中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Reciprocatory magnetic reconnection in a coronal bright point

文献类型:期刊论文

作者Zhang, Q. M.1,3; Chen, P. F.2,3; Ding, M. D.2,3; Ji, H. S.1
刊名ASTRONOMY & ASTROPHYSICS
出版日期2014-08-01
卷号568期号:0页码:0
ISSN号0004-6361
关键词Sun: corona Sun: flares Sun: X-rays, gamma rays
英文摘要Context. Coronal bright points (CBPs) are small-scale and long-duration brightenings in the lower solar corona. They are often explained in terms of magnetic reconnection.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]HOLE BOUNDARIES EVOLUTION ; X-RAY TELESCOPE ; SOLAR-FLARE ; ACTIVE-REGION ; OSCILLATORY RECONNECTION ; TRANSITION-REGION ; FLUX EMERGENCE ; EMERGING FLUX ; BLOWOUT JETS ; NULL-POINT
收录类别SCI
原文出处10.1051/0004-6361/201322815
语种英语
WOS记录号WOS:000341185900014
公开日期2014-11-20
源URL[http://libir.pmo.ac.cn/handle/332002/10654]  
专题紫金山天文台_太阳活动的多波段观测研究团组
作者单位1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Sci, Nanjing 210008, Jiangsu, Peoples R China
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
3.Minist Educ, Key Lab Modern Astron & Astrophys, Beijing, Peoples R China
推荐引用方式
GB/T 7714
Zhang, Q. M.,Chen, P. F.,Ding, M. D.,et al. Reciprocatory magnetic reconnection in a coronal bright point[J]. ASTRONOMY & ASTROPHYSICS,2014,568(0):0.
APA Zhang, Q. M.,Chen, P. F.,Ding, M. D.,&Ji, H. S..(2014).Reciprocatory magnetic reconnection in a coronal bright point.ASTRONOMY & ASTROPHYSICS,568(0),0.
MLA Zhang, Q. M.,et al."Reciprocatory magnetic reconnection in a coronal bright point".ASTRONOMY & ASTROPHYSICS 568.0(2014):0.

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来源:紫金山天文台

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