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Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S)
Bai, Xianyong1,2,3; Deng, Yuanyong1,2,3; Zhang, Haiying2,4; Yang, Jianfeng5; Li, Fu5; Su, Jiangtao1,2,3; Liu, Suo1,3; Song, Yongliang1,3; Ji KF(季凯帆)6; Huang, Yu7; Yang, Xiao1,3; Wang, Dongguang1,3; Lin, Jiaben1,3; Hou, Junfeng1,2,3; Sun, Yingzi1,3; Duan, Wei1,2; Song, Qian1; Bai, Yang1,3; Wang, Xiaofan1,3; Xu, Haiqing1,3; Chen, Jie1,3; Hu, Ziyao1,2,3; Zheng, Zhaoying4; Ni, Houkun4; Zeng, Yizhong4; Wu, Zhen4; Wang, Jianing4; Ge, Wei5; Lv, Juan5; Shen, Lun5; Wang, Nange5; He, Jiawei5; Wang, Chenjie5
发表期刊SOLAR PHYSICS
2024-11
卷号299期号:11
DOI10.1007/s11207-024-02400-0
产权排序第6完成单位
收录类别SCI
关键词Sun Magnetic fields Polarimetry Calibration
摘要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.
资助项目Strategic Priority Research Program of the Chinese Academy of Sciences; National Astronomical Observatories of China of CAS, Nanjing Institute of Astronomical Optics and Technology of CAS; Precision Mechanics of CAS; National Space Science Center of CAS; Innovation Academy for Microsatellites of CAS, Xi'an Microelectronics Technology Institute of China Aerospace Science and Technology Corporation, Institute of Fluid Physics, China Academy of Engineering Physics
项目资助者Strategic Priority Research Program of the Chinese Academy of Sciences ; National Astronomical Observatories of China of CAS, Nanjing Institute of Astronomical Optics and Technology of CAS ; Precision Mechanics of CAS ; National Space Science Center of CAS ; Innovation Academy for Microsatellites of CAS, Xi'an Microelectronics Technology Institute of China Aerospace Science and Technology Corporation, Institute of Fluid Physics, China Academy of Engineering Physics
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article
出版者SPRINGER
出版地VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS
ISSN0038-0938
URL查看原文
WOS记录号WOS:001354749700001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]TELESCOPE
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文献类型期刊论文
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条目标识符http://ir.ynao.ac.cn/handle/114a53/27682
专题天文技术实验室
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing, 101408, China;
3.Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;
4.Nanjing Institute of Astronomical Optics Technology, Chinese Academy of Sciences, Nanjing, 210042, China;
5.Xi’an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi’an, 710119, China;
6.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650011, China;
7.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210013, China
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Bai, Xianyong,Deng, Yuanyong,Zhang, Haiying,et al. Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S)[J]. SOLAR PHYSICS,2024,299(11).
APA Bai, Xianyong.,Deng, Yuanyong.,Zhang, Haiying.,Yang, Jianfeng.,Li, Fu.,...&Wang, Chenjie.(2024).Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S).SOLAR PHYSICS,299(11).
MLA Bai, Xianyong,et al."Calibration and Performance of the Full-Disk Vector MagnetoGraph (FMG) on Board the Advanced Space-Based Solar Observatory (ASO-S)".SOLAR PHYSICS 299.11(2024).
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