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1.
Using the Lomb-Scargle periodogram we analyzed two sunspot series: the one over the past 11000 years at the 10-year interval based upon the survey data of 14C concentration in tree-rings, recon- structed by Solanki et al.; and the sunspot number over the past 7000 years, derived from geomagnetic variations by Usoskin et al. We found the periods and quasi-periods in solar activity, such as about 225, 352, 441, 522 and 561 a, and near 1000 and 2000 a. An approach of wavelet transform was applied to check the two sunspot time series, with emphasis on investigating time-varying characteristics in the long-term fluctuations of solar activity. The results show that the lengths and amplitudes of the periods have changed with time, and large variations have taken place during some periods.  相似文献   

2.
介绍自2007年下半年到现在的非常低的太阳活动状况:无黑子活动天数为16太阳活动周以来最多,不排除24周的无黑子天数是现代黑子周内最多的可能;高纬度(35°)黑子的纬度为12周最低;从2003年11月~2008年9月,较高纬度(20°)每月没有黑子或只有1个黑子,共计持续了58个月,也为12周以来第一次观测到;太阳风速度、太阳风压、10cm电磁波辐射、太阳极区磁场、太阳总光度辐射等参量都为有观测资料以来的最低.对于这种极低太阳活动的现象,介绍了从当前的日震观测给予的解释、也从Gleissberg周期的长尺度、超长太阳活动周期尺度给予了解释.依据目前的观测,我们确定24黑子活动周于2008年11月开始.综合多种经典太阳活动预报方法给出的对24周太阳活动水平的预报,以及美国国家航空航天局和美国国家海洋大气局对24周的未来发展趋势的预报,认为24周太阳活动水平估计比23周将要弱30%左右.异常的24太阳活动周为太阳物理和日地关系物理研究带来机遇.  相似文献   

3.
  总被引:4,自引:0,他引:4  
The variation of the near 5-month period of sunspot numbers is discussed on the basis of the wavelet transform of the daily sunspot number series in the 14th—22nd solar cycles. The result shows that the period exists in every cycle and its energy density (amplitude) is comparatively large in the peak section of the cycle. In the distinct cycle, the length and intensity of the period is different, which means that the period varies with time. The near 25-day period is also analyzed and it is found to be timevariable and even not very stable in the peak section of the cycle. The variations of the two periods show that the near 5-month period should not be simply regarded as the multiples of the near 25-day period.  相似文献   

4.
利用小波技术以沈阳昭陵古油松为样本建立的古油松年轮宽度年表与太阳黑于活动为研究对象,分析了沈阳的古油松生长与太阳活动的关系。油松在5~8年、10-12年和20-30年周期段对太阳活动表现出积极的响应,呈现5.8、11.5和27.2年的强周期震荡,响应信号在太阳活动的主周期11.1年左右表现最强。太阳黑子活动对油松年轮宽度年表总的影响是负效应,是多种抑、促效应的复合。  相似文献   

5.
A range of analysis approaches,namely continuous wavelet,cross wavelet,and wavelet coherence analyses,are employed to clarify the phase relationship between the smoothed monthly mean sunspot number and solar 10.7 cm flux(F10.7).Analysis shows that there is a region of high spectral power sitting across the Schwabe cycle belt,where the two time series are in phase.However,analysis of the cross-wavelet transform and wavelet coherence unveils asynchronous behavior featured with phase mixing in the high-frequency components of sunspot activity and solar F10.7,which may explain the different activity properties of the photosphere and corona on a short time scale.  相似文献   

6.
  总被引:1,自引:1,他引:0  
Sunspot number, sunspot area and sunspot unit area are usually used to show sunspot activity. In this paper,periodicity of sunspot activity of modern solar cycles has been investigated through analyzing the monthly mean values of the three indices in the time interval of May 1874 to May 2004 by use of the wavelet transform. Their global power spectra and local power spectra are given while the statistical tests of these spectra are taken into account. The main results are (1) the local wavelet power spectrum of the sunspot number seems like that of the sunspot area, indicating that the periodicity of the both indices is similar. The local power spectrum of the sunspot unit area resembles the local power spectra of the previous two indices, but looks more complicated. (2) the possible periods in sunspot activity are about 10.6 (or 10.9 years for the sunspot unit area), 31,and 42 years, and the period of about 10.6 years is statistically significant in the considered time. For the periods of about 31 and 42 years, their power peaks are under the 95% confidence level line but over the mean red-noise spectral line, and for the other rest periods, their power peaks are even under the mean red-noise spectral line, which are statistically insignificant. (3) the local power of the three periods is higher in the late stage than in the early stage of the considered time. (4) the period characteristics of the three indices, shown in the global power spectra and the local power spectra, are similar but there is difference in detail.  相似文献   

7.
基于小波变换的含间隙太阳能帆板动力学试验分析   总被引:1,自引:0,他引:1  
为了有效地提取含间隙可展结构振动信号中所包含的动力学特征量,在分析传统Fourier方法局限性的基础上,引入基于小波变换的数据处理和分析方法。对含间隙太阳能帆板在收拢和展开状态下施加单脉冲的激励,测试标志点的加速度信号,系统地分析了间隙对动力学性能的影响。结果表明:小波变换能够较好地表征含间隙可展结构的时频特征信息,可以得到系统的频带以及各个频度衰减的速度和时间。实现了对航天可展结构动力学性能在时频域内的“精细”考察,将有助于提高航天器结构的分析与设计水平。  相似文献   

8.
为了进一步探讨太阳耀斑与太阳黑子参量的关系,本文采集了大规模的活动区黑子数据,统计其与耀斑发生的产率关系,应用得到的拟和公式对原始数据计算得到规范化后的数据集.在此基础上使用数据挖掘技术对黑子耀斑数据建立决策树模型和建立分类规则,具体描述了黑子数据和太阳耀斑之间的相关性.最后应用这两种技术对活动区未来48h是否爆发耀斑给出了预报,预报结果具有较高的准确率和较低的虚报率.  相似文献   

9.
根据南充地区多年灾害性天气资料(1951—1991年)与太阳黑子资料(1900-1991年),对南充地区主要灾害性天气与太阳活动的关系进行了初步探讨,发现南充地区的严重夏旱发生在太阳活动的上升时期,而严重伏旱、春旱、秋绵雨及洪涝大多出现在太阳活动的下降时期.  相似文献   

10.
采用交叉谱分析方法,通过年全球平均的大气臭氧总量和10.7cm大阳通量两时间序列的对比分析发现,大气臭氧的短期变化和大阳自转活动之间有着极为密切的相关关系:大气臭氧准27天周期变化和太阳10.7cm辐射通量之间存在约140°的位相差,落后时间为10.2天.//关键词  相似文献   

11.
    
A method to predict the amplitude and date of the maximum sunspot number is introduced. The regression analysis of the relationship between the variation rate of monthly sunspot numbers in the initial stage of solar cycles and both of the maximum and the time-length of ascending period of the cycle showed that they are closely correlative. In general, the maximum will be larger and the ascending period will be shorter when the rate is larger. The rate of sunspot numbers in the initial 2 years of the 23rd cycle is thus analyzed based on these grounds and the maximum of the cycle is predicted. For the smoothed monthly sunspot numbers, the maximum will be about 139.2±18.8 and the time-length of ascending period will be about 3.31±0.42 years, that is to say, the maximum will appear around the spring of the year 2000. For the mean monthly ones, the maximum will be near 170.1±22.9 and the time-length of ascending period will be about 3.42±0.46 years, that is to say, the appearing date of the maximum will be later.  相似文献   

12.
充分利用小波和现代谱分析的优点,提出一种新的谱分析方法——高斯小波-最大熵谱分析方法。介绍了该方法的分析步骤,并应用于减速机的故障诊断。该方法实现了在机械设备故障诊断中不同频带范围内零部件故障信息的分离和提取。  相似文献   

13.
14.
To study the temporally varying features of summer thermal contrast between the Asian continent and the adjacent ocean on decadal-centennial time scales and the links between thermal contrast and solar irradiance, we used a time series of the reconstructed Asian-Pacific oscillation index and solar irradiance over the past millennium. The results showed that thermal contrast in the Asian monsoon region has quasi-90-year, 10-13-year, and 3-7-year periods. On the centennial time scale, thermal contrast showed ...  相似文献   

15.
基于小波变换的火车车轮扁疤信号能量分析   总被引:1,自引:0,他引:1  
火车车轮扁疤是火车行车事故的重大隐患之一,了解扁疤信号的能量分布情况对正确检测车轮扁疤有重要的意义.针对车轮扁疤信号具有持续时间短、突变快等特点,提出了一种运用小波变换的多分辨率分析和小波能量谱对扁疤信号进行分析的方法,通过比较扁疤信号在不同尺度下的能量密度,找出能量与各频段之间的对应关系,得出了扁疤信号的能量主要集中在2500Hz以下的频带范围内,在实际的车轮扁疤检测算法中只需分析频带范围为2500Hz以下的扁疤信号即可,通过实验验证了该能量分析方法的有效性.  相似文献   

16.
  总被引:3,自引:0,他引:3  
The low signal to noise ratio (SNR) of functional MRI (fMRI) prefers more sensitive data analysis methods. Based on stationary wavelet transform and spectrum analysis, a new method with high detective sensitivity was developed for analyzing fMRI time series, which does not require any prior assumption of the characteristics of noises. In the proposed method, every component of fMRI time series in the different time-frequency scales of stationary wavelet transform was discerned by the spectrum analysis, then the components from noises were removed using the stationary wavelet transform, finally the components of real brain activation were detected by cross-correlation analysis. The results obtained from both simulated and in vivo visual experiments illustrated that the proposed method has much higher sensitivity than the traditional cross-correlation method.  相似文献   

17.
提出利用连续小波变换计算纱条波谱图的方法,并构造出适合纱条波谱图计算的小波函数。利用本文方法计算波谱图,其波道数可根据需要进行选择,并能得到相应的三维波谱图。  相似文献   

18.
二维非平稳信号的小波谱均衡分析方法   总被引:1,自引:0,他引:1  
小波变换对信号的分时分频的精细表达和多分辨率的全面把握,使我们能更深入地认识信号和噪声的特性,便于基于小波域进行更有效的高分辩率的处理工作;而谱均衡处理技术是提高信号纵向分辨率的有效方法.本文结合上述两种处理手段,提出了一种小波谱均衡方法:先将二维非平稳信号进行小波分频处理,得到不同尺度的信号;然后将各尺度上的信号分别进行谱均衡处理,再将经谱均衡处理的不同尺度信号进行重建,从而得到高分辨率信号.利用小波谱均衡进行实际信号处理,处理结果表明该方法的处理效果要好于常规的谱均衡方法,它既能提高二维非平稳信号的纵向分辨率,同时又能保持原信号的固有特征.  相似文献   

19.
阐述了日月食观测在研究太阳大气结构、太阳活动,寻找近日彗星和水内行星,检验广义相对论理论以及校正历史中年日次序诸多方面的价值.  相似文献   

20.
  总被引:1,自引:0,他引:1  
Using the observational data of total solar irradiance (TSI) from 1976 to 2006, the evolution of total solar irradiance and the rela-tionship between TSI and sunspot number (SSN) have been analyzed with the wavelet technique. The results of the continuous wavelet transform (CWT) indicate that the TSI has multi-scale evolutionary characteristics. In the low frequency band, the TSI and SSN show similar variation with a significant and steady oscillation period from 8 to 11.4 a. While in the high frequency band, only around the maximum time of solar cycles, both the TSI and SSN present a significant intermittent oscillation period from 2 to 6 months. The results of the cross wavelet transform indicate that there is significant in-phase resonance oscillation between the TSI and SSN in 8–11.4 a band, where the variation of the SSN is 2 months ahead of that of TSI. Those results confirm the SSN as the primary cause for TSI’s periodic variation in the time scale of 8–11.4 a. However for the 2–6 month band, significant resonance periodicity is observed only within the maximum time of solar cycle, but the phase relationship between the TSI and SSN is unsteady. Finally, a reliable TSI monthly series from 1878 to 1975 is reconstructed and tested.  相似文献   

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