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Fine Features of Magnetic Field and Electric Current in Solar Active Regions

机译:太阳能有源区磁场和电流的精细特征

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NOAA 10930 was a fast developing active region. We take on the analysis of the fine features of vector magnetic field in active region NOAA 10930 on 2006 December 12, which vector magnetograms were observed by SP of Hinode in Fig. 1. For resolving the 180o ambiguity of the transverse components of vector magnetograms a method for the minimum of angle difference have been used, which is to find the minimum of the azimuth angle between the observed transverse field component and that of a linear force free field, calculated by using the line-of-sight component as the boundary condition for the field normal to the image plane. It is fond the relevant consistence with the evolution of vector magnetic field in the active region, even if the magnetic field in the active region is far from the linear force free magnetic field.
机译:NOAA 10930是一种快速发展的活性区域。我们在2006年12月12日参加有源区NOAA 10930中矢量磁场的细节的分析,在图1中的Hinode的SP观察到的矢量磁力图。用于解析矢量磁图的横向部件的180o模糊性a已经使用了角度差的最小方法,这是通过使用视线部件作为边界条件来计算观察到的横向场分量和线性力场之间的方位角的最小值。对于常规到图像平面的字段。即使有源区中的磁场远离线性力的自由磁场,它也是如此与有源区中的矢量磁场的演变的相关的一致性。

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