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首页> 外文期刊>Geophysics: Journal of the Society of Exploration Geophysicists >3D Kirchhoff prestack time migration in average illumination-azimuth and incident-angle domain for isotropic and vertical transversely isotropic media
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3D Kirchhoff prestack time migration in average illumination-azimuth and incident-angle domain for isotropic and vertical transversely isotropic media

机译:各向同性和垂直横向各向同性介质在平均照明方位角和入射角域中的3D Kirchhoff叠前时间偏移

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摘要

Conventional offset domain prestack migration tends to bring ambiguity and migration artifacts because it smears energy from different angles at the image point. To avoid this, prestack depth migration implementations in angle domain have been investigated in the past decades. As an efficient imaging tool, angle domain Kirchhoff prestack time migration is still useful and was proposed recently. However, existing algorithms cannot handle ray bending and anisotropy correctly. Practically, azimuth analysis for fractured reservoirs should be carried out after migration for most geological settings. Unfortunately, the existing migration algorithm implicitly involves some kind of binning to source-receiver azimuth, which may not be the real wave-path azimuth, especially for side-scattering or out-of-plane waves. In this paper, we present an algorithm for 3D Kirchhoff prestack time migration in average illumination azimuth and incident angle domain, which matches true wave path naturally and more accurately. To handle ray bending and vertical transversely isotropy, we propose several approaches to estimate two-way travel-time and the corresponding angular attributes through extended offset-to-angle mapping. Based upon these approaches, our 3D prestack time migration can provide high-quality common-image gathers for amplitude variation with incident angle and/or amplitude variation with offset and azimuth analyses, even in media with slight to moderate lateral heterogeneity. The 2D and 3D synthetic examples prove the validity of our methods.
机译:传统的偏移域叠前偏移往往会带来歧义和偏移伪影,因为它会在像点上从不同角度涂抹能量。为了避免这种情况,过去几十年来已经研究了角度域中叠前深度偏移的实现方法。作为一种有效的成像工具,角域Kirchhoff叠前时间偏移仍然很有用,并且最近已经提出。但是,现有算法无法正确处理射线弯曲和各向异性。实际上,对于大多数地质环境,应在迁移后对裂缝性储层进行方位角分析。不幸的是,现有的迁移算法隐含地涉及对源-接收方方位的某种合并,这可能不是真正的波径方位,尤其是对于侧向散射或面外波而言。在本文中,我们提出了一种在平均照明方位角和入射角域内进行3D Kirchhoff叠前时间偏移的算法,该算法自然且准确地匹配了真实的波路径。为了处理射线弯曲和垂直横向各向同性,我们提出了几种方法来通过扩展的偏移量到角度映射来估计双向传播时间和相应的角度属性。基于这些方法,我们的3D叠前时间偏移可以提供高质量的通用图像采集,即使入射角略有中度变化的介质,也可以通过入射角和/或振幅变化(通过偏移和方位角分析)来提供幅值变化。 2D和3D合成示例证明了我们方法的有效性。

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