| 太阳强磁区的精细结构形态 |
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| 引用本文： | 邓元勇,艾国祥.太阳强磁区的精细结构形态[J].天文学进展,1995,13(4):335-342. |
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| 作者姓名： | 邓元勇 艾国祥 |
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| 作者单位： | 中国科学院北京天文台!北京，100080，中国科学院北京天文台!北京，100080，中国科学院北京天文台!北京，100080 |
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| 摘 要： | 作者希望通过对国内外太阳物理学家多年来在太阳磁场精细结构方面的研究成果的回顾，探讨立足现有和将有的仪器设备，可能和应该从事的高分辨太阳磁场的研究工作。为突出重点，侧重评述１０００Ｇ以上的强磁场精细结构特征及与之相关的亮度特征的精细结构。
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| 关 键 词： | 太阳 磁场 强磁场 精细结构 结构形态 |
The Fine Structures of Strong Magnetic Regions on the Sun |
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| Deng Yuanyong, Wang Jingxiu, Ai Guoxiang.The Fine Structures of Strong Magnetic Regions on the Sun[J].Progress In Astronomy,1995,13(4):335-342. |
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| Authors: | Deng Yuanyong Wang Jingxiu Ai Guoxiang |
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| Abstract: | After reviewing the progress on the study of fine structures of solar magnetic fields made in the past years, we discuss what is possible to be done and what must be done about the research of high resolution solar magnetic flelds based on the instruments we have had and will have. We mainly review the fine structures of strong magnetic regions and their brightness characteristics in order to emphasize our focus. The magnetic field whose strength is above 1000G is named as strong magnetic field. Many results have proven there exist some relations between the strong magnetic field and its brightness feature that. Unfortunately, now it is not clear what they are. It will be a focus to flnd these relations because they are important for us to study the fine structures of solax magnetic fields. |
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| Keywords: | Sun magnetic field-Sun strong magnetic field-Sun fine structures-Sun brightness features-method observation |
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