高级检索

    基于自适应空间网格的逆时偏移成像

    Reverse time migration based on adaptive spatial grids

    • 摘要: 面向深层复杂地质目标时,逆时偏移(RTM)是深度域偏移成像的有力工具。深层地震成像需要使用深大偏移速度模型,所以,基于波动方程理论的RTM成像计算成本更为高昂。当近地表速度较低或采用较高主频的子波时,常规网格往往采样不充分,这会导致数值频散,从而影响成像精度。为保证成像精度,采用细网格将带来庞大的计算量和内存需求。提出了一种基于自适应空间网格的逆时偏移成像方法:首先,对偏移速度模型进行自适应网格剖分;然后,采用自适应网格坐标系下的波动方程模拟震源波场和检波点反传波场;最后,将成像结果转换回常规网格坐标系,得到最终的RTM成像结果。模型测试和实际资料应用结果表明,该方法在浅层低速区能够自适应加密网格,有效压制频散,提升浅层成像效果;在深层高速区,能够自适应增大网格空间步长,减少网格数量,有效降低计算量,节约内存。

       

      Abstract: Reverse time migration (RTM) is a powerful tool for depth-domain imaging to reconstruct geologically complex deep targets. Deep seismic imaging, particularly through wave-equation-based RTM, is computationally intensive owing to the large-scale migration velocity model from shallow to deep zones. When near-surface velocities are low or a high-frequency wavelet is used, conventional coarse grid sampling often proves inadequate, leading to numerical dispersion and consequent low imaging accuracy. Conversely, fine grid sampling achieves high-precision imaging at the sacrifice of significantly increased computational costs and memory requirements. We propose a RTM method based on adaptive spatial grids. The approach consists of three key steps: adaptive grid partitioning of the migration velocity model, finite-difference wave-equation simulation of forward-time source wavefield and reverse-time receiver wavefield based on adaptive spatial grids, and transformation back to the conventional-grid coordinate system to obtain the final RTM image. Automatic grid refinement in shallow low-velocity zones effectively alleviates dispersion and enhances imaging quality, and adaptive grid coarsening in deep high-velocity zones reduces grid count, computational load, and memory requirements. Model and field data tests demonstrate the accuracy and computational efficiency of this method.

       

    /

    返回文章
    返回