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Estimating Near-Surface Q Value based on the centroid frequency shift and integral area of the logarithmic spectral

机译:基于对数光谱的质心频移和积分面积估计近表面Q值

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Estimation of quality factor Q plays a fundamental role to enhance seismic resolution via absorption compensation of the near surface layer. Two methods have been widely used to estimate the Q value, the spectral ratio method (SRM) and the centroid frequency shift method (CFS). However, the SRM is too sensitive to noise and performance poorly under the low signal-to-noise (SNR) data. When the spectrum of the wavelet deviates from the Gaussian-like, the Q value estimated by the CFS will produce deviation. In this paper, we present a new method for Q estimation. Through establishment the relationship between reference wavelet logarithmic spectrum area and centroid frequency shift of logarithmic spectrum (LSCFS) to inverse Q value. we use the cross-hole data to analyze the stability and reliability of this method. The results of absorption compensation shows that our method apply much more to the real data, which indicates that the LSCFS method is more robust and more precise for Q estimation than the other two methods.
机译:质量因子Q的估计起着基本作用,以通过近表面层的吸收补偿来增强地震分辨率。已经广泛用于估计Q值,光谱比例(SRM)和质心频移方法(CFS)的两种方法。但是,在低信噪比(SNR)数据下,SRM对噪声和性能太敏感。当小波的频谱偏离高斯类似时,CFS估计的Q值将产生偏差。在本文中,我们提出了一种新方法进行Q估计。通过建立参考小波对数频谱区域与对数频谱(LSCF)的质心频移到逆Q值的关系。我们使用交叉孔数据来分析该方法的稳定性和可靠性。吸收补偿的结果表明,我们的方法对实际数据施加了更多的应用,这表明LSCFS方法比其他两种方法更加坚固,更精确的Q估计。

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