Further numerical study of a maser instability driven by an electron beam
文献类型：期刊论文
| 作者 | Chen, YP; Zhou, GC |
| 刊名 | ACTA PHYSICA SINICA
 |
| 出版日期 | 2004-10-01 |
| 卷号 | 53期号:10页码:3398-3403 |
| 关键词 | maser-instability weak relativistic electron beam growth rate |
| 英文摘要 | Thorough numerical studies of the characters of maser-instability driven by a beam of weak relativistic electrons are performed on the basis of the theoretical model of Chen et al due to its important application in the solar radio emission. It enriches the fundamental content of the plasma instabilities. And it is expected to be applicable widely in the study of solar and celestial emission mechanism. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000224421300030 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/8396]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 2.Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing 100080, Peoples R China |
| 推荐引用方式 GB/T 7714 | Chen, YP,Zhou, GC. Further numerical study of a maser instability driven by an electron beam[J]. ACTA PHYSICA SINICA,2004,53(10):3398-3403. |
| APA | Chen, YP,&Zhou, GC.(2004).Further numerical study of a maser instability driven by an electron beam.ACTA PHYSICA SINICA,53(10),3398-3403. |
| MLA | Chen, YP,et al."Further numerical study of a maser instability driven by an electron beam".ACTA PHYSICA SINICA 53.10(2004):3398-3403. |
入库方式： OAI收割
来源：国家天文台
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