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Height-dependent differential rotation of the solar atmosphere detected by CHASE
Rao, Shihao1,2; Li, Chuan1,2,3; Ding, Mingde1,2; Hong, Jie1,2; Chen, Feng1,2; Fang, Cheng1,2; Qiu, Ye1,2,3; Li, Zhen1,2; Chen, Pengfei1,2; Li KJ(李可军)4; Hao, Qi1,2; Guo, Yang1,2; Cheng, Xin1,2; Dai, Yu1,2; Peng, Zhixin1,2; You, Wei5; Yuan, Yuan5
发表期刊NATURE ASTRONOMY
2024
DOI10.1038/s41550-024-02299-4
产权排序第4完成单位
收录类别SCI
摘要Rotation is an intrinsic property of stars and provides essential constraints on their structure, formation, evolution and interaction with the interplanetary environment. The Sun provides a unique opportunity to explore stellar rotation from the interior to its atmosphere in great detail. We know that the Sun rotates faster at the equator than at the poles, but how this differential rotation behaves at different atmospheric layers within it is not yet clear. Here we extract the rotation curves of different layers of the solar photosphere and chromosphere by using whole-disk Dopplergrams obtained by the Chinese H alpha Solar Explorer (CHASE) for the wavebands Si i (6,560.58 & Aring;), H alpha (6,562.81 & Aring;) and Fe i (6,569.21 & Aring;) with a spectral resolution of 0.024 & Aring;. We find that the Sun rotates progressively faster from the photosphere to the chromosphere. For example, at the equator, it increases from 2.81 +/- 0.02 mu rad s-1 at the bottom of the photosphere to 3.08 +/- 0.05 mu rad s-1 in the chromosphere. The ubiquitous small-scale magnetic fields and the height-dependent degree of their frozen-in effect with the solar atmosphere are plausible causes of the height-dependent rotation rate. The results have important implications for understanding solar subsurface processes and solar atmospheric dynamics. Spectroscopic observations of the CHASE mission reveal the differential rotation of the solar atmosphere, finding quantitively that the Sun rotates progressively faster from the bottom of the photosphere to the chromosphere.
资助项目National Science Foundation of China | National Natural Science Foundation of China-Yunnan Joint Fund (NSFC-Yunnan Joint Fund)[050101]; China National Space Administration[12333009]; National Natural Science Foundation of China (NSFC)[12173019]; NSFC; Programme for Innovative Talents and Entrepreneurs of Jiangsu Province[2022YFF0503004]; National Key R&D Program of China[202201AS070042]; Basic Research Foundation of Yunnan Province
项目资助者National Science Foundation of China | National Natural Science Foundation of China-Yunnan Joint Fund (NSFC-Yunnan Joint Fund)[050101] ; China National Space Administration[12333009] ; National Natural Science Foundation of China (NSFC)[12173019] ; NSFC ; Programme for Innovative Talents and Entrepreneurs of Jiangsu Province[2022YFF0503004] ; National Key R&D Program of China[202201AS070042] ; Basic Research Foundation of Yunnan Province
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article; Early Access
出版者NATURE PORTFOLIO
出版地HEIDELBERGER PLATZ 3, BERLIN, 14197, GERMANY
ISSN2397-3366
URL查看原文
WOS记录号WOS:001247083500002
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]MOUNT-WILSON ; INTERNAL-ROTATION ; VELOCITY ; ORIGIN
引用统计
被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27398
专题抚仙湖太阳观测和研究基地
作者单位1.School of Astronomy and Space Science, Nanjing University, Nanjing, China;
2.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, China;
3.Institute of Science and Technology for Deep Space Exploration, Suzhou Campus, Nanjing University, Suzhou, China;
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming, China;
5.Shanghai Institute of Satellite Engineering, Shanghai, China
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GB/T 7714
Rao, Shihao,Li, Chuan,Ding, Mingde,et al. Height-dependent differential rotation of the solar atmosphere detected by CHASE[J]. NATURE ASTRONOMY,2024.
APA Rao, Shihao.,Li, Chuan.,Ding, Mingde.,Hong, Jie.,Chen, Feng.,...&Yuan, Yuan.(2024).Height-dependent differential rotation of the solar atmosphere detected by CHASE.NATURE ASTRONOMY.
MLA Rao, Shihao,et al."Height-dependent differential rotation of the solar atmosphere detected by CHASE".NATURE ASTRONOMY (2024).
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