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
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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 | |
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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