中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
solarenergeticparticleeventof2005january20releasetimesandpossiblesources

文献类型:期刊论文

作者Guiming Le1; Yuhua Tang2; Yanben Han1
刊名chinesejournalofastronomyandastrophysics
出版日期2006
卷号6期号:6页码:751
ISSN号1009-9271
英文摘要Based on cosmic ray data obtained by neutron monitors. at the Earth's surface, and data on near-relativistic electrons measured by the WIND satellite, as well as on solar X-ray and radio burst data, the solar energetic particle (SEP) event of 2005 January 20 is studied. The results show that this event is a mixed event where the flare is dominant in the acceleration of the SEPs, the interplanetary shock accelerates mainly solar protons with energies below 130 MeV, while the relativistic protons are only accelerated by the solar flare. The interplanetary shock had an obvious acceleration effect on relativistic electrons with energies greater than 2 MeV. It was found that the solar release time for the relativistic protons was about 06:41 UT, while that for the near-relativistic electrons was about 06:39 UT. The latter turned out to be about 2 min later than the onset time of the interplanetary type III burst.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/53587]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.南京大学
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GB/T 7714
Guiming Le,Yuhua Tang,Yanben Han. solarenergeticparticleeventof2005january20releasetimesandpossiblesources[J]. chinesejournalofastronomyandastrophysics,2006,6(6):751.
APA Guiming Le,Yuhua Tang,&Yanben Han.(2006).solarenergeticparticleeventof2005january20releasetimesandpossiblesources.chinesejournalofastronomyandastrophysics,6(6),751.
MLA Guiming Le,et al."solarenergeticparticleeventof2005january20releasetimesandpossiblesources".chinesejournalofastronomyandastrophysics 6.6(2006):751.

入库方式: OAI收割

来源:国家天文台

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