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Layer thickness estimation from the frequency spectrum of seismic reflection data

机译:地震反射数据频谱层厚度估计

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We compare the spectra of Short Time Window Fourier Transform (STFT) and Constrained Least Squares Spectral Analysis (CLSSA) for spectral minima periodicity. Using time thickness equals 1/df, where df is frequency period, we show that spectral minima approach using CLSSA gives more accurate time thicknesses than STFT for the same analysis window. Starting with a broad band synthetic seismic data generated from a wedge model, we extract selected traces at known temporal thicknesses for time frequency analysis. We cross plot apparent time thicknesses derived from CLSSA and STFT line spectra using the approach above, against true time thicknesses of the wedge model. The result shows apparent CLSSA thicknesses that are strongly correlated with true time thicknesses We extend this study to real seismic data from Hitts Lake Field, onshore Texas and show that the results are consistent with the results from model studies.
机译:我们比较短时间窗口傅立叶变换(STFT)的光谱,并限制最小二乘频谱分析(CLSSA),用于光谱最短的周期性。使用时间厚度等于1 / DF,其中DF是频率周期,我们表明使用CLSSA的光谱最小值方法比同一分析窗口的STFT提供比STF更精确的时间厚度。从楔形模型产生的宽带合成地震数据开始,我们以已知的时间厚度提取所选择的迹线进行时间频率分析。我们使用上面的方法对来自CLSSA和STFT线谱衍生自CLSSA和STFT线光谱的绘图表观时间厚度,抵抗楔形模型的真实厚度。结果表明,明显的CLSA厚度与真实厚度强烈相关,我们将本研究扩展到来自Hitts Lake Field的真实地震数据,德克萨斯州北京德克萨斯州北京德克萨斯州,并表明结果与模型研究的结果一致。

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