地表通量传输和太阳地震远侧活动区组合模型 (FARM)

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Dan Yang, Stephan G. Heinemann, Robert H. Cameron, Laurent Gizon
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引用次数: 0

摘要

太阳表面的磁场图通常被用作空间天气建模的边界条件。然而,只有太阳表面面向地球的部分才能进行连续观测。缓解远侧信息不足的一个常用方法是应用表面磁通量传输(SFT)模型来模拟太阳旋转时磁场的演变。日震学可以利用声波振荡对远侧的活跃区域进行成像,因此有可能改进建模的表面磁场。在这项研究中,我们提出了一种基于地震测量估算太阳远侧活动区磁场的新方法,然后将其纳入 SFT 模型。为了校准从日震信号到磁场的转换,我们将 SFT 模型应用于太阳动力学天文台(SDO)上的日震和磁成像仪(HMI)的视线磁图,以获得全球磁场(包括远侧)的参考图。将得到的磁场图与利用日震全息技术计算的太阳远侧日震相位图进行比较。活动区域内磁场的空间结构反映在日震相移的空间结构中。我们根据黑尔定律为单极磁场浓度分配极性,并要求两个极性之间的近似磁通量平衡。从2010年到2024年,我们模拟了859个活跃区域,平均总无符号通量为(7.84 \cdot 10^{21}\) Mx,平均面积为(4.48 \cdot 10^{10}\) km2。发现大约有(4.2%)的活跃区具有反黑尔构造,我们对其进行了人工校正。将这些远侧活跃区域包括进来,会使无符号磁图总通量平均增加(1.2%)(最多25.3%)。建模的开场区域与欧伏观测之间的比较显示,当包括远侧活跃区域时,两者之间的一致性有了很大提高。这项概念验证研究证明了 "地表通量传输和日震远侧活动区组合模型"(FARM)在改进空间天气建模方面的潜力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM)

Maps of the magnetic field at the Sun’s surface are commonly used as boundary conditions in space-weather modeling. However, continuous observations are only available from the Earth-facing part of the Sun’s surface. One commonly used approach to mitigate the lack of far-side information is to apply a surface flux transport (SFT) model to model the evolution of the magnetic field as the Sun rotates. Helioseismology can image active regions on the far side using acoustic oscillations and hence has the potential to improve the modeled surface magnetic field. In this study, we propose a novel approach for estimating magnetic fields of active regions on the Sun’s far side based on seismic measurements and then include them into an SFT model. To calibrate the conversion from helioseismic signal to magnetic field, we apply our SFT model to line-of-sight magnetograms from Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) to obtain reference maps of global magnetic fields (including the far side). The resulting magnetic maps are compared with helioseismic phase maps on the Sun’s far side computed using helioseismic holography. The spatial structure of the magnetic field within an active region is reflected in the spatial structure of the helioseismic phase shifts. We assign polarities to the unipolar magnetic-field concentrations based upon Hale’s law and require approximate flux balance between the two polarities. From 2010 to 2024, we modeled 859 active regions, with an average total unsigned flux of \(7.84 \cdot 10^{21}\) Mx and an average area of \(4.48 \cdot 10^{10}\) km2. Approximately \(4.2\%\) of the active regions were found to have an anti-Hale configuration, which we manually corrected. Including these far-side active regions resulted in an average increase of \(1.2\%\) (up to \(25.3\%\)) in the total unsigned magnetogram flux. Comparisons between modeled open-field areas and EUV observations reveal a substantial improvement in agreement when far-side active regions are included. This proof of concept study demonstrates the potential of the “combined surface flux transport and helioseismic Far-side Active Region Model” (FARM) to improve space-weather modeling.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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