Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S)

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Xianyong Bai, Yuanyong Deng, Haiying Zhang, Jianfeng Yang, Fu Li, Jiangtao Su, Suo Liu, Yongliang Song, Kaifan Ji, Yu Huang, Xiao Yang, Dongguang Wang, Jiaben Lin, Junfeng Hou, Yingzi Sun, Wei Duan, Qian Song, Yang Bai, Xiaofan Wang, Haiqing Xu, Jie Chen, Ziyao Hu, Zhaoying Zheng, Houkun Ni, Yizhong Zeng, Zhen Wu, Jianing Wang, Wei Ge, Juan Lv, Lun Shen, Nange Wang, Jiawei He, Chenjie Wang
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引用次数: 0

Abstract

We present the ground calibration and on-orbit performance of the Full-disk vector MagnetoGraph (FMG) payload on board the Advanced Space-Based Solar Observatory (ASO-S), which is China’s first spaceborne magnetograph. FMG has the ability to acquire the full-disk Stokes I, Q/I, U/I, and V/I maps with a spatial resolution of about 1.5 arcsec. The Lyot filter for the flight model has a full width at half maximum of 0.01 nm. Using two calibration lenses, we measure the non-uniform wavelength drift across the entire field of view, with a maximum value of 0.003 nm. The on-orbit polarization sensitivity is approximately 0.00039 and 0.0009 for the deep integration and routine modes, corresponding to a cadence of 18 and 2 minutes, respectively. The corresponding sensitivity of the longitudinal magnetic field is 8.5 G and 20 G with the current linear calibration coefficient of 21,913. Since 1 April 2023, FMG has released Level 2 filtergram and longitudinal magnetic field data products for active regions. Furthermore, line-of-sight Carrington synoptic magnetograms spanning a 27-day solar rotation can be generated, which have been released to the public since February 2024. The longitudinal magnetic field obtained by FMG is consistent with that of the Helioseismic and Magnetic Imager on board the Solar Dynamic Observatory and the Solar Magnetism and Activity Telescope at Huairou Solar Observing Station for the regions without magnetic saturation.

Abstract Image

先进天基太阳观测站(ASO-S)上的全盘矢量磁图(FMG)的校准和性能
我们介绍了先进天基太阳观测站(ASO-S)上搭载的全磁盘矢量磁图(FMG)有效载荷的地面校准和在轨性能,这是中国第一台星载磁图仪。FMG 能够获取空间分辨率约为 1.5 弧秒的全磁盘斯托克斯 I、Q/I、U/I 和 V/I 图。飞行模型的 Lyot 滤波器半最大全宽为 0.01 nm。我们使用两个校准透镜测量整个视场的非均匀波长漂移,最大值为 0.003 nm。深度积分模式和常规模式的在轨偏振灵敏度分别约为 0.00039 和 0.0009,分别对应 18 分钟和 2 分钟的周期。纵向磁场的相应灵敏度为 8.5 G 和 20 G,当前的线性校准系数为 21913。自 2023 年 4 月 1 日起,FMG 发布了活动区的二级滤波图和纵向磁场数据产品。此外,还可以生成跨越 27 天太阳公转的视线卡林顿同步磁图,该磁图已于 2024 年 2 月向公众发布。对于没有磁饱和的区域,FMG 获得的纵向磁场与太阳动力学观测站上的日震和磁成像仪以及怀柔太阳观测站的太阳磁性和活动望远镜获得的纵向磁场一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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