PMO OpenIR  > 太阳活动的多波段观测研究团组
Reciprocatory magnetic reconnection in a coronal bright point
Zhang, Q. M.1,3; Chen, P. F.2,3; Ding, M. D.2,3; Ji, H. S.1
2014-08-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume568Issue:0Pages:0
AbstractContext. 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.
KeywordSun: Corona Sun: Flares Sun: X-Rays, Gamma Rays
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201322815
WOS KeywordHOLE BOUNDARIES EVOLUTION ; X-RAY TELESCOPE ; SOLAR-FLARE ; ACTIVE-REGION ; OSCILLATORY RECONNECTION ; TRANSITION-REGION ; FLUX EMERGENCE ; EMERGING FLUX ; BLOWOUT JETS ; NULL-POINT
URL查看原文
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000341185900014
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/10654
Collection太阳活动的多波段观测研究团组
Affiliation1.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
Recommended Citation
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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