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A Quantitative Study on Magnetic Configuration for Active Regions

机译:活性区的磁性构型的定量研究

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摘要

As compared with the Mount Wilson Magnetic Classification (MWMC), effective distance (d E) is a useful parameter because it gives a quantitative measure of magnetic configuration in active regions. We have analyzed magnetograms of 24 active regions of different types with MWMC. We have studied the evolution of magnetic fields of five active regions using d E, total flux (F t) and tilt angle (Tilt) quantitatively. Furthermore, 43 flare-associated and 25 CME-associated active regions have been studied to investigate and quantify the statistical correlation between flares/CMEs and the three parameters. The main results are as follows: (1) There is a basic agreement between d E and MWMC. (2) The evolution of magnetic fields can be described in three aspects quantitatively and accurately by the three parameters, in particular by d E on the analysis of δ-type active regions. (3) The high correlation between d E and flares/CMEs means that d E could be a promising measure to predict the flare-CME activity of active regions.
机译:与威尔逊山磁分类法(MWMC)相比,有效距离(d E )是一个有用的参数,因为它可以定量测量活动区域中的磁配置。我们用MWMC分析了24种不同类型的活动区域的磁图。我们使用d E ,总通量(F t )和倾斜角(Tilt)定量研究了五个活动区域的磁场演化。此外,已经研究了与耀斑相关的43个活动区域和与CME相关的25个活动区域,以研究和量化耀斑/ CME与这三个参数之间的统计相关性。主要结果如下:(1)d E 与MWMC之间有基本的约定。 (2)磁场的演化可以通过这三个参数来定量,准确地从三个方面来描述,尤其是在分析δ型有源区时用d E 来描述。 (3)d E 与耀斑/ CME之间的高度相关性意味着d E 可能是预测活性区域耀斑CME活性的有前途的手段。

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  • 来源
    《Solar Physics 》 |2006年第1期| 25-43| 共19页
  • 作者单位

    National Astronomical Observatories Chinese Academy of Science;

    National Astronomical Observatories Chinese Academy of Science;

    Sternberg Astronomical Institute (SAI) Moscow State University;

    Institute for Astronomy University of Hawaii;

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  • 正文语种 eng
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