Photometric Calibration of Spectral Imaging CoronaGraph with Dual-wavelength Observation
文献类型:期刊论文
作者 | Tang, Ning1; Liu, Wei-Xin1; Mao, Xian-Liang1; Yu, Xiao-Yu1; Zuo, Xiu-Hui1; Sun, Bo-Yu1; Zheng, Hao-Ran1; Liu, Da-Yang1; Zhang XF(张雪飞)2![]() |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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出版日期 | 2025-05-01 |
卷号 | 25期号:5 |
关键词 | Sun: corona instrumentation: miscellaneous methods: data analysis techniques: photometric |
ISSN号 | 1674-4527 |
DOI | 10.1088/1674-4527/adcc7d |
产权排序 | 第2完成单位 |
文献子类 | Article |
英文摘要 | The Spectral Imaging CoronaGraph (SICG) serves as the optical observation equipment of E-corona in the Chinese Meridian Project Phase II, which aims at monitoring the initial source of solar activities. For the purpose of in-depth exploration and space weather forecast in the full chain of Sun-Earth space, SICG is designed to work at two wavelengths of 637.4 and 530.3 nm in the quasi-simultaneous observation mode. Thus, the photometric calibration is more challenging to guarantee accurate scientific data of SICG. Two solar photometers are specially developed to match the observing wavelengths and make the photoelectronic conversion traceable. Correspondingly, the calibration process selects the solar disk center as the brightness reference, which compensates for the photometric losses along the atmospheric transmission path. This study derives the calibration coefficients from the two photometers for the E-coronal brightness processing in real time. By modeling aerosol absorption and scattering and comparing with continuous flat-field observation, the photometric calibration of SICG is evaluated with deviations of 2.1% and 2.3% at 637.4 nm and 530.3 nm, respectively. Based on this, the evolution speed of a multi-temperature coronal loop was analyzed, facilitating further research into the physical mechanisms of coronal mass ejections. |
学科主题 | 天文学 ; 天体物理学 ; 实测天体物理学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | SOLAR ; ASTROMETRY |
资助项目 | Chinese Meridian Project (CMP); National Natural Science Foundation of China[42230203]; National Natural Science Foundation of China[42374220]; National Natural Science Foundation of China[12173086] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001491993200001 |
出版者 | IOP Publishing Ltd |
资助机构 | Chinese Meridian Project (CMP) ; National Natural Science Foundation of China[42230203, 42374220, 12173086] |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/28308] ![]() |
专题 | 无名山观测站 |
作者单位 | 1.Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, China; liuwx@sdu.edu.cn; 2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China |
推荐引用方式 GB/T 7714 | Tang, Ning,Liu, Wei-Xin,Mao, Xian-Liang,et al. Photometric Calibration of Spectral Imaging CoronaGraph with Dual-wavelength Observation[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2025,25(5). |
APA | Tang, Ning.,Liu, Wei-Xin.,Mao, Xian-Liang.,Yu, Xiao-Yu.,Zuo, Xiu-Hui.,...&Xia, Li-Dong.(2025).Photometric Calibration of Spectral Imaging CoronaGraph with Dual-wavelength Observation.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,25(5). |
MLA | Tang, Ning,et al."Photometric Calibration of Spectral Imaging CoronaGraph with Dual-wavelength Observation".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 25.5(2025). |
入库方式: OAI收割
来源:云南天文台
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