Periodicity of flare index revisited using the Hilbert-Huang transform method | |
Gao PX(高朋鑫)1,2; Liang, HF3; Zhu WW(朱玮文)1,2; Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. | |
发表期刊 | NEW ASTRONOMY |
2011-04 | |
卷号 | 16期号:3页码:147-151 |
DOI | 10.1016/j.newast.2010.09.006 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Methods: Data Analysis Sun: Activity Sun: Flares |
摘要 | Using the Hilbert-Huang Transform (HHT) method, we investigate the periodicity in the monthly mean flare indices from 1966 to 2007 (corresponding to almost four complete solar cycles), calculated by T. Atac and A. Ozguc. The results show as following. (1) The periods of 9.37 +/- 2.53, 11.8 +/- 0.172 and 23.6 +/- 0.316 years are found to be statistically significant in the flare index. The most eminent period is 9.37 +/- 2.53 years. (2) Other periods of 0.237 +/- 0.196 years (86.6 +/- 71.6 days), 0.525 +/- 0.0508 years (191 +/- 18.5 days), 1.05 +/- 0.478 years (383 +/- 174 days) and 2.37 +/- 0.395 years are below the 99% confidence level line, suggesting they are due to stochastic random noise. (C) 2010 Elsevier B.V. All rights reserved. |
项目资助者 | NSFC [10873032, 10921303, 40636031] ; National Key Research Science Foundation [2006CB806303] ; Chinese Academy of Sciences |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 1384-1076 |
URL | 查看原文 |
归档日期 | 2010-11-04 |
WOS记录号 | WOS:000285660400001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | EMPIRICAL MODE DECOMPOSITION ; TERM PERIODICITIES ; WAVELET ANALYSIS ; SUNSPOT NUMBERS ; SOLAR ; IDENTIFICATION ; SOLAR-CYCLE-23 ; FREQUENCY ; SPECTRUM |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6181 |
专题 | 太阳物理研究组 |
通讯作者 | Gao, PX (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China 2.Graduate University of Chinese Academy of Sciences, Beijing 100049, China 3.Department of Physics, Yunnan Normal University, Kunming 650093, 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 | Gao PX,Liang, HF,Zhu WW,et al. Periodicity of flare index revisited using the Hilbert-Huang transform method[J]. NEW ASTRONOMY,2011,16(3):147-151. |
APA | Gao PX,Liang, HF,Zhu WW,&Gao, PX .(2011).Periodicity of flare index revisited using the Hilbert-Huang transform method.NEW ASTRONOMY,16(3),147-151. |
MLA | Gao PX,et al."Periodicity of flare index revisited using the Hilbert-Huang transform method".NEW ASTRONOMY 16.3(2011):147-151. |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Periodicity of flare(336KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论