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The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere
Li KJ(李可军)2; Xu JC(徐景晨)2; Feng, W.1
刊名SCIENTIFIC REPORTS
2022-09-23
卷号12期号:1
ISSN号2045-2322
DOI10.1038/s41598-022-20094-x
产权排序第1完成单位
文献子类Article
英文摘要

The anomalous heating of the solar upper atmosphere is one of the eight key problems in modern astronomy. Moreover, the stratification of the solar atmosphere is an outstanding key-problem in solar physics. In this study, a hot butterfly-like pattern is found to run through the chromosphere to the corona lying right on top of the magnetic butterfly pattern of sunspots in the photosphere. We thus propose to introduce the term butterfly body to describe the butterfly diagram in the 3-dimensional atmosphere. Besides, we discuss the so-called polar brightening in different layers. It is found to be statistically in anti-phase with the solar cycle in the photosphere and the chromosphere, while in phase with the solar cycle in the corona. Accordingly, we describe the role and relationship of solar magnetic elements of different magnetic flux strengths to explain the statistical structuring of the solar atmosphere with the butterfly body over the solar cycle.

学科主题天文学 ; 太阳与太阳系 ; 太阳物理学
URL标识查看原文
出版地HEIDELBERGER PLATZ 3, BERLIN, 14197, GERMANY
资助项目National Natural Science Foundation of China[11973085] ; National Natural Science Foundation of China[11903077] ; National Natural Science Foundation of China[11803086] ; National Natural Science Foundation of China[12273087] ; Yunnan Fundamental Research Projects[202201AS070042] ; Yunnan Ten-Thousand Talents Plan (the Yunling-Scholar Project) ; project of the Group for Innovation of Yunnan Province[2022HC020] ; Chinese Academy of Sciences ; national project for large scale scientific facilities[2019YFA0405001]
WOS关键词ACTIVITY CYCLE ; GREEN CORONA ; CHROMOSPHERE ; MODEL ; SUN ; TEMPERATURE ; HOLE
WOS研究方向Science & Technology - Other Topics
语种英语
出版者NATURE PORTFOLIO
WOS记录号WOS:001012301900050
资助机构National Natural Science Foundation of China[11973085, 11903077, 11803086, 12273087] ; Yunnan Fundamental Research Projects[202201AS070042] ; Yunnan Ten-Thousand Talents Plan (the Yunling-Scholar Project) ; project of the Group for Innovation of Yunnan Province[2022HC020] ; Chinese Academy of Sciences ; national project for large scale scientific facilities[2019YFA0405001]
内容类型期刊论文
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/26134]  
专题云南天文台_抚仙湖太阳观测站
通讯作者Li KJ(李可军)
作者单位1.Kunming Univ Sci & Technol, Res Ctr Anal & Measurement, Kunming 650093, Peoples R China
2.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China;
推荐引用方式
GB/T 7714
Li KJ,Xu JC,Feng, W.. The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere[J]. SCIENTIFIC REPORTS,2022,12(1).
APA Li KJ,Xu JC,&Feng, W..(2022).The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere.SCIENTIFIC REPORTS,12(1).
MLA Li KJ,et al."The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere".SCIENTIFIC REPORTS 12.1(2022).
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