PMO OpenIR  > 太阳活动的多波段观测研究团组
Blobs in recurring extreme-ultraviolet jets
Zhang, Q. M.; Ji, H. S.
2014-07-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume567Issue:0Pages:0
AbstractContext. Coronal jets are one type of ubiquitous small-scale activity that is caused by magnetic reconnection in the solar corona. They are often associated with cool surges in the chromosphere.
KeywordSun: Chromosphere Sun: Corona Sun: Activity
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201423698
WOS KeywordX-RAY JETS ; CORONAL MASS EJECTIONS ; H-ALPHA SURGES ; EMISSION MEASURE ANALYSIS ; CHROMOSPHERIC ANEMONE JETS ; MOVING MAGNETIC FEATURES ; EMERGING FLUX REGION ; SOLAR-FLARE ; BLOWOUT JETS ; PHYSICAL PARAMETERS
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Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000341185300101
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/10656
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.. Blobs in recurring extreme-ultraviolet jets[J]. ASTRONOMY & ASTROPHYSICS,2014,567(0):0.
APA Zhang, Q. M.,&Ji, H. S..(2014).Blobs in recurring extreme-ultraviolet jets.ASTRONOMY & ASTROPHYSICS,567(0),0.
MLA Zhang, Q. M.,et al."Blobs in recurring extreme-ultraviolet jets".ASTRONOMY & ASTROPHYSICS 567.0(2014):0.
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