NAOC Open IR  > 光学天文研究部
Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region
Chen, YP; Zhou, AC
2003-07-01
发表期刊SOLAR PHYSICS
卷号215期号:1页码:57-68
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
WOS记录号WOS:000184251900004
引用统计
被引频次:4[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8423
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, Inst Phys, Beijing 100080, Peoples R China
3.Chinese Acad Sci, Ctr Space Sci & Appl Res, Beijing 100080, Peoples R China
推荐引用方式
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):57-68.
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),57-68.
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):57-68.
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Chen, YP]的文章
[Zhou, AC]的文章
百度学术
百度学术中相似的文章
[Chen, YP]的文章
[Zhou, AC]的文章
必应学术
必应学术中相似的文章
[Chen, YP]的文章
[Zhou, AC]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。