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Changing photospheric vector magnetic fields associated with a B4.2-class solar flare
Su, Jiangtao1,2; Liu Y(刘煜)3; Shen YD(申远灯)3
Source PublicationProceedings of the International Astronomical Union (IAU) Symposium - Solar and astrophysical dynamos and magnetic activity
2013-07
Volume294
Pages561-564
DOI10.1017/S1743921313003219
Contribution Rank第3完成单位
Indexed By其他
Conference Namethe 294th International Astronomical Union (IAU) Symposium: Solar and Astrophysical Dynamos and Magnetic Activity
Conference Date2012-08-27
Conference PlaceBeijing, China
KeywordSun: Photosphere Sun: Flares Sun: Magnetic Fields
Abstract

Recent observations have provided evidence that the solar photospheric magnetic fields could have rapid and permanent changes in both longitudinal and transverse components associated with large (X- or M-class) solar flares. However, few observations have been reported about small flares. In this paper we find the observational evidence of changing photospheric vector magnetic fields associated with a B4.2-class flare obtained with the Solar Magnetic Field Telescope (SMFT) installed at Huairou Solar Observing Station (HSOS) of Nation Astronomical Observatories of Chinese Academy of Sciences.

Funding Projectthe Grants[KJCX2-EW-T07] ; the Grants[2011CB811401] ; the Grants[11178005] ; the Grants[10878004] ; the Grants[11221063] ; the Grants[11203036] ; the Specialized Research Fund for State Key Laboratories
Funding Organizationthe Specialized Research Fund for State Key Laboratories
Language英语
Subject Area恒星形成与演化 ; 太阳物理学
MOST Discipline Catalogue理学 ; 理学::天文学
PublisherCambridge University Press
Publication PlaceCambridge, UK
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Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/12112
Collection选址与日冕观测组
Corresponding AuthorSu, Jiangtao
Affiliation1.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Science, Beijing 100012, China
2.State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100190
3.National Astronomical Observatories, Yunnan observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Su, Jiangtao,Liu Y,Shen YD. Changing photospheric vector magnetic fields associated with a B4.2-class solar flare[C]. Cambridge, UK:Cambridge University Press,2013:561-564.
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