Phase asynchrony between coronal index and sunspot numbers | |
Deng LH(邓林华)1,2; Qu ZQ(屈中权)1; Wang, KR3; Li, XB1; Deng, LH (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China. | |
发表期刊 | ADVANCES IN SPACE RESEARCH |
2012-11-15 | |
卷号 | 50期号:10页码:1425-1433 |
DOI | 10.1016/j.asr.2012.07.017 |
产权排序 | 第1完成单位 |
收录类别 | SCI ; EI |
关键词 | Sun: Corona - Sunspots Methods: Data Analysis |
摘要 | In this paper, the phase asynchrony between coronal index and sunspot numbers is investigated. It is found that, (1) the sunspot numbers begin one month earlier than coronal index, which should mathematically lead to phase asynchrony between them but with a slight effect; (2) the 11-year Schwabe cycle is the only one period with statistical significance for coronal index and sunspot numbers, and the difference between the length of the Schwabe cycle of them should also lead to phase asynchrony between them; (3) although coronal index and sunspot numbers are coherent in low-frequency components corresponding to the 11-year Schwabe cycle, they are asynchronous in phase in high-frequency components; (4) their different definitions and physical meanings may be a major rea ion why there is a phase asynchrony between them. (C) 2012 COSPAR. Published by Elsevier Ltd. All rights reserved. |
项目资助者 | National Natural Science Foundation of China (NSFC) [11003041] ; Yunnan Science Foundation of China [2009CD120] ; Chinese Academy of Sciences |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
文章类型 | Article |
ISSN | 0273-1177 |
URL | 查看原文 |
归档日期 | 2012-11-05 |
WOS记录号 | WOS:000310099500010 |
WOS研究方向 | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
WOS类目 | Astronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences |
关键词[WOS] | SOLAR-ACTIVITY RECONSTRUCTION ; WAVELET ANALYSIS ; POLAR FACULAE ; TIME-SERIES ; LINE INTENSITY ; GREEN CORONA ; VARIABILITY ; ASYMMETRY ; CYCLE ; SUN |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4683 |
专题 | 抚仙湖太阳观测和研究基地 |
通讯作者 | Deng, LH (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, PR China 2.Graduate School of the Chinese Academy of Sciences, ShijingShan Block, 100049 Beijing, PR China 3.North China Electric Power University, Beijing 102206, PR 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 | Deng LH,Qu ZQ,Wang, KR,et al. Phase asynchrony between coronal index and sunspot numbers[J]. ADVANCES IN SPACE RESEARCH,2012,50(10):1425-1433. |
APA | Deng LH,Qu ZQ,Wang, KR,Li, XB,&Deng, LH .(2012).Phase asynchrony between coronal index and sunspot numbers.ADVANCES IN SPACE RESEARCH,50(10),1425-1433. |
MLA | Deng LH,et al."Phase asynchrony between coronal index and sunspot numbers".ADVANCES IN SPACE RESEARCH 50.10(2012):1425-1433. |
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Phase asynchrony bet(1137KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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