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The quiet chromosphere: Phase relation with the solar cycle
Li KJ(李可军)1; Feng, W.2
发表期刊ADVANCES IN SPACE RESEARCH
2022-09-01
卷号70期号:5页码:1539-1546
DOI10.1016/j.asr.2022.06.003
产权排序第1完成单位
收录类别SCI
关键词Sun activity chromosphere atmosphere
摘要

The solar chromosphere was daily observed in the Ca II K line from 1915 August 10 to 1985 July 7, and correspondingly, 938 synoptic maps are measured. The valuable database is utilized to explore phase relationship of long-term evolution of the quiet chromosphere and sunspot numbers. Temporal change of the quiet chromosphere is found to be in anti-phase with the solar cycle on the whole, as the smallscale magnetic elements whose flux is in a span of (2.9 - 32.0) x 1018(Mx) do. The abnormal heating of the quiet chromosphere is accordingly suggested to be related mainly to the magnetic elements, and they may likely function in reducing chromosphere material loss. (c) 2022 COSPAR. Published by Elsevier B.V. All rights reserved.

资助项目National Natural Science Foundation of China[11973085] ; National Natural Science Foundation of China[11903077] ; 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[11703085] ; National Natural Science Foundation of China[12025008] ; Yunnan Ten-Thousand Talents Plan (the Yunling-Scholar Project), Yunnan Fundamental Research Project[202201AS070042] ; national project for large scale scientific facilities[2019YFA0405001] ; Chinese Academy of Sciences
项目资助者National Natural Science Foundation of China[11973085, 11903077] ; National Natural Science Foundation of China[11973085, 11903077, 11803086, 11703085, 12025008] ; Yunnan Ten-Thousand Talents Plan (the Yunling-Scholar Project), Yunnan Fundamental Research Project[202201AS070042] ; national project for large scale scientific facilities[2019YFA0405001] ; Chinese Academy of Sciences
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ELSEVIER SCI LTD
出版地THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
ISSN0273-1177
URL查看原文
WOS记录号WOS:000835505900008
WOS研究方向Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
WOS类目Engineering, Aerospace ; Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences
关键词[WOS]FEATURES ; POINTS ; CORONA ; SUN
引用统计
被引频次:2[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/114a53/25517
专题抚仙湖太阳观测和研究基地
通讯作者Li KJ(李可军)
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
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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GB/T 7714
Li KJ,Feng, W.. The quiet chromosphere: Phase relation with the solar cycle[J]. ADVANCES IN SPACE RESEARCH,2022,70(5):1539-1546.
APA Li KJ,&Feng, W..(2022).The quiet chromosphere: Phase relation with the solar cycle.ADVANCES IN SPACE RESEARCH,70(5),1539-1546.
MLA Li KJ,et al."The quiet chromosphere: Phase relation with the solar cycle".ADVANCES IN SPACE RESEARCH 70.5(2022):1539-1546.
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