Toward a Consensus for Multi-Sourced Photospheric Line-of-Sight Magnetic Field Cross-Calibration

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Yang Liu, Jon Todd Hoeksema, Luca Bertello, Gordon Petrie, Alexei Pevtsov
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引用次数: 0

Abstract

In this work we compare the full-disk line-of-sight magnetic field measurements of the Helioseismic and Magnetic Imager (HMI) with the magnetograms from multiple sources including the Global Oscillation Network Group (GONG), the Michelson Doppler Imager (MDI), the Synoptic Optical Long-term Investigations of the Sun (SOLIS) instrument, the Mount Wilson Observatory (MWO), and the Wilcox Solar Observatory (WSO). A scaling factor is then derived that matches the magnetograms from these instruments to those of HMI. The scaling factors are \(1.438\pm 0.000\) for GONG, \(0.701\pm 0.001\) for MDI, \(1.038\pm 0.001\) for SOLIS, \(2.795\pm 0.002\) for MWO, and \({3.582\pm 0.006}\) for WSO. This scaling factor varies with the center-to-limb distance and field strength. Distortion maps for these instruments are also determined using the HMI data as a reference.

Abstract Image

Abstract Image

多源光球视线磁场交叉标定的共识
在这项工作中,我们比较了日震和磁成像仪(HMI)的全圆盘视线磁场测量与多个来源的磁图,包括全球振荡网络组(GONG),迈克尔逊多普勒成像仪(MDI),太阳天气光学长期调查(SOLIS)仪器,威尔逊山天文台(MWO)和威尔考克斯太阳天文台(WSO)。然后推导出一个比例因子,使这些仪器的磁图与HMI的磁图相匹配。比例系数分别为:GONG (\(1.438\pm 0.000\))、MDI (\(0.701\pm 0.001\))、SOLIS (\(1.038\pm 0.001\))、MWO (\(2.795\pm 0.002\))、WSO (\({3.582\pm 0.006}\))。该比例因子随中心到分支的距离和场强而变化。这些仪器的失真图也是使用HMI数据作为参考来确定的。
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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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