首页 | 本学科首页   官方微博 | 高级检索  
     检索      

基于Chebyshev多项式的非对称走时Kirchhoff叠前时间偏移角道集求取
引用本文:刘志远,常旭,刘伊克,王一博,杜向东.基于Chebyshev多项式的非对称走时Kirchhoff叠前时间偏移角道集求取[J].地球物理学报,2013,56(8):2783-2789.
作者姓名:刘志远  常旭  刘伊克  王一博  杜向东
作者单位: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. 中海油研究总院, 北京 100027; 3. 中石化勘探开发研究院油气地球物理研究中心, 北京 100083
基金项目:国家重点基础研究发展计划项目,国家科技重大专项子课题
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.

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  
收稿时间:2012-04-02

Using Chebyshev polynomial asymmetric calculation to obtain angle domain common imaging gathers by Kirchhoff pre-stack time migration
LIU Zhi-Yuan , CHANG Xu , LIU Yi-Ke , WANG Yi-Bo , DU Xiang-Dong.Using Chebyshev polynomial asymmetric calculation to obtain angle domain common imaging gathers by Kirchhoff pre-stack time migration[J].Chinese Journal of Geophysics,2013,56(8):2783-2789.
Authors:LIU Zhi-Yuan  CHANG Xu  LIU Yi-Ke  WANG Yi-Bo  DU Xiang-Dong
Institution:1. Key Lab of Engineering Geomechanics, Institute of Geology and Geophysics,Chinese Academy of Sciences, Beijing 100029,China; 2. Science and Technology Development Department of China National Offshore Oil Corp,Beijing 100027,China; 3. Geophysical Research Center,SINOPEC Exploration & Production Research Institute,Beijing 100083,China
Abstract:Kirchhoff pre-stack 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. It is verified that using our method to obtain ADCIG is more precise and consumes less computation time.
Keywords:Kirchhoff pre-stack time migration  Chebyshev polynomial  Bend-ray  Asymmetric travel time formula  Angle domain common image gathers
本文献已被 CNKI 万方数据 等数据库收录!
点击此处可从《地球物理学报》浏览原始摘要信息
点击此处可从《地球物理学报》下载免费的PDF全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号