Study on the relation of the solar coronal rotation with magnetic field structures
文献类型：期刊论文
| 作者 | Xiang NB(向南彬)1,7 ; Zhao, X. H.1; Deng, L. H.6; Li, F. Y.1,3,4,5; Zheng, S.2
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| 刊名 | SCIENTIFIC REPORTS
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| 出版日期 | 2023-07-22 |
| 卷号 | 13期号:1 |
| ISSN号 | 2045-2322 |
| DOI | 10.1038/s41598-023-48447-0 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Article |
| 英文摘要 | Daily solar spectral irradiances (SSIs) at the spectral intervals 1-40, 116-264 and 950-1600 nm and four categories of solar small-scale magnetic elements (MFno, MFanti, MFtran and MFin) are used to study the temporal variation of coronal rotation and investigate the relation of the coronal rotation with magnetic field structures through continuous wavelet transform and Pearson correlation analysis. The results reveal the contributions of different magnetic structures to the temporal variation of the rotation for the coronal atmosphere during different phases of the solar cycle. During the solar maximum, the temporal variation of rotation for the coronal plasma atmosphere is mainly dominated by the small-scale magnetic elements of MFanti; whereas during the epochs of the relatively weak solar activity, it is controlled by the joint effect of the small-scale magnetic elements of both MFanti and MFin. The weaker the solar activity, the stronger the effect of MFin would be. Furthermore, this study presents an explanation for the inconsistent results for the coronal rotation issue among the previous studies, and also reveals the reason why the coronal atmosphere rotates faster than the lower photosphere. |
| 学科主题 | 天文学 |
| URL标识 | 查看原文 |
| 出版地 | HEIDELBERGER PLATZ 3, BERLIN, 14197, GERMANY |
| WOS关键词 | DIFFERENTIAL ROTATION ; PERIODICITIES ; IRRADIANCE ; IMAGES |
| 资助项目 | National Natural Science Foundation of China[12373059]; National Natural Science Foundation of China[12003068]; Strategic Priority Research Program of Chinese Academy of Sciences[XDB 41000000]; Yunnan Revitalization Talent Support Program Young Talent Project; CAS 'Light in Western China' Program, Yunnan Fundamental Research Projects[202301AV070007]; Specialized Research Fund for State Key Laboratories; Chinese Academy of Sciences |
| WOS研究方向 | Science & Technology - Other Topics |
| 语种 | 英语 |
| 出版者 | NATURE PORTFOLIO |
| WOS记录号 | WOS:001120258800106 |
| 资助机构 | National Natural Science Foundation of China[12373059, 12003068] ; Strategic Priority Research Program of Chinese Academy of Sciences[XDB 41000000] ; Yunnan Revitalization Talent Support Program Young Talent Project ; CAS 'Light in Western China' Program, Yunnan Fundamental Research Projects[202301AV070007] ; Specialized Research Fund for State Key Laboratories ; Chinese Academy of Sciences |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/26431]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 |
| 作者单位 | 1.State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China; 2.College of Science, China Three Gorges University, Yichang, China 3.The Key Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, China; 4.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University)-Ministry of Education, Nanjing, China; 5.Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, China; 6.School of Mathematics and Computer Science, Yunnan Minzu University, Kunming, China; 7.Yunnan Observatories, Chinese Academy of Sciences, Kunming, China; |
| 推荐引用方式 GB/T 7714 | Xiang NB,Zhao, X. H.,Deng, L. H.,et al. Study on the relation of the solar coronal rotation with magnetic field structures[J]. SCIENTIFIC REPORTS,2023,13(1). |
| APA | 向南彬,Zhao, X. H.,Deng, L. H.,Li, F. Y.,&Zheng, S..(2023).Study on the relation of the solar coronal rotation with magnetic field structures.SCIENTIFIC REPORTS,13(1). |
| MLA | 向南彬,et al."Study on the relation of the solar coronal rotation with magnetic field structures".SCIENTIFIC REPORTS 13.1(2023). |
入库方式： OAI收割
来源：云南天文台
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