Activity cycle of solar filaments
文献类型:期刊论文
作者 | Li KJ(李可军)1![]() ![]() ![]() ![]() ![]() ![]() |
刊名 | JOURNAL OF ASTROPHYSICS AND ASTRONOMY
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出版日期 | 2007-06 |
卷号 | 28期号:2-3页码:147-156 |
关键词 | sun activity-filaments-active cycle |
ISSN号 | 0250-6335 |
产权排序 | 第一完成单位 |
通讯作者 | Li, KJ (reprint author), CAS, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China. |
英文摘要 | Long-term variation in the distribution of the solar filaments observed at the Observatorie de Paris, Section de Meudon from March 1919 to December 1989 is presented to compare with sunspot cycle and to study the periodicity in the filament activity, namely the periods of the coronal activity with the Morlet wavelet used. It is inferred that the activity cycle of solar filaments should have them same cycle length as sunspot cycle, but the cycle behavior of solar filaments is globally similar in profile with, but different in detail from, that of sunspot cycles. The amplitude of solar magnetic activity should not keep in phase with the complexity of solar magnetic activity. The possible periods in the filament activity are about 10.44 and 19.20 years. The wavelet local power spectrum of the period 10.44 years is statistically significant during the whole consideration time. The wavelet local power spectrum of the period 19.20 years is under the 95% confidence spectrum during the whole consideration time, but over the mean red-noise spectrum of alpha = 0.72 before approximate Carrington rotation number 1500, and after that the filament activity does not statistically show the period. Wavelet reconstruction indicates that the early data of the filament archive (in and before cycle 16) are more noiseful than the later (in and after cycle 17). |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | WAVELET ANALYSIS ; GREEN CORONA ; PROMINENCES ; PERIODICITIES ; OSCILLATIONS ; PARAMETERS ; INDEXES |
收录类别 | SCI |
原文出处 | http://link.springer.com/article/10.1007%2Fs12036-007-0012-8 |
语种 | 英语 |
WOS记录号 | WOS:000250388800006 |
公开日期 | 2016-05-03 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6106] ![]() |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming, 650 011, China 2.School of Graduate, CAS, Beijing, 100 863, China |
推荐引用方式 GB/T 7714 | Li KJ,Li QX,Gao PX,et al. Activity cycle of solar filaments[J]. JOURNAL OF ASTROPHYSICS AND ASTRONOMY,2007,28(2-3):147-156. |
APA | Li KJ,Li QX,Gao PX,Mu J,Chen HD,&Su TW.(2007).Activity cycle of solar filaments.JOURNAL OF ASTROPHYSICS AND ASTRONOMY,28(2-3),147-156. |
MLA | Li KJ,et al."Activity cycle of solar filaments".JOURNAL OF ASTROPHYSICS AND ASTRONOMY 28.2-3(2007):147-156. |
入库方式: OAI收割
来源:云南天文台
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