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An improved speckle filtering method for weaken signal

机译:一种改进的散斑滤波方法,用于减弱信号

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A New Filtering Method for Pulsar weaken signal In order to improve the denoising quality of the pulsar signal, a mode cell proportion shrinking denoising method is proposed based on empirical mode decomposing. Firstly, the pulsar signal is decomposed into a series intrinsic mode functions (IMFs), and the part between the two adjacent zero-crossing within IMF is defined as a mode cell. Then, treating mode cell as the basic unit of analysis and computing the optimal proportional shrinking factor of mode cell. Finally, the all mode cells within IMF are preceded by proportion shrinking, and the noise of IMF is suppressed. The experimental results show that, compared to SureShrink wavelet hard threshold method, BayesShrink wavelet hard threshold method, EMD mode cell threshold method, the proposed method can remove the pulsar signal noise more effectively, while preserving the useful detail information in the original signal better.
机译:脉冲星减弱信号的一种新滤波方法为了提高脉冲星信号的去噪质量,提出了一种基于经验模态分解的模元比例缩小去噪方法。首先,将脉冲星信号分解为一系列固有模式函数(IMF),并将IMF中两个相邻的零交叉之间的部分定义为模式单元。然后,将模态单元作为分析的基本单元,并计算出模态单元的最佳比例收缩因子。最后,在IMF中的所有模式单元之前都会进行比例缩小,从而抑制了IMF的噪声。实验结果表明,与SureShrink小波硬阈值方法,BayesShrink小波硬阈值方法,EMD模式单元阈值方法相比,该方法可以更有效地去除脉冲星信号噪声,同时更好地保留原始信号中的有用细节信息。

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