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Crooked-line 2D seismic reflection imaging in crystalline terrains: Part 2, migration

机译:结晶地形中的弯曲线二维地震反射成像:第2部分,迁移

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摘要

Seismic reflection surveys are frequently conducted over very complicated geological structure, but surveying often must be confined to existing crooked roads or tracks. Typically, data from such 2D crooked-line surveys are processed using standard common midpoint (CMP) stacking techniques to obtain a 2D time section which is then 2D migrated. In Part I, we show that a reflector dip component across the processing line can cause serious problems for standard CMP stacking. We also propose a supplementary processing step in which cross-dip is determined locally and cross-dip moveout (CDMO) is removed from data to form an optimum cross-dip stack. However, a crooked-line survey is really a swath 3D survey, and ideally we would like to obtain a 3D image of reflectivity surrounding the profile. Here we investigate the potential of 3D prestack Kirchhoff migration to directly image all observed reflections; i.e., we attempt to construct a 3D image volume of all reflectors viewed by the survey. Because reflectors that face away from the acquisition line cannot return much wave energy from available sources to available receivers, they cannot be imaged even if they lie directly beneath the survey profile. Tests show that the cross-profile spread of trace midpoints usually is sufficient to provide a useful degree of cross-line positioning of reflection points. A very helpful image volume is thus obtained. Kirchhoff 3D prestack migration is computationally laborious. A much quicker but less complete method is to create the 3D migrated image volume from the 2D optimum cross-dip stack and the associated set of cross-dips. Robustness of migration methods to time errors in the prestack data traces such as poorly corrected statics is also an issue. Tests show that in difficult cases, particularly where only 2D processing is warranted, migration of trace absolute amplitude rather than standard phase data may lead to a superior result.
机译:地震反射调查通常是在非常复杂的地质结构上进行的,但是调查通常必须限于现有的弯曲道路或轨道。通常,使用标准的公共中点(CMP)堆栈技术处理来自此类2D弯曲线勘测的数据,以获得2D时间段,然后将其进行2D迁移。在第一部分中,我们展示了跨越生产线的反射器浸入组件可能会导致标准CMP堆叠的严重问题。我们还提出了一个补充处理步骤,在该步骤中,局部确定交叉倾角,并从数据中删除交叉倾角偏移(CDMO),以形成最佳的交叉倾角堆栈。但是,弯曲线勘测实际上是3D测绘,理想情况下,我们希望获得轮廓周围反射率的3D图像。在这里,我们研究了3D叠前Kirchhoff偏移直接成像所有观测到的反射的潜力;即,我们尝试构建调查所查看的所有反射器的3D图像体积。由于背离采集线的反射器无法将大量波能从可用光源返回到可用接收器,因此即使它们直接位于勘测剖面图之下也无法成像。测试表明,迹线中点的交叉分布通常足以提供反射点的交叉线定位的有用程度。由此获得非常有用的图像体积。 Kirchhoff 3D叠前迁移在计算上很费力。一种更快但不完整的方法是根据2D最佳交叉浸入堆栈和相关的交叉浸入集合创建3D迁移的图像体积。迁移方法对叠前数据迹线中的时间错误(例如校正不佳的静态数据)的鲁棒性也是一个问题。测试表明,在困难的情况下,尤其是仅需要进行2D处理的情况下,迹线绝对幅度而不是标准相位数据的偏移可能会导致更好的结果。

著录项

  • 来源
    《Geophysics》 |2003年第1期|p.286-296|共11页
  • 作者单位

    Formerly Geological Survey of Canada―Pacific, Natural Resources Canada;

    presently Columbia University, Lamont-Doherty Earth Observatory, 61 Route 9W, P.O. Box 1000, Palisades, New York 10964-8000;

  • 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

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