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High-resolution velocity gathers and offset space reconstruction

机译:高分辨率速度采集和偏移空间重构

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摘要

We present a high-resolution procedure to reconstruct common-midpoint (CMP) gathers. First, we describe the forward and inverse transformations between offset and velocity space. Then, we formulate an underdetermined linear inverse problem in which the target is the artifacts-free, aperture-compensated velocity gather. We show that a sparse inversion leads to a solution that resembles the infinite-aperture velocity gather. The latter is the velocity gather that should have been estimated with a simple conjugate operator designed from an infinite-aperture seismic array. This high-resolution velocity gather is then used to reconstruct the offset space. The algorithm is formally derived using two basic principles. First, we use the principle of maximum entropy to translate prior information about the unknown parameters into a probabilistic framework, in other words, to assign a probability density function to our model. Second, we apply Bayes's rule to relate the a priori probability density function (pdf) with the pdf corresponding to the experimental uncertainties (likelihood function) to construct the a posteriori distribu- tion of the unknown parameters. Finally the model is evaluated by maximizing the a posteriori distribution. When the problem is correctly regularized, the algorithm converges to a solution characterized by different degrees of sparseness depending on the required resolution. The solutions exhibit minimum entropy when the entropy is measured in terms of Burg's definition. We emphasize two crucial differences in our approach with the familiar Burg method of maximum entropy spectral analysis. First, Burg's entropy is minimized rather than maximized, which is equivalent to inferring as much as possible about the model from the data. Second, our approach uses the data as constraints in contrast with the classic maximum entropy spectral analysis approach where the autocorrelation function is the constraint. This implies that we recover not only amplitude information but also phase information, which serves to extrapolate the data outside the original aperture of the array. The tradeoff is controlled by a single parameter that under asymptotic conditions reduces the method to a damped least-squares solution. Finally, the high-resolution or aperture-compensated velocity gather is used to extrapolate near- and far-offset traces.
机译:我们提出了一种高分辨率程序来重建公共中点(CMP)集。首先,我们描述了偏移量和速度空间之间的正向和反向变换。然后,我们制定了一个不确定的线性逆问题,其中的目标是无伪像,孔径补偿的速度聚集。我们表明,稀疏反演会导致类似于无限孔径速度聚集的解决方案。后者是应该由无穷大地震阵列设计的简单共轭算子估计的速度聚集。然后,此高分辨率速度采集用于重构偏移空间。该算法是使用两个基本原理正式得出的。首先,我们使用最大熵原理将关于未知参数的先验信息转换为概率框架,换句话说,为我们的模型分配了概率密度函数。其次,我们应用贝叶斯规则将先验概率密度函数(pdf)与对应于实验不确定性(似然函数)的pdf相关联,以构造未知参数的后验分布。最后,通过最大化后验分布来评估模型。当正确地解决了问题后,该算法将收敛到一个解决方案,该解决方案的特征在于所需的分辨率取决于不同的稀疏程度。当根据Burg的定义测量熵时,解决方案显示出最小的熵。我们用熟悉的最大熵谱分析的Burg方法强调了我们方法中的两个关键差异。首先,伯格的熵被最小化而不是最大化,这等效于从数据中尽可能多地推断模型。其次,与经典的最大熵谱分析方法(自相关函数是约束)相比,我们的方法将数据用作约束。这意味着我们不仅恢复幅度信息,而且还恢复相位信息,这有助于将数据外推到阵列的原始孔径之外。折衷由单个参数控制,该参数在渐近条件下将方法简化为阻尼最小二乘解。最后,高分辨率或孔径补偿的速度采集用于外推近,远偏移轨迹。

著录项

  • 来源
    《Geophysics》 |1995年第4期|p.1169-1177|共9页
  • 作者单位

    Dept. of Geophysics and Astronomy, The University of British Columbia, 129-2219 Main Mall, Vancouver, B.C., V6T 1Z4, Canada;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地球物理学;
  • 关键词

  • 入库时间 2022-08-18 00:20:14

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