中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The periodicity of high-latitude solar activity

文献类型:期刊论文

作者Li KJ(李可军)1; Li QX(李启秀)1,2; Su TW(苏同卫)1,2; Gao PX(高朋鑫)1,2
刊名SOLAR PHYSICS
出版日期2006-12
卷号239期号:1-2页码:493-501
ISSN号0038-0938
产权排序第一完成单位
通讯作者Li, KJ (reprint author), CAS, Natl Astron Observ, Yunnan Observ, Yunnan, Peoples R China.
英文摘要The periodicity of high-latitude solar activity has been studied with the use of the Carte Synoptique solar filaments archive. The Morlet wavelet is utilized to analyze the periodicity of the number of solar filaments at latitudes over 50 degrees during Carrington solar rotations 876-1823. For solar filaments at latitudes over 50 degrees, the most eminent periods are about 10.23 and 10.90 years, which correspond to the Schwabe period of high-latitude solar activity, and the these periods make-up a highly significant proportion of the time span considered. The periods of 1.3 and 1.7 years and the quasi-biennial 2-3-year oscillation often mentioned in the literature are not found to be a feature of every solar cycle but seem to appear only from time to time.
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]COSMIC-RAY INTENSITY ; WAVELET ANALYSIS ; POLAR FACULAE ; MAGNETIC-FIELDS ; CYCLES ; PARAMETERS ; WIND ; OSCILLATIONS ; EVOLUTION ; FREQUENCY
收录类别SCI
原文出处http://link.springer.com/article/10.1007%2Fs11207-006-0008-6
语种英语
WOS记录号WOS:000242706500023
公开日期2016-05-03
源URL[http://ir.ynao.ac.cn/handle/114a53/6083]  
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, Yunnan, China
2.School of Graduate, CAS, Beijing, China
推荐引用方式
GB/T 7714
Li KJ,Li QX,Su TW,et al. The periodicity of high-latitude solar activity[J]. SOLAR PHYSICS,2006,239(1-2):493-501.
APA Li KJ,Li QX,Su TW,&Gao PX.(2006).The periodicity of high-latitude solar activity.SOLAR PHYSICS,239(1-2),493-501.
MLA Li KJ,et al."The periodicity of high-latitude solar activity".SOLAR PHYSICS 239.1-2(2006):493-501.

入库方式: OAI收割

来源:云南天文台

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