Relative phase analyses of long-term hemispheric solar flare activity | |
Li KJ(李可军)1,2; Gao PX(高朋鑫)1,3; Zhan, LS4; Shi XJ(石祥军)1,3; Zhu WW(朱玮文)1,3; Li, KJ (reprint author), CAS, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. | |
发表期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
2010 | |
卷号 | 401期号:1页码:342-346 |
DOI | 10.1111/j.1365-2966.2009.15639.x |
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 | Wavelet transform methods, including the continuous wavelet transform, cross-wavelet transform and wavelet coherence, have been proposed to investigate the phase synchrony of the monthly mean flare indices in the time interval 1966 January-2007 December in the solar northern and southern hemispheres, respectively. The Schwabe cycle is the only period of statistical significance, and its mean value is 10.7 yr for the monthly mean flare indices in the northern hemisphere but slightly smaller, 10.1 yr, in the southern hemisphere - this should lead to phase asynchrony between the two. Both the cross-wavelet transform and wavelet coherence analyses show asynchronous behaviour with strong phase mixing in the high-frequency components of hemispheric flare activity, and strong synchronous behaviour with coherent phase angles in the low-frequency components, corresponding to the period-scales around the Schwabe cycle. The northern flare activity should lead the southern for the low-frequency components. |
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 | 0035-8711 |
URL | 查看原文 |
归档日期 | 2010-01-05 |
WOS记录号 | WOS:000272867100045 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | WAVELET ANALYSIS ; SUNSPOT ACTIVITY ; SYNCHRONIZATION ; COHERENCE |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6169 |
专题 | 太阳物理研究组 |
通讯作者 | Li, KJ (reprint author), CAS, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China 3.School of Graduate, CAS, Beijing, China 4.Jingdezhen Ceramic Institute, Jingdezhen 333001, Jiangxi, 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 | Li KJ,Gao PX,Zhan, LS,et al. Relative phase analyses of long-term hemispheric solar flare activity[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2010,401(1):342-346. |
APA | Li KJ,Gao PX,Zhan, LS,Shi XJ,Zhu WW,&Li, KJ .(2010).Relative phase analyses of long-term hemispheric solar flare activity.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,401(1),342-346. |
MLA | Li KJ,et al."Relative phase analyses of long-term hemispheric solar flare activity".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 401.1(2010):342-346. |
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