PMO OpenIR  > 太阳活动的多波段观测研究团组
Chromospheric evaporation in sympathetic coronal bright points
Zhang, Q. M.; Ji, H. S.
2013-09-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume557Pages:9PP
AbstractContext. Chromospheric evaporation is a key process in solar flares that has been extensively investigated using spectroscopic observations. However, direct soft X-ray (SXR) imaging of the process is rare, especially in remote brightenings associated with the primary flares that have recently attracted a great deal of attention.
KeywordSun: Corona Sun: Activity Sun: X-Rays, Gamma Rays
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201321908
WOS KeywordLOOP RADIATIVE HYDRODYNAMICS ; MAGNETIC-FIELD CONFIGURATION ; HIGH TIME RESOLUTION ; X-RAY OBSERVATIONS ; SOLAR-FLARE LOOP ; OBSERVATIONAL EVIDENCE ; NONTHERMAL ELECTRONS ; IMPULSIVE PHASE ; REMOTE ; MODEL
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000325211900132
Citation statistics
Cited Times:17[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9960
Collection太阳活动的多波段观测研究团组
AffiliationChinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Sci, Nanjing 210008, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Zhang, Q. M.,Ji, H. S.. Chromospheric evaporation in sympathetic coronal bright points[J]. ASTRONOMY & ASTROPHYSICS,2013,557:9PP.
APA Zhang, Q. M.,&Ji, H. S..(2013).Chromospheric evaporation in sympathetic coronal bright points.ASTRONOMY & ASTROPHYSICS,557,9PP.
MLA Zhang, Q. M.,et al."Chromospheric evaporation in sympathetic coronal bright points".ASTRONOMY & ASTROPHYSICS 557(2013):9PP.
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