基于Chebyshev多项式的非对称走时Kirchhoff叠前时间偏移角道集求取  

Using Chebyshev polynomial asymmetric calculation to obtain angle domain common imaging gathers by Kirchhoff pre-stack time migration

作　　者：刘志远[1,2] 常旭[1] 刘伊克[1] 王一博[1] 杜向东 

机构地区：[1]中国科学院地质与地球物理研究所中国科学院工程地质力学重点实验室,北京100029 [2]中石化勘探开发研究院油气地球物理研究中心,北京100083 [3]中海油研究总院,北京100027

出　　处：《地球物理学报》2013年第8期2783-2789,共7页Chinese Journal of Geophysics

基　　金：国家重点基础研究发展计划项目(2009CB219404);国家科技重大专项子课题(2011ZX05030-004-001)联合资助

摘　　要：地震射线走时的求取方法是叠前时间偏移研究的核心问题之一,也是影响计算时间域角道集角度精确性的关键因素之一.本文基于Kirchhoff叠前时间偏移,应用第一类切比雪夫多项式,对弯曲射线对称走时加以改进,引进非对称项,优化后得到切比雪夫非对称走时方程,与高精度走时进行比较和误差分析,再将该走时求取方法应用于时间域角道集的求取中,得到地下较真实的入射角.通过模型计算和实际地震资料处理证明,此种非对称走时及其角道集的求取方法具有精度高、计算量少的优点.Kirehhoff pre-staek time migration （KPSTM） is widely used in production due to its high efficiency and good suitability, especially for exploration in central and western China. Angle domain common image gathers （ADCIG） serve as the link between migration and reservoir attribute analysis. Getting ADCIG in the time domain is more efficient than in the depth domain. Seismic travel time calculation is one of the key problems of KPSTM and is also a key problem in ADCIG calculation. Using Chebyshev orthogonal polynomial and optimizing algorithm, we develop a new asymmetric Chebyshev travel time formula and compare it with high-precision taylor travel time formulas. Based on this, considering the bend-way effect, we apply the new Chebyshev travel time formula to calculate incident angles, and achieve more precise ADCIG from the original seismic gathers. The method is tested by both synthetic data and real marine data. Itis verified that using our method to obtain ADCIG is more precise and consumes less computation time.

关 键 词：KIRCHHOFF叠前时间偏移 切比雪夫多项式 弯曲射线 非对称走时方程 角道集 

分 类 号：P631[天文地球—地质矿产勘探]