中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Changing photospheric vector magnetic fields associated with a B4.2-class solar flare

文献类型:会议论文

作者Su, Jiangtao1,2; Liu Y(刘煜)3; Shen YD(申远灯)3
出版日期2013-07
会议日期2012-08-27
会议地点Beijing, China
关键词Sun: Photosphere Sun: Flares Sun: Magnetic Fields
卷号294
DOI10.1017/S1743921313003219
页码561-564
英文摘要

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.

产权排序第3完成单位
资助机构the Specialized Research Fund for State Key Laboratories
会议录Proceedings of the International Astronomical Union (IAU) Symposium - Solar and astrophysical dynamos and magnetic activity
会议录出版者Cambridge University Press
学科主题恒星形成与演化 ; 太阳物理学
会议录出版地Cambridge, UK
语种英语
URL标识查看原文
资助项目the 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
源URL[http://ir.ynao.ac.cn/handle/114a53/12112]  
专题云南天文台_选址与日冕观测组
通讯作者Su, Jiangtao
作者单位1.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
推荐引用方式
GB/T 7714
Su, Jiangtao,Liu Y,Shen YD. Changing photospheric vector magnetic fields associated with a B4.2-class solar flare[C]. 见:. Beijing, China. 2012-08-27.

入库方式: OAI收割

来源:云南天文台

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