中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Long-term variations of the coronal rotation and solar activity

文献类型:期刊论文

作者Li KJ(李可军)1,2; Shi XJ(石祥军)1,3; Feng, W4; Xie, JL1,3; Gao PX(高朋鑫)1; Zhan, LS5; Liang, HF6
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2012-07
卷号423期号:4页码:3584-3588
ISSN号0035-8711
关键词methods: data analysis Sun: activity Sun: corona Sun: rotation
通讯作者Li, KJ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
产权排序第一完成单位
英文摘要Recently, Chandra and Vats have obtained the yearly period length of the solar coronal rotation cycle by analysing the daily adjusted solar radio flux at the 10.7-cm wavelength for the years 19472009. In this paper, we use the time series (series I) of the yearly period length to investigate the long-term variation of the rotation of radio emission corona, and we find a weak decreasing trend in the time series. We use the empirical mode decomposition to decompose both the yearly mean value (series II) of the solar radio flux at the 10.7-cm wavelength and series I into different periodical components. There is a secular trend for each of the two series, and we find a negative correlation in the two trends. The decomposed 11-yr-cycle components of the two series show different and complicated periods and there is a phase relation between them. We investigate the cycle-related variation of the coronal rotation length, and we find that there is no Schwable cycle of statistical significance for the long-term variation of the rotation cycle length.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]X-RAY CORONA ; DIFFERENTIAL ROTATION ; BRIGHT POINTS ; TIME-SERIES ; FE-XIV ; CYCLE ; PERIODICITIES ; RATES
收录类别SCI
原文出处http://mnras.oxfordjournals.org/content/423/4/3584
语种英语
WOS记录号WOS:000306003600044
源URL[http://ir.ynao.ac.cn/handle/114a53/6199]  
专题云南天文台_太阳物理研究组
作者单位1.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China
3.Graduate School of the Chinese Academy of Sciences, Beijing, China
4.Research Center of Analysis and Measurement, Kunming University of Science and Technology, Kunming 650093, China
5.Jingdezhen Ceramic Institute, Jingdezhen 333001, Jiangxi, China
6.Department of Physics, Yunnan Normal University, Kunming 650093, China
推荐引用方式
GB/T 7714
Li KJ,Shi XJ,Feng, W,et al. Long-term variations of the coronal rotation and solar activity[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2012,423(4):3584-3588.
APA Li KJ.,Shi XJ.,Feng, W.,Xie, JL.,Gao PX.,...&Liang, HF.(2012).Long-term variations of the coronal rotation and solar activity.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,423(4),3584-3588.
MLA Li KJ,et al."Long-term variations of the coronal rotation and solar activity".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 423.4(2012):3584-3588.

入库方式: OAI收割

来源:云南天文台

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