Analysis of 1991 March 24 CME's structure using galactic cosmic rays' data
文献类型：期刊论文
| 作者 | Le GM(乐贵明); Han YB(韩延本) |
| 刊名 | ACTA PHYSICA SINICA
 |
| 出版日期 | 2005 |
| 卷号 | 54期号:1页码:467 |
| 关键词 | CME geomagnetic storm galactic cosmic ray storm wavelet transform |
| ISSN号 | 1000-3290 |
| 英文摘要 | 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. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/63389]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 中国科学院国家天文台 |
| 推荐引用方式 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. |
入库方式： OAI收割
来源：国家天文台
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