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Further numerical study of a maser instability driven by an electron beam
Chen, YP; Zhou, GC
2004-10-01
Source PublicationACTA PHYSICA SINICA
Volume53Issue:10Pages:3398-3403
AbstractThorough 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.
KeywordMaser-instability Weak Relativistic Electron Beam Growth Rate
Indexed BySCI
Language英语
WOS IDWOS:000224421300030
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8396
Collection光学天文研究部
Affiliation1.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
Recommended Citation
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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