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A full-disk image standardization of the chromosphere observation at Huairou Solar Observing Station
Suo, Liu1,2
刊名ADVANCES IN SPACE RESEARCH
2020-02-01
卷号65期号:3页码:1054-1061
关键词Chromosphere Data standardization Physical parameters Big data
ISSN号0273-1177
DOI10.1016/j.asr.2019.10.035
英文摘要Observations of local features in the solar chromosphere began in 1992 at Huairou Solar Observing Station, while the full-disk chromosphere observations were carried out since 2000. In order to facilitate researchers to use full-disk chromosphere observation, algorithms have been developed to standardize the full-disk images. The algorithms include the determination of the center of the image and size standardization, geometric correction and intensity normalization. The solar limb of each image is determined from a histogram analysis of its intensity distribution. The center and radius are then calculated and the image is corrected for geometric distortions. Images are re-scaled to have a fixed radius of 500 pixels and centered within the 1024 x 1024 frame. Finally, large-scale variations in intensity, such as limb-darkening, are removed using a median filter. This paper provides a detailed description of these algorithms, and a summary of the properties of these chromospheric full-disk observations to be used for further scientific investigations. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
资助项目National Natural Science Foundation of China[U1531247] ; National Natural Science Foundation of China[2014FY120300] ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences[XDA15320302] ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences[XDA15320102] ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences[XDA15052200] ; 13th Five-year Informatization Plan of Chinese Academy of Sciences[XXH13505-04] ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences
WOS关键词FILAMENT RECOGNITION ; BRIGHTENINGS
WOS研究方向Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
出版者ELSEVIER SCI LTD
WOS记录号WOS:000514016200014
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; 13th Five-year Informatization Plan of Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Young Researcher Grant of National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences ; Key Laboratory of Solar Activity National Astronomical Observations, Chinese Academy of Sciences
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/54548]  
专题中国科学院国家天文台
通讯作者Suo, Liu
作者单位1.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100101, Peoples R China
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Suo, Liu. A full-disk image standardization of the chromosphere observation at Huairou Solar Observing Station[J]. ADVANCES IN SPACE RESEARCH,2020,65(3):1054-1061.
APA Suo, Liu.(2020).A full-disk image standardization of the chromosphere observation at Huairou Solar Observing Station.ADVANCES IN SPACE RESEARCH,65(3),1054-1061.
MLA Suo, Liu."A full-disk image standardization of the chromosphere observation at Huairou Solar Observing Station".ADVANCES IN SPACE RESEARCH 65.3(2020):1054-1061.
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