High- and low-latitude solar activities: Who leads whom in time phase?

doi:10.1007/s11207-006-0027-3

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	High- and low-latitude solar activities: Who leads whom in time phase?
	Li KJ(李可军)1 ; Liang HF(梁红飞)1,2 ; Gao PX(高朋鑫)1,2 ; Su TW(苏同卫)1,2 ; Li, KJ (reprint author), CAS, Natl Astron Observ, Yunnan Observ, Kunming, Yunnan, Peoples R China.
发表期刊	SOLAR PHYSICS
	2006-06
卷号	236 期号:1 页码:185-197
DOI	10.1007/s11207-006-0027-3
产权排序	第1完成单位
收录类别	SCI
摘要	Using the data from observations of polar faculae by the National Astronomical Observatory of Japan from July 1951 to December 1998, we investigate whether there is a time lag between high-latitude solar activity and low-latitude solar activity. The cross-correlation analysis of the smoothed monthly numbers of the polar faculae with the smoothed monthly sunspot numbers shows that, high-latitude solar activity should lead low-latitude solar activity in time phase. The periodic characteristics of both of them also indicate that high-latitude activity evidently leads low-latitude activity.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0038-0938
URL	查看原文
归档日期	2006-09-01
WOS记录号	WOS:000239087300012
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	POLAR FACULAE ; WAVELET ANALYSIS ; MAGNETIC-FIELD ; SUNSPOT CYCLES ; SUN
引用统计	被引频次：9[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/6091
专题	太阳物理研究组
通讯作者	Li, KJ (reprint author), CAS, Natl Astron Observ, Yunnan Observ, Kunming, Yunnan, Peoples R China.
作者单位	1.National Astronomical Observatories/Yunnan Observatory, CAS, Yunnan, China 2.School of Graduate, CAS, Beijing, China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Li KJ,Liang HF,Gao PX,et al. High- and low-latitude solar activities: Who leads whom in time phase?[J]. SOLAR PHYSICS,2006,236(1):185-197.
APA	Li KJ,Liang HF,Gao PX,Su TW,&Li, KJ .(2006).High- and low-latitude solar activities: Who leads whom in time phase?.SOLAR PHYSICS,236(1),185-197.
MLA	Li KJ,et al."High- and low-latitude solar activities: Who leads whom in time phase?".SOLAR PHYSICS 236.1(2006):185-197.

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