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。现有的研究成果已经表明：磁场精细结构与亮度精细结构之间存在着某些目前还不十分明确的关系，而这种关系对小尺度磁场的研究有着重要意义，因此探索这种内分关系将是今后工作的一个重要方向。
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.
出处
《天文学进展》
CSCD
北大核心
1995年第4期335-342,共8页
Progress In Astronomy
关键词
太阳
磁场
强磁场
精细结构
结构形态
Sun
magnetic field-Sun
strong magnetic field-Sun
fine structures-Sun
brightness features-method
observation
