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, Y. P. ; Zhou GC(周国成)
刊名Solar Physics
出版日期2003
卷号215期号:1页码:57-68
关键词electromagnetic instabilities heating mechanisms
ISSN号0038-0938
通讯作者北京8701信箱
英文摘要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.
学科主题空间物理
收录类别SCI
原文出处://000184251900004
语种英语
源URL[http://ir.cssar.ac.cn/handle/122/1019]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Chen, Y. P.,Zhou GC. Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region[J]. Solar Physics,2003,215(1):57-68.
APA Chen, Y. P.,&周国成.(2003).Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region.Solar Physics,215(1),57-68.
MLA Chen, Y. P.,et al."Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region".Solar Physics 215.1(2003):57-68.

入库方式: OAI收割

来源:国家空间科学中心

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