对 ASO-S/FMG 观测到的太阳黑子 "伞 "内磁场减弱的修正

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Haiqing Xu, Jiangtao Su, Suo Liu, Yuanyong Deng, Xianyong Bai, Jie Chen, Xiaofan Wang, Xiao Yang, Yongliang Song
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引用次数: 0

摘要

先进天基太阳观测站(ASO-S)上的全盘磁图(FMG)观测到太阳黑子本影内部的磁场正在减弱。为了解决这个问题,我们采用了 Xu 等人(2021 年)开发的一种方法,对 FMG 在 2022 年 12 月 29 日至 2023 年 7 月 23 日期间观测到的 20 个活动区的数据进行了削弱校正。我们计算了太阳黑子本影内无符号磁通量的变化率\(R_{1}\),同时考虑了校正前后的测量值。变化率\(R_{1}\)从26%到124%不等,表明修正后FMG观测到的太阳黑子本影内的无符号磁通量显著增加。为了说明这一点,我们选择了四个活跃区域与太阳地震和磁成像仪(HMI)的数据进行比较。经过校正后,我们发现 FMG 测得的太阳黑子本影中的无符号磁通量与 HMI 的数据更为接近。这支持了 FMG 校正方法的有效性,尽管它还不完善,特别是在本影-半影边界。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Correction for the Weakening Magnetic Field Within the Sunspot Umbra Observed by ASO-S/FMG

Correction for the Weakening Magnetic Field Within the Sunspot Umbra Observed by ASO-S/FMG

The magnetic field inside the sunspot umbra, as observed by the Full-disk MagnetoGraph (FMG) onboard the Advanced Space based Solar Observatory (ASO-S), was found to be experiencing a weakening. To address this issue, we employed a method developed by Xu et al. (2021) to correct the weakening in the data of 20 active regions observed by FMG during the period from 29 December 2022 to 23 July 2023. Research has revealed that the onset of magnetic field weakening occurs at a minimum magnetic field strength of 705 G, with the peak strength reaching up to 1931 G. We computed the change ratio \(R_{1}\) of the unsigned magnetic flux within the sunspot umbra, considering measurements both before and after correction. The change ratio \(R_{1}\) spans from 26% to 124%, indicating a significant increase in the unsigned magnetic flux within sunspot umbrae observed by FMG after correction. To illustrate this, we selected four active regions for comparison with data from the Helioseismic and Magnetic Imager (HMI). After correction, we found that the unsigned magnetic flux in sunspot umbrae measured by FMG aligns more closely with that of HMI. This supports the effectiveness of the corrective method for FMG, despite imperfections, particularly at the umbra–penumbra boundary.

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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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