A first arrival detection method for low SNR microseismic signal

2018 ◽  
Vol 66 (5) ◽  
pp. 945-957 ◽  
Author(s):  
Ruiqing Hu ◽  
Yanchun Wang
Author(s):  
K. Manoj Kumar ◽  
P. J. Sijomon ◽  
K. Shamju Joseph ◽  
D. M. Premod ◽  
V. S. Shenoi ◽  
...  

2014 ◽  
Vol 596 ◽  
pp. 433-436 ◽  
Author(s):  
Yao Qi Wang ◽  
Xiao Peng Wang ◽  
Lv Cheng Wang

A new method of pitch detection based on morphological filtering is proposed. Noisy speech signal is filtered by morphological filtering to remove the noise and highlight pitch, and then HHT is employed to get Hilbert-Huang spectrum and to calculate instantaneous energy and its derivative. The moment of glottal opening and closing can be accurately located through tracking mutation of instantaneous energy, so that variation of pitch period can be accurately tracked. Compared with other traditional method of pitch detection, this method not only truly describes non-stationary and non-linear characteristics of speech signal, but also it is an adaptive process for the analysis of the speech signal. The experiments showed that the method has strong anti-noise and can accurately detect the pitch of speech in low SNR.


2019 ◽  
Vol 8 (8) ◽  
pp. 363-368
Author(s):  
Congshuang Xie ◽  
Junjie Li ◽  
Qin Chen ◽  
Zihao Zhao ◽  
Chunyi Song ◽  
...  

2014 ◽  
Vol 1049-1050 ◽  
pp. 1167-1170
Author(s):  
Jin Li ◽  
Kun Shen

Aiming at traditional methods cannot get good performance in noisy environments, an improved method for pitch detection was proposed. In this method, noisy speech was enhanced by using wiener filtering at first, and then analyzing linear prediction residual and power spectrum reprocessing, the feature of weighted residual power spectrum reprocessing was extracted to detect speech pitch period. Experimental results indicate that the proposed pitch detection method has higher reliability with lower computational complexity. It can detect pitch more accurately in low SNR environments and has better robustness.


2011 ◽  
Vol 28 (2) ◽  
pp. 144-149 ◽  
Author(s):  
Jia Zhu ◽  
Zhangqin Zhu ◽  
Zhongfu Ye

AbstractAnovel profile detection method is proposed for astronomical fiber spectrum data with low signalto-noise ratio. This approach can be applied to the pretreatment for 2-D astronomical spectrum data before the extraction of spectra. The Wigner bispectrum, a classical higher-order spectrum analysis method, is introduced and applied to deal with the spectrumsignal in this article.After analyzing the Wigner higher-order spectra distribution of the target profile signal, the combination of the Wigner bispectrum algorithm and the fast Fourier transform algorithm is used to weaken the effect of the noise to obtain more accurate information. Both the reconstruction method of the Wigner bispectrum and inverse fast Fourier transform are used to acquire the detection signal. At the end of this paper, experiments with both simulated and observed data based on the Large Sky Area Multi-Object Fiber Spectroscopy Telescope project are presented to demonstrate the effectiveness of the proposed method.


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