Institutional Repository System Of Yunnan Observatories, CAS
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 |
DOI | 10.1007/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 |
ISSN | 0038-0938 |
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 |
引用统计 | |
文献类型 | 期刊论文 |
版本 | 出版稿 |
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 |
推荐引用方式 GB/T 7714 | 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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Calibration and Perf(2120KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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