太阳磁活动的增强子波分析与全球温度和英格兰中部温度记录的比较
Enhanced Wavelet Analysis of Solar Magnetic Activity with Comparison to Global Temperature and the Central England Temperature Record
摘要：
连续子波变换可以通过利用子波响应函数的反卷积来增强。校正后的影响锥，太阳磁记录的功率谱密度的derectified每年的太阳黑子数计算，揭示了一个频谱的奇次谐波的基本海尔周期，和集成的瞬时功率进行比较，重建全球温度的归一化散点图显示的正相关后，二十世纪之交。与英格兰中部温度记录的光谱比较表明，有些特征是共享的，而另一些则不是，散点图再次表明可能的相关性。
英文摘要：
The continuous wavelet transform may be enhanced by deconvolution with the wavelet response function. After correcting for the cone-of-influence, the power spectral density of the solar magnetic record as given by the derectified yearly sunspot number is calculated, revealing a spectrum of odd harmonics of the fundamental Hale cycle, and the integrated instant power is compared to a reconstruction of global temperature in a normalized scatter plot displaying a positive correlation after the turn of the twentieth century. Comparison of the spectrum with that obtained from the Central England Temperature record suggests that some features are shared while others are not, and the scatter plot again indicates a possible correlation.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
