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solarenergeticparticleeventof2005january20releasetimesandpossiblesources
Guiming Le1; Yuhua Tang2; Yanben Han1
2006
Source Publicationchinesejournalofastronomyandastrophysics
ISSN1009-9271
Volume6Issue:6Pages:751
AbstractBased 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.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/53588
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.南京大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
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.
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