KMS National Astronomical Observatories, CAS
| 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 Publication | ACTA PHYSICA SINICA
 |
| ISSN | 1000-3290 |
| Volume | 54Issue:1Pages:467 |
| Abstract | In 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. |
| Keyword | CME geomagnetic storm galactic cosmic ray storm wavelet transform |
| Language | 英语 |
| Document Type | 期刊论文 |
| Identifier | http://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 Affilication | National 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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