs, in an attempt to judge the acceleration mechanism of SEPs. The SRT computation of SEPs is an important and commonly used approach to study the acceleration mechanism of SEPs in corona. This paper reviews some important findings concerning the SRT computation of SEPs, and analyzes different merits of each approach for such calculation, based on a range of SEPE case studies. This paper also analyzes and discusses both possible and actual acceleration mechanisms of a number of SEPEs, by calculating the SRT of the SEPEs. Finally, the paper summarizes the possible problems in studying an acceleration mechanism of SEPEs inferred from the SRT of SEP.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/51654]  
专题中国科学院国家天文台
作者单位1.南京大学
2.中国科学院国家天文台
推荐引用方式
GB/T 7714
LE GuiMing,TANG YuHua,HAN YanBen. solarreleasetimeofsolarenergeticparticlesandassociatedaccelerationsourceincorona[J]. chinesesciencebulletin,2008,53(2):161.
APA LE GuiMing,TANG YuHua,&HAN YanBen.(2008).solarreleasetimeofsolarenergeticparticlesandassociatedaccelerationsourceincorona.chinesesciencebulletin,53(2),161.
MLA LE GuiMing,et al."solarreleasetimeofsolarenergeticparticlesandassociatedaccelerationsourceincorona".chinesesciencebulletin 53.2(2008):161.

入库方式: OAI收割

来源:国家天文台

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