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Phase relationship between polar faculae and sunspot numbers
Deng LH(邓林华)1,2
2013-07
会议名称294th IAU Symposium - Solar and Astrophysical Dynamos and Magnetic Activity
会议日期2012-08-27
会议地点Beijing, China
关键词Sun: sunspot faculae methods: data analysis
卷号294
页码61-62
英文摘要Linear and nonlinear approaches are used to investigate the phase asynchrony between the polar faculae (PF) and sunspot numbers (SNs). It is found that, (1) PF show leads of 52 months relative to SNs on the average of the considered time interval; (2) the cross-wavelet transform analysis shows that they are asynchronous in both the low- and high-frequency components. These indicate that their phase relationship is not only time-dependent but also frequency-dependent.
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会议网址http://adsabs.harvard.edu/abs/2013IAUS..294...61D
会议录Proceedings of the International Astronomical Union, IAU Symposium - Solar and Astrophysical Dynamos and Magnetic Activity
学科主题天文学
语种英语
内容类型会议论文
源URL[http://ir.ynao.ac.cn/handle/114a53/4871]  
专题云南天文台_抚仙湖太阳观测站
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, 650011, Kunming, China
2.University of Chinese Academy of Sciences, 100049, Beijing, China
推荐引用方式
GB/T 7714
Deng LH. Phase relationship between polar faculae and sunspot numbers[C]. 见:294th IAU Symposium - Solar and Astrophysical Dynamos and Magnetic Activity. Beijing, China. 2012-08-27.http://adsabs.harvard.edu/abs/2013IAUS..294...61D.
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