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 | |
会议录名称 | Proceedings of the International Astronomical Union (IAU) Symposium - Solar and astrophysical dynamos and magnetic activity |
2013-07 | |
卷号 | 294 |
页码 | 561-564 |
DOI | 10.1017/S1743921313003219 |
产权排序 | 第3完成单位 |
收录类别 | 其他 |
会议名称 | the 294th International Astronomical Union (IAU) Symposium: Solar and Astrophysical Dynamos and Magnetic Activity |
会议日期 | 2012-08-27 |
会议地点 | Beijing, China |
关键词 | Sun: Photosphere Sun: Flares Sun: Magnetic Fields |
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. |
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 |
项目资助者 | the Specialized Research Fund for State Key Laboratories |
语种 | 英语 |
学科领域 | 恒星形成与演化 ; 太阳物理学 |
出版者 | Cambridge University Press |
出版地 | Cambridge, UK |
URL | 查看原文 |
引用统计 | |
文献类型 | 会议论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/12112 |
专题 | 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]. Cambridge, UK:Cambridge University Press,2013:561-564. |
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