中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A model for the coherent emission of solar radio moving type IV bursts

文献类型:期刊论文

作者Wang, DY
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期2004-10-01
卷号28期号:4页码:404-411
ISSN号0275-1062
关键词sun : flares radio continuum : sun plasma
英文摘要A theoretical model is proposed for interpreting the coherent emission mechanism of solar radio moving type IV bursts. Energetic electrons produced in flares captured by an expanding and rising magnetic flux tube exhibit a beam-like distribution of velocities on the top of the flux tube. These excite beaming plasma instability and directly amplifies O-mode electromagnetic waves. The instability growth rate sensitively depends on the coronal plasma parameter, f(pe)/f(ce), and the beam-temperature T-b. This can qualitatively explain the high brightness temperature and high degree of polarization as well as the broad spectrum observed in this type of solar radio bursts.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]CYCLOTRON
收录类别SCI
语种英语
WOS记录号WOS:000226493300004
公开日期2012-12-22
源URL[http://libir.pmo.ac.cn/handle/332002/7760]  
专题紫金山天文台_太阳和太阳系等离子体研究团组
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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Wang, DY. A model for the coherent emission of solar radio moving type IV bursts[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2004,28(4):404-411.
APA Wang, DY.(2004).A model for the coherent emission of solar radio moving type IV bursts.CHINESE ASTRONOMY AND ASTROPHYSICS,28(4),404-411.
MLA Wang, DY."A model for the coherent emission of solar radio moving type IV bursts".CHINESE ASTRONOMY AND ASTROPHYSICS 28.4(2004):404-411.

入库方式: OAI收割

来源:紫金山天文台

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