中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region

文献类型:期刊论文

作者Chen, YP ; Zhou, AC
刊名SOLAR PHYSICS
出版日期2003
卷号215期号:1页码:57
关键词ELECTROMAGNETIC INSTABILITIES HEATING MECHANISMS
ISSN号0038-0938
通讯作者Chen, YP (reprint author), Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China.
中文摘要A source mechanism for the generation of shear Alfven waves in the low solar corona is suggested. It is attributed to newly created ions associated with the ionization of neutral atoms in the chromosphere - corona transition region. In the present discussion attention is mainly paid to the excitation of shear Alfven waves rather than compressional Alfven waves, i.e., fast and slow magnetosonic waves. A kinetic instability, which amplifies Alfven waves propagating in an arbitrary direction, due to the newborn ions, is studied. In the present analysis heavy ion species are emphasized.
收录类别SCI
语种英语
公开日期2013-09-24
源URL[http://ir.iphy.ac.cn/handle/311004/50119]  
专题物理研究所_物理所公开发表论文_物理所公开发表论文_期刊论文
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GB/T 7714
Chen, YP,Zhou, AC. Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region[J]. SOLAR PHYSICS,2003,215(1):57.
APA Chen, YP,&Zhou, AC.(2003).Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region.SOLAR PHYSICS,215(1),57.
MLA Chen, YP,et al."Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region".SOLAR PHYSICS 215.1(2003):57.

入库方式: OAI收割

来源:物理研究所

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