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Multi-Azimuth Seismic Data Imaging in the Presence of Orthorhombic Anisotropy

机译:在正交各向异性存在下的多方位角地震数据成像

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Orthorhombic anisotropy is considered to be the simplest realistic symmetry for many geophysical problems. Orthorhombic anisotropy exhibits both HTI (Horizontal Transverse Anisotropy) and VTI (Vertical Transverse Anisotropy) effects, making seismic velocity varying with azimuthal direction as well as polar direction. In many cases, these effects are important by themselves and can be a target of special studies. The presence of orthorhombic anisotropy poses challenges in wide azimuth imaging which has been rapidly developed for better illumination, better imaging, and better multiple elimination. Analysis of multi-azimuth (MAZ) data often reveals noticeable fluctuations in moveout between different acquisition directions, preventing constructive summation of MAZ images due to the azimuthal dependency nature of wave propagation in orthorhombic medium. On the other hand, the co- existing VTI effects of orthorhombic anisotropy can also cause well misties and higher order moveout. Orthorhombic anisotropy can take into account the co-existing HTI/VTI effects. We have developed an approach for imaging in the presence of orthorhombic anisotropy, including orthorhombic velocity analysis and orthorhombic migration. Following Tsvankin’s work, we put forward a ray tracing approach suitable for both weak and strong anisotropy which applies to both Kirchhoff and Beam PSDM. Aimed at the challenge in orthorhombic anisotropy model building, we have developed a practical workflow which combines the co-existing HTI/VTI anisotropy estimated through multi-azimuth tomography to form the orthorhombic model. In this paper, we first describe our approach for imaging in the presence of orthorhombic anisotropy, including the newly developed orthorhombic ray tracing method and the newly developed practical method for orthorhombic anisotropy model building. We then demonstrate with both synthetic and real data from offshore Australia that our approach can successfully take into account the co-existing HTI/VTI effects, reduce the structural discrepancies between seismic images built for different azimuths, hence produce constructive summation of MAZ dataset, resolve well mistie to match with geology, and deliver a step-change in the final seismic image quality.
机译:正交各向异性被认为是许多地球物理问题的最简单的逼真对称性。正交性各向异性表现出HTI(水平横向各向异性)和VTI(垂直横向各向异性)效应,使地震速度随方向方向和极性方向而变化。在许多情况下,这些效果本身是重要的,并且可以是特殊研究的目标。正交各向异性的存在在宽方形成像中存在挑战,这已经迅速开发,以便更好地照明,更好的成像和更好的多重消除。多方位角(MAZ)数据的分析通常揭示了不同采集方向之间的偏移中的显着波动,防止了MAZ图像的建设性总和导致的逆转介质中波传播的方位角性质。另一方面,正交各向异性的共同VTI效应也会导致井下误差和更高阶的震动。正交各向异性可以考虑到共同存在的HTI / VTI效应。我们开发了在正交各向异性存在下成像的方法,包括矫正速度分析和矫正迁移。在Tsvankin的工作之后,我们提出了一种适用于弱和强大的各向异性的光线跟踪方法,适用于Kirchhoff和Beam Psdm。旨在在正交各向异性模型建筑中挑战,我们开发了一种实用的工作流程,它将通过多方位角断层扫描估计的共同现有的HTI / VTI各向异性组合来形成正交模型。在本文中,我们首先描述了我们在正交各向异性存在下进行成像的方法,包括新开发的正交射线跟踪方法和新开发的正交各向异性模型建筑的实用方法。然后,我们从澳大利亚海上综合和实际数据展示了我们的方法可以成功考虑到共存的HTI / VTI效应,从而减少为不同方位角构建的地震图像之间的结构差异,因此产生了MAZ数据集的建设性求和,解决了朦胧与地质相匹配,并在最终的地震图像质量方面提供一步变化。

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