Abstract
Migration deconvolution is an image domain approach to least-squares migration, which is considered the state-of-the-art algorithm for obtaining seismic reflectivity models of the earth from seismic acquisition results. Seismic imaging is an active research field with the development over the last few years of several techniques that have mitigated imaging issues. Ongoing research aims to improve image resolution and thus provide a more reliable seismic amplitude for the interpreter. Migration deconvolution can be framed as an inverse problem in the image domain to mitigate image resolution problems and reduce migration artifacts. This paper presents a migration deconvolution method via deep learning based on the Hessian filter least-squares migration (HF-LSM) algorithm. The idea is to use deep learning techniques to model the inverse operator instead of directly estimating the inverse Hessian matrix. A data set is generated from a given velocity model by applying Born modeling to the migrated image, followed by application of the reverse time migration algorithm. The resultant data set is then used to train several neural network models. The networks learn the blurring operator that describes the image degradation due to the effects of acquisition geometry. Three different network topologies were developed to handle this problem: a simple fully convolutional neural network, a U-Net and a generative adversarial network. Our results show that the proposed approach provides images of higher resolution and superior quality than the traditional HF-LSM workflow.
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Acknowledgements
The authors would like to thank PETROBRAS for providing financial support to this project as well for authorizing the publication of the results. We would also like to thank the Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) for providing scholarships to the authors. Nvidia Corporation provided the computational resources required for this research.
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Appendices
Appendix 1: Neural Network Topologies
This appendix presents details of the neural network topologies proposed in this work, such as activation functions and the kernel size of each convolutional layer, among others, as shown in the Tables 2, 3 and 4 for the SFCNN, WGAN and U-Net topologies, respectively.
Appendix 2: Parallel Plan Velocity Model Results
This section presents the results obtained for the parallel plan velocity model. See Fig. 3.
Appendix 3: Modified SEG/EAGE Velocity Model Results
This section shows the results obtained for the modified SEG/EAGE velocity model. See Fig. 4.
Appendix 4: SMAART Pluto Velocity Model Results
This section presents the results obtained for the SMAART Pluto velocity model, with a more detailed discussion of these results given in Sect. 4.3. See Figs. 5, 6, 7, 8, 9 and 10.
Appendix 5: Evaluation Measures for All Velocity Models
Table 5 shows the evaluation measures for all velocity models tested. As we can see from the results, the neural networks achieved better results than the HF-LSM method for both PSNR and SSIM. This shows that the networks were better amplitude-wise and structurally.
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Avila, M.R.V., Osorio, L.N., de Castro Vargas Fernandes, J. et al. Migration Deconvolution via Deep Learning. Pure Appl. Geophys. 178, 1677–1695 (2021). https://doi.org/10.1007/s00024-021-02707-0
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DOI: https://doi.org/10.1007/s00024-021-02707-0