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Analysis of Vector Magnetic Fields in Solar Active Regions by Huairou, Mees and Mitaka Vector Magnetographs

机译:怀柔,米斯和三鹰矢量磁力仪分析太阳活动区中的矢量磁场

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摘要

We analyze the vector magnetograms in several well-developed active regions obtained at Huairou Solar Observing Station, National Astronomical Observatories of China, at Mees Solar Observatory, University of Hawaii, and at National Astronomical Observatory of Japan. It is found that there is a basic agreement on the transversal fields among these magnetographs. The observational error (mutual difference) for the transversal magnetic fields is estimated. In addition to comparison of transversal fields among different instruments, we used the morphological configurations of sunspot penumbrae in white-light and EUV 171 Å images obtained by the TRACE satellite as a reference of the orientation of transversal magnetic fields.
机译:我们分析了在中国国家天文台怀柔太阳观测站,夏威夷大学米斯太阳台和日本国家天文台获得的几个发达的活动区域中的矢量磁图。发现在这些磁力计之间在横向场上有基本的共识。估计横向磁场的观测误差(互差)。除了比较不同仪器之间的横向磁场外,我们还使用了白光中的黑子半影的形态结构和TRACE卫星获得的EUV 171Å图像作为横向磁场方向的参考。

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  • 来源
    《Solar Physics》 |2003年第1期|87-102|共16页
  • 作者单位

    National Astronomical Observatories Chinese Academy of Sciences;

    Institute for Astronomy University of Hawaii;

    Institute for Astronomy University of Hawaii;

    National Astronomical Observatory of Japan;

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  • 正文语种 eng
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