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Obliquely propagating shear Alfven waves excited by newborn ions in the chromosphere - Corona transition region
Chen, YP; Zhou, AC
2003-07-01
Source PublicationSOLAR PHYSICS
Volume215Issue:1Pages:57-68
AbstractA 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.
Indexed BySCI
Language英语
WOS IDWOS:000184251900004
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Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8423
Collection光学天文研究部
Affiliation1.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
Recommended Citation
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.
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