PMO OpenIR  > 太阳高能及相关物理过程研究团组
Progress in the heating of active region loops
Feng, L ; Gan, WQ
2005
Source PublicationCORONAL AND STELLAR MASS EJECTIONS
ISSN1743-9213
Issue226Pages:309-310
AbstractCoronal heating is an important problem in solar physics. With the development of highly qualified instruments, such as TRACE, SOHO and Yohkoh, more and more observations about coronal loops have been obtained. The coronal loops' heating, being an important ingredient of coronal heating, has been paid particular attentions recently. But there are still some key issues about the structure and mechanism of the loops' heating unresolved. In this paper, after a brief review on the latest progress in both observations and modeling of coronal loops, we emphatically discuss the heating of hydrostatic loops and hydrodynamic loops based on the ID model. The prospect of the subject is presented.
KeywordCorona Trace
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4118
Collection太阳高能及相关物理过程研究团组
Recommended Citation
GB/T 7714
Feng, L,Gan, WQ. Progress in the heating of active region loops[J]. CORONAL AND STELLAR MASS EJECTIONS,2005(226):309-310.
APA Feng, L,&Gan, WQ.(2005).Progress in the heating of active region loops.CORONAL AND STELLAR MASS EJECTIONS(226),309-310.
MLA Feng, L,et al."Progress in the heating of active region loops".CORONAL AND STELLAR MASS EJECTIONS .226(2005):309-310.
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