NAOC Open IR  > 星系宇宙学研究部
Phase relation between activities of solar active prominences separately at low and high latitudes
Li, KJ; Liu, XH; Xiong, SY; Liang, HF; Zhan, LS; Zhao, HJ
2002-12-01
发表期刊SOLAR PHYSICS
卷号211期号:1-2页码:165-177
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).
收录类别SCI
语种英语
WOS记录号WOS:000181071700011
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文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8549
专题星系宇宙学研究部
作者单位1.Yunnan Observ, Kunming 650011, Peoples R China
2.Natl Astron Observ, Beijing 100012, Peoples R China
3.Jiao Zuo Educ Coll, Dept Phys, Henan, Peoples R China
4.Yunnan Univ, Lib, Yunnan, Peoples R China
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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.
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