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A method to evaluate the level of solar activity at the remainder of a progressing solar cycle
Li KJ(李可军)1,2; Qiu, J2; Xiang, FY3; Gao PX(高朋鑫)1; Su TW(苏同卫)1; Li, KJ (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Solar Phys Div, Kunming 650011, Peoples R China.
发表期刊NEW ASTRONOMY
2005-01
卷号10期号:3页码:209-218
DOI10.1016/j.newast.2004.10.003
产权排序第1完成单位
收录类别SCI
关键词Sun : Activity Sun : Active Cycle Sun : General
摘要A modified method is developed to evaluate the level of solar activity at the remainder of a progressing solar cycle based on a method previously proposed by [Li, K.J., Zhan, L.S., Wang, JX, et al., 2002a. A&A 392, 301]. The behavior of sunspot numbers at the remainder of cycle 23 is studied. A comparison of different methods that predict sunspot numbers of a whole cycle is also given in this paper. (C) 2004 Elsevier B.V. All rights reserved.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1384-1092
URL查看原文
归档日期2004-12-23
WOS记录号WOS:000226385600004
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]MAXIMUM AMPLITUDE ; SUNSPOT NUMBERS ; PREDICTION ; SOLAR-CYCLE-23
引用统计
被引频次:2[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/114a53/6080
专题太阳物理研究组
通讯作者Li, KJ (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Solar Phys Div, Kunming 650011, Peoples R China.
作者单位1.Solar Physics Division, National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China
2.Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA 92314, USA
3.Department of Physics, Xiangtan University, Hunan, China
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GB/T 7714
Li KJ,Qiu, J,Xiang, FY,et al. A method to evaluate the level of solar activity at the remainder of a progressing solar cycle[J]. NEW ASTRONOMY,2005,10(3):209-218.
APA Li KJ,Qiu, J,Xiang, FY,Gao PX,Su TW,&Li, KJ .(2005).A method to evaluate the level of solar activity at the remainder of a progressing solar cycle.NEW ASTRONOMY,10(3),209-218.
MLA Li KJ,et al."A method to evaluate the level of solar activity at the remainder of a progressing solar cycle".NEW ASTRONOMY 10.3(2005):209-218.
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