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首页> 外文期刊>The Astrophysical Journal. Supplement Series >Mount Wilson synoptic magnetic fields: Improved instrumentation, calibration, and analysis applied to the 2000 July 14 flare and to the evolution of the dipole field
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Mount Wilson synoptic magnetic fields: Improved instrumentation, calibration, and analysis applied to the 2000 July 14 flare and to the evolution of the dipole field

机译:威尔逊山天气电磁场:改进的仪器,校准和分析应用于2000年7月14日的耀斑和偶极子场的演变

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摘要

This paper describes the current status of the 150 foot solar tower telescope program of synoptic observations with an emphasis on the magnetic field data. A newly installed 24-channel system permits routine intercomparison of magnetic fields measured by the lambda676.8 nm line used by the Michelson Doppler Imager (MDI) on the Solar and Heliospheric Observatory and the lambda525.0 nm line used by the 150 foot tower. Two important calibration procedures for treatment of saturation and zero-point offset are described. It is demonstrated that solar rotation can be used to extract the east-west component of the slowly evolving, large-scale magnetic field in a stable fashion. This same analysis produces maps of the neutral line configurations that are well correlated with the positions of quiescent prominences. The analysis is applied to the 2000 July 14 are and shown to demonstrate that the field was sheared due to the westward-moving intrusion of a region just north of the neutral line along which the flaring occurred. A new method for preparing synoptic charts by averaging without differential rotation smearing is presented. These synoptic charts are combined into a new format termed a supersynoptic chart, which makes possible the identification of systematic long-term trends in the magnetic field evolution. Based on these charts, distinct large-scale events of magnetic field bias opposing the old-cycle dipole field are seen. A statistical method using the skewness in the distribution of the polarity bias as a function of longitude is developed. The coincidence between pulses in this skewness and times of rapid change in the Sun's dipole moment is consistent with the idea that a tilt in the orientation of bipolar magnetic regions is responsible for the dipole field reversal. The pulses in skewness are large and limited in number, suggesting the operation of a large-scale instability such as the kink instability. [References: 68]
机译:本文介绍了天气观测的150英尺太阳塔望远镜程序的当前状态,重点是磁场数据。新安装的24通道系统可以进行常规比对,该比对由太阳和日球观测台上的迈克尔逊多普勒成像仪(MDI)使用的lambda676.8 nm线和150英尺塔架使用的lambda525.0 nm线测量。描述了用于处理饱和度和零点偏移的两个重要的校准程序。结果表明,太阳旋转可用于以稳定的方式提取缓慢发展的大型磁场的东西方向分量。相同的分析会产生与静态突出位置紧密相关的中性线配置图。将该分析应用于2000年7月14日,并显示该油田被剪切,这是由于在发生膨胀的中性线以北的区域向西移动侵入造成的。提出了一种通过平均而无差动旋转拖影的方式来绘制天气图的新方法。这些天气图被组合成一种称为超天气图的新格式,这使人们能够确定磁场演化中系统的长期趋势。根据这些图表,可以看到与旧周期偶极子场相反的磁场偏置的各种大规模事件。开发了一种统计方法,该方法使用极性偏差的分布中的偏度作为经度的函数。这种偏斜的脉冲与太阳的偶极矩快速变化的时间之间的巧合与双极磁区取向的倾斜导致偶极子场反转的想法是一致的。偏斜的脉冲很大且数量有限,表明存在较大的不稳定性,例如扭结不稳定性。 [参考:68]

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