中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Coexisting fast and slow propagating waves of the extreme-UV intensity in solar coronal plasma structures

文献类型:期刊论文

作者Zhang, Yuzong1; Zhang, Jun1; Wang, Jingxiu1; Nakariakov, Valery M.2,3
刊名ASTRONOMY & ASTROPHYSICS
出版日期2015-09-01
卷号581
关键词Sun: corona Sun: oscillations methods: observational
英文摘要Context. From 06: 15 UT to 08: 15 UT on 2011 June 2, a toroidal filament located at the joint of two active regions, 11226 and 11227, appeared to perform two eruptions. During this phenomenon, fast and slow magnetoacoustic waves were detected to propagate simultaneously along a funnel coronal loop system of AR 11227.
收录类别SCI
语种英语
WOS记录号WOS:000361803900078
源URL[http://ir.bao.ac.cn/handle/114a11/5562]  
专题国家天文台_太阳物理研究部
作者单位1.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
3.Russian Acad Sci Pulkovo, Cent Astron Observ, St Petersburg 196140, Russia
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GB/T 7714
Zhang, Yuzong,Zhang, Jun,Wang, Jingxiu,et al. Coexisting fast and slow propagating waves of the extreme-UV intensity in solar coronal plasma structures[J]. ASTRONOMY & ASTROPHYSICS,2015,581.
APA Zhang, Yuzong,Zhang, Jun,Wang, Jingxiu,&Nakariakov, Valery M..(2015).Coexisting fast and slow propagating waves of the extreme-UV intensity in solar coronal plasma structures.ASTRONOMY & ASTROPHYSICS,581.
MLA Zhang, Yuzong,et al."Coexisting fast and slow propagating waves of the extreme-UV intensity in solar coronal plasma structures".ASTRONOMY & ASTROPHYSICS 581(2015).

入库方式: OAI收割

来源:国家天文台

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