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Divergent and asymptotic nature of the time-offset Taner-Koehler series in reflection seismics

机译:反射地震中时间偏移量Taner-Koehler级数的发散和渐近性质

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摘要

Power series (1) has been known in essence for more than four decades and has long been used to represent traveltime in reflection seismics. We show the series is degenerate, divergent, and an asymptotic expansion about the zero offset. The accuracy of the truncated series, though remarkable for small offsets, is usually poor for large offsets; equation (7) is a better alternative. The analytical results imply the formal invalidity of the proof in Al-Chalabi (1973) that rms velocity is less than or equal to stacking velocity. The asymptotic nature controls the accuracy of the series approximation, implying initial convergence and subsequent divergence. The use of the series must be limited to the range of convergence, which ends at the term with the smallest magnitude. The optimal strategy is to include not as many terms as possible but only the first several terms before the smallest, the ensuing error being of the order of the magnitude of the first discarded term. The asymptotic nature explains several of the convergence characteristics of the partial sum and the latter's oscillation about the true traveltime. The nonanalytic nature of traveltime also implies (a) the increasing order of an optimal polynomial does not necessarily improve accuracy while representing traveltime in terms of offset and (b) an optimal polynomial in terms of offset is an inadequate model of travel-time at large offsets. Another consequence is the feasibility of an asymptotic expansion about a nonzero offset, which eventuall leads to equation (7), apt for represeting traveltime in the far-offset range. The use of equations (6) and (7) and a regression analysis of the observed traveltimes over all offsets yield estimates of the coefficients of series (1), which are useful for moveout correction and have interpretation in terms of velocity models of the earth.
机译:幂级数(1)从本质上讲已有40多年的历史了,长期以来一直被用来代表反射地震的传播时间。我们证明了该级数是退化的,发散的并且关于零偏移量的渐近展开。截短序列的精度尽管对于小偏移量来说是显着的,但对于大偏移量通常是差的。等式(7)是更好的选择。分析结果表明,Al-Chalabi(1973)的均方根速度小于或等于堆积速度的证明在形式上是无效的。渐近性质控制级数逼近的准确性,这意味着初始收敛和随后的发散。该系列的使用必须限于收敛范围,该收敛范围以最小量级的项结束。最佳策略是不包括尽可能多的项,而仅包括最小项之前的前几个项,随之而来的误差约为第一个被舍弃项的数量级。渐近性质解释了部分和的一些收敛特征以及后者关于真实旅行时间的振荡。行程时间的非分析性质还意味着(a)最优多项式的递增阶数不一定可以在以偏移量表示行程时间的同时提高准确性,并且(b)偏移量的最优多项式在很大程度上是行程时间模型的不足抵消。另一个结果是围绕非零偏移量进行渐近展开的可行性,最终导致方程(7),该方程式易于在远偏移范围内预设行进时间。使用方程式(6)和(7)以及在所有偏移量上观察到的行进时间进行回归分析,可以得出级数(1)的系数的估计值,这对于校正位移很有用,并且可以解释地球的速度模型。

著录项

  • 来源
    《Geophysics》 |2002年第6期|p.1913-1919|共7页
  • 作者单位

    National Geophysical Research Institute, Uppal Road, Hyderabad 500007, India;

  • 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 00:19:53

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