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The quiet chromosphere: differential rotation
Li KJ(李可军)1,2; Wan M(万苗)1,3; Feng, W4
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2023-02-22
卷号520期号:4页码:5928-5937
DOI10.1093/mnras/stad478
产权排序第1完成单位
收录类别SCI ; EI
关键词Sun: activity Sun: chromosphere Sun: rotation
摘要The solar chromosphere was daily observed in the Ca ii K line at the Mount Wilson Observatory from 1915 August to 1985 July. A digitized data base was created, which includes synoptical maps of the chromosphere in Ca ii intensity from Carrington rotations 827 to 1764. We have used the data base to investigate rotation and its differential of the chromosphere and the quiet chromosphere. The chromosphere is found to rotate faster than sunspots, but the difference in their rotation rates decreases with decreasing latitude, and near the equator they rotate at nearly the same speed. The chromosphere is obviously faster than the quiet photosphere and slightly faster than the quiet chromosphere at low latitudes, but slightly slower than the quiet chromosphere at middle latitudes. The differential degree of the rotation rate at low latitudes, ranging from largest to smallest in order, is found to be: sunspots, the chromosphere, the quiet photosphere, and the quiet chromosphere. The differential of the rotation rate is found to be different in different solar cycles for the chromosphere and the quiet chromosphere. Helioseismology observations suggest that these findings are plausible.
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] ; (Yunnan Ten-Thousand Talents Plan), Yunnan Fundamental Research Project[202201AS070042] ; (Yunnan Ten-Thousand Talents Plan), Yunnan Fundamental Research Project[2019YFA0405001] ; Specialized Research Fund for State Key Laboratories ; Chinese Academy of Sciences ; Yunling-Scholar Project (the Yunnan Ten-Thousand Talents Plan) ; Yunnan Fundamental Research Project[202201AS070042] ; National Project for Large-Scale Scientific Facilities[2019YFA0405001]
项目资助者National Natural Science Foundation of China[11973085, 11903077, 11803086] ; (Yunnan Ten-Thousand Talents Plan), Yunnan Fundamental Research Project[202201AS070042, 2019YFA0405001] ; Specialized Research Fund for State Key Laboratories ; Chinese Academy of Sciences ; Yunling-Scholar Project (the Yunnan Ten-Thousand Talents Plan) ; Yunnan Fundamental Research Project[202201AS070042] ; National Project for Large-Scale Scientific Facilities[2019YFA0405001]
语种英语
学科领域天文学 ; 太阳与太阳系 ; 太阳物理学
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
WOS记录号WOS:000943248300016
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR CORONAL ROTATION ; DEPENDENCE ; BEHAVIOR ; FLUX
EI入藏号20232014094175
EI主题词Rotation rate
EI分类号804.1 Organic Compounds - 931.1 Mechanics
引用统计
被引频次:3[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/114a53/25877
专题抚仙湖太阳观测和研究基地
通讯作者Li KJ(李可军); Feng, W
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China;
2.Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093, China;
3.University of Chinese Academy of Sciences, Beijing 100049, China;
4.State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100190, China
第一作者单位中国科学院云南天文台
通讯作者单位中国科学院云南天文台
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Li KJ,Wan M,Feng, W. The quiet chromosphere: differential rotation[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,520(4):5928-5937.
APA Li KJ,Wan M,&Feng, W.(2023).The quiet chromosphere: differential rotation.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,520(4),5928-5937.
MLA Li KJ,et al."The quiet chromosphere: differential rotation".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 520.4(2023):5928-5937.
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