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Migration Deconvolution via Deep Learning

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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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Correspondence to Manuel Ramón Vargas Avila.

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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.

Table 2 SFCNN topology
Table 3 WGAN topology
Table 4 U-NET topology

Appendix 2: Parallel Plan Velocity Model Results

This section presents the results obtained for the parallel plan velocity model. See Fig. 3.

Fig. 3
figure 3

a Parallel plan velocity model. b Filtered parallel plan reflectivity model. c The network input (\(m_2\)). d The network target (\(m_1\)). e The HF-LSM result. f The result for SFCNN topology. g The result for U-Net topology. h The result for WGAN topology

Appendix 3: Modified SEG/EAGE Velocity Model Results

This section shows the results obtained for the modified SEG/EAGE velocity model. See Fig. 4.

Fig. 4
figure 4

a SEG/EAGE velocity model. b SEG/EAGE filtered reflectivity model. c The network input (\(m_2\)). d The network target (\(m_1\)). e The HF-LSM result. f The result for SFCNN topology. g The result for U-Net topology. h The result for WGAN topology

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.

Fig. 5
figure 5

a SMAART Pluto velocity model. b Filtered SMAART Pluto reflectivity model. c The network input (\(m_2\)). d The network target (\(m_1\)). e The HF-LSM result. f The result for SFCNN topology. g The result for U-Net topology. h The result for WGAN topology

Fig. 6
figure 6

Zoom view of the marked box in images in the a filtered reflectivity model (Fig. 5b). b The network target (Fig. 5d). c The HF-LSM result (Fig. 5e). d The result for SFCNN topology (Fig. 5f). e The result for U-Net topology (Fig. 5g). f The result for WGAN topology (Fig. 5h)

Fig. 7
figure 7

Wavenumber amplitude spectra from Fig. 6a–e. a Filtered reflectivity model. b The network target, \(\mathbf{m}_1\). c The HF-LSM result. d The result for SFCNN topology. e The result for U-Net topology. f The result for WGAN topology

Fig. 8
figure 8

Normalized mean vertical spectra of the images: filtered reflectivity model, the HF-LSM result, the network target and the results of SFCNN, U-Net and WGAN topology

Fig. 9
figure 9

Curves extracted at a depth of 8991.6 m

Fig. 10
figure 10

a Zoom view of the region where the pseudo-wells are extracted on the filtered reflectivity model. b Pseudo-well comparison at 28 km

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.

Table 5 Evaluation measure of the topologies for each data set

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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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