NAOC Open IR
色球和日冕的mhd加热机制
王华宁
1996
Source Publication天文学进展
ISSN1000-8349
Volume14Issue:3Pages:204
Abstract介绍四种MHD色球和日免加热机制:(1)阿尔芬波;(2)MHD湍动;(3)场向电流;(4)磁重联.由于这四种加热机制的有效性都需要通过高分辨率观测来判定,所以空间太阳观测对于研究色球和日冕加热问题具有重大意义.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52174
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
王华宁. 色球和日冕的mhd加热机制[J]. 天文学进展,1996,14(3):204.
APA 王华宁.(1996).色球和日冕的mhd加热机制.天文学进展,14(3),204.
MLA 王华宁."色球和日冕的mhd加热机制".天文学进展 14.3(1996):204.
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