Resolution Enhancement of SOHO/MDI Magnetograms | |
Tan Y(覃瑛)1,2,3; Ji KF(季凯帆)1,3,4; Liu H(刘辉)1,3,4; Yu XG(余晓光)1,3,4 | |
发表期刊 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2024-06-01 | |
卷号 | 24期号:6 |
DOI | 10.1088/1674-4527/ad3b3b |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | magnetic fields techniques: image processing virtual observatory tools Sun: magnetic fields |
摘要 | Research on the solar magnetic field and its effects on solar dynamo mechanisms and space weather events has benefited from the continual improvements in instrument resolution and measurement frequency. The augmentation and assimilation of historical observational data timelines also play a significant role in understanding the patterns of solar magnetic field variation. Within the realm of astronomical data processing, super-resolution (SR) reconstruction refers to the process of using a substantial corpus of training data to learn the nonlinear mapping between low-resolution (LR) and high-resolution (HR) images, thereby achieving higher-resolution astronomical images. This paper is an application study in high-dimensional nonlinear regression. Deep learning models were employed to perform SR modeling on SOHO/MDI magnetograms and SDO/HMI magnetograms, thus reliably achieving resolution enhancement of full-disk SOHO/MDI magnetograms and enhancing the image resolution to obtain more detailed information. For this study, a data set comprising 9717 pairs of data from 2010 April to 2011 February was used as the training set, 1332 pairs from 2011 March were used as the validation set and 1034 pairs from 2011 April were used as the test set. After data preprocessing, we randomly cropped 128 x 128 sub-images as the LR cases from the full-disk MDI magnetograms, and the corresponding 512 x 512 sub-images as HR ones from the HMI full-disk magnetograms for model training. The tests conducted have shown that the study successfully produced reliable 4x SR reconstruction of full-disk MDI magnetograms. The MESR model's results (0.911) were highly correlated with the target HMI magnetographs as indicated by the correlation coefficient values. Furthermore, the method achieved the best PSNR, SSIM, MAE and RMSE values, indicating that the MESR model can effectively reconstruct magnetograms. |
资助项目 | National Natural Science Foundation of China (NSFC)[12003068]; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] |
项目资助者 | National Natural Science Foundation of China (NSFC)[12003068] ; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009] |
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 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
出版地 | 20A DATUN RD, CHAOYANG, BEIJING, 100101, PEOPLES R CHINA |
ISSN | 1674-4527 |
URL | 查看原文 |
WOS记录号 | WOS:001249981300001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | DEEP ; SUPERRESOLUTION ; MISSION |
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/114a53/27412 |
专题 | 抚仙湖太阳观测和研究基地 南方基地 中国科学院天体结构与演化重点实验室 天文技术实验室 |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China; [email protected], [email protected]; 2.University of Chinese Academy of Sciences, Beijing 100049, China; 3.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, China; 4.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Tan Y,Ji KF,Liu H,et al. Resolution Enhancement of SOHO/MDI Magnetograms[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2024,24(6). |
APA | 覃瑛,季凯帆,刘辉,&余晓光.(2024).Resolution Enhancement of SOHO/MDI Magnetograms.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,24(6). |
MLA | 覃瑛,et al."Resolution Enhancement of SOHO/MDI Magnetograms".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 24.6(2024). |
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