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Introduction

Velocity model building has been one of the most challenging problems in the seismic exploration industry. Wave-Equation Migration Velocity Analysis (WEMVA) has been widely studied for velocity building and can be implemented either in the data space (Woodward, 1992; Tarantola, 1984) or in the image space (Shen, 2004; Guerra et al., 2009; Sava and Biondi, 2004b; Shen and Symes, 2008; Sava and Biondi, 2004a). Several advantages drive us to use the image-space WEMVA instead of data-space WEMVA (which is also known as Full-Waveform Inversion): 1), migrated image is often much cleaner than the recorded wavefields; 2), the objective function is directly related to the final image; 3), image-space WEMVA can use a less accurate initial solution without encountering the cycle-skipping problems that can plague FWI. In fact, the optimized output of the image-space WEMVA can be used as the input for FWI (Li and Biondi, 2011).

Since first reported in exploration seismology in the 1930s (McCollum and Snell, 1932), anisotropy has become increasingly important in seismic imaging and exploration. The increasing offset and azimuth in data acquisition has heightened the need for anisotropic imaging and model building. Until now, the transverse isotropic (TI) model has been one most commonly used in seismic imaging and has been considered a better description of the subsurface. Li and Biondi (2011) extend the WEMVA framework to VTI media using the one-way wave-equation. However, the one-way wave-equation cannot accurately describe the wave propagation at large angles with respect to vertical, where anisotropy has larger effects. There have been extensive studies on anisotropic RTM with increasingly complex subsurface models (Zhang and Zhang, 2009; Fletcher et al., 2009), but reliable anisotropic model-building techniques are still needed.

Therefore, we propose an image-space WEMVA method using a VTI two-way wave-equation as the propagation engine, and evaluate the flatness of the RTM images in the angle domain. In this paper, we first derive the gradient of the differential semblance optimization (DSO) objective function with respect to velocity and $ \epsilon $ using a Lagrangian augmented functional. To resolve the ambiguity between velocity and $ \epsilon $ and ensure that our model honors the geology, we use a preconditioning inversion scheme. Finally, we test the proposed method on a synthetic VTI Marmousi model.


next up previous [pdf]

Next: First-order Two-way VTI wave-equation Up: Li et al.: VTI Previous: Li et al.: VTI

2012-05-10