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Analysis of 1991 March 24 CME's structure using galactic cosmic rays' data
Le GM(乐贵明); Han YB(韩延本)
2005
Source PublicationACTA PHYSICA SINICA
ISSN1000-3290
Volume54Issue:1Pages:467
AbstractIn this paper, 1991 March 24 CME's structure is analyzed by determining the moment of sudden change in galactic cosmic ray intensites using wavelet method based on the sudden change in galactic cosmic ray intensities when a CME just arrives at the magnetosphere. The results show that the thickness of the CME-driven shock is about 0.2228AU, while the space scale from the front side of the CME to the most intense magnetic structure is about 0.325AU.
KeywordCME geomagnetic storm galactic cosmic ray storm wavelet transform
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/63390
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
Le GM,Han YB. Analysis of 1991 March 24 CME's structure using galactic cosmic rays' data[J]. ACTA PHYSICA SINICA,2005,54(1):467.
APA 乐贵明,&韩延本.(2005).Analysis of 1991 March 24 CME's structure using galactic cosmic rays' data.ACTA PHYSICA SINICA,54(1),467.
MLA 乐贵明,et al."Analysis of 1991 March 24 CME's structure using galactic cosmic rays' data".ACTA PHYSICA SINICA 54.1(2005):467.
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