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Further numerical study of a maser instability driven by an electron beam
Chen, YP; Zhou, GC
2004-10-01
发表期刊ACTA PHYSICA SINICA
卷号53期号:10页码:3398-3403
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.
关键词Maser-instability Weak Relativistic Electron Beam Growth Rate
收录类别SCI
语种英语
WOS记录号WOS:000224421300030
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8396
专题光学天文研究部
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
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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.
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