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Changing photospheric vector magnetic fields associated with a B4.2-class solar flare
Su, JT1,2; 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
DOI10.1017/S1743921313003219
产权排序第3完成单位
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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.
项目资助者the Grants(KJCX2-EW-T07, 2011CB811401, 11178005, 10878004, 11221063, 11203036) ; the Specialized Research Fund for State Key Laboratories ; the Grants(KJCX2-EW-T07, 2011CB811401, 11178005, 10878004, 11221063, 11203036) ; 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
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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, JT
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
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Su, JT,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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