Phase relation between activities of solar active prominences separately at low and high latitudes

	Phase relation between activities of solar active prominences separately at low and high latitudes
	Li KJ(李可军)1,2; Liu, XH 3; Xiong, SY 4; Liang HF(梁红飞)1,2 ; Zhan LS(占腊生)1,2 ; Zhao HJ(赵海娟)1,2
刊名	SOLAR PHYSICS
	2002-12
卷号	211 期号:1-2 页码:165-177
ISSN号	0038-0938
通讯作者	Li, KJ (reprint author), Yunnan Observ, Kunming 650011, Peoples R China.
产权排序	第一完成单位
英文摘要	In the present work, the phase relation between activities of solar active prominences respectively at low and high latitudes in the period 1957-1998 has been studied. We found that from the solar equator to the solar poles, the activity of the solar active prominences occurs earlier at higher latitudes, and that the cycle of the solar active prominences at high latitudes (larger than 50degrees) leads by 4 years both the sunspot cycle and the corresponding cycle of the solar active prominences at low latitudes (less than 40degrees).
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]	NORTH-SOUTH ASYMMETRY ; POLAR FACULAE ; SUNSPOT CYCLES ; FLARE INDEX ; SUN ; MIGRATION ; AREAS
收录类别	SCI
原文出处	http://link.springer.com/article/10.1023%2FA%3A1022480515250
语种	英语
WOS记录号	WOS:000181071700011
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/6048]
专题	云南天文台_太阳物理研究组
作者单位	1.Yunnan Observatory, Kunming, 650011, China 2.National Astronomical Observatories, Beijing, 100012, China 3.Department of Physics, Jiao-Zuo Educational College, Henan, China 4.Library, Yunnan University, Yunnan, China
推荐引用方式 GB/T 7714	Li KJ,Liu, XH,Xiong, SY,et al. Phase relation between activities of solar active prominences separately at low and high latitudes[J]. SOLAR PHYSICS,2002,211(1-2):165-177.
APA	Li KJ,Liu, XH,Xiong, SY,Liang HF,Zhan LS,&Zhao HJ.(2002).Phase relation between activities of solar active prominences separately at low and high latitudes.SOLAR PHYSICS,211(1-2),165-177.
MLA	Li KJ,et al."Phase relation between activities of solar active prominences separately at low and high latitudes".SOLAR PHYSICS 211.1-2(2002):165-177.