scholarly journals REVERSE TIME MIGRATION BY INTERPOLATION AND PSEUDO-ANALYTICAL METHODS

2014 ◽  
Vol 32 (4) ◽  
pp. 753 ◽  
Author(s):  
Rafael L. de Araújo ◽  
Reynam Da C. Pestana

ABSTRACT. Within the seismic method, in order to obtain an accurate image, it is necessary to use some processing techniques, among them the seismic migration. The reverse time migration (RTM) uses the complete wave equation, which implicitly includes multiple arrivals, can image all dips and, therefore, makes it possible to image complex structures. However, its application on 3D pre-stack data is still restricted due to the enormous computational effort required. With recent technological advances and faster computers, 3D pre-stack RTM is being used to address the imaging challenges posed by sub-salt and other complex subsurface targets. Thus, in order to balance processing cost and with image’s quality and confiability, different numeric methods are used to compute the migration. This work presents two different ways of performing the reverse time migration using the complete wave equation: RTMby interpolation and by the pseudo-analytical method. The first migrates the data with different constant velocities and interpolate the results, while the second uses modifications in the computation of the Laplacian operator inorder to improve the finite difference scheme used to approximate the second-order time derivative, making it possible to propagate the wave field stably even using larger time steps. The method’s applicability was tested by the migration of two-dimensional pre- and pos-stack synthetic datasets, the SEG/EAGE salt model and the Marmousi model. A real pre-stack data from the Gulf of Mexico was migrated successfully and is also presented. Through the numerical examples the applicabilityand robustness of these methods were proved and it was also showed that they can extrapolate wavefields with a much larger time step than commonly used.Keywords: acoustic wave equation, seismic migration, reverse time migration, pseudo-spectral method, pseudo-analytical method, pseudo-Laplacian operator. RESUMO. No método sísmico, a fim de se obter uma imagem precisa, faz-se necessário o uso de técnicas de processamento, entre elas a migração sísmica.A migração reversa no tempo (RTM) empregada aqui não é um conceito novo. Ela usa a equação completa da onda, implicitamente inclui múltiplas chegadas, consegue imagear todos os mergulhos e, assim, possibilita o imageamento de estruturas complexas. Porém, sua aplicação em problemas 3D pré-empilhamento continua endo restrita por conta do grande esforço computacional requerido. Mas, recentemente, com o avanço tecnológico e computadores mais rápidos, a migração 3D pré-empilhamento tem sido aplicada, especialmente, em problemas de difícil imageamento, como o de estruturas complexas em regiões de pré-sal. Assim, com o intuito de equilibrar o custo de processamento com a qualidade e confiabilidade da imagem obtida, são utilizados diferentes métodos numéricos para computar a migração. Este trabalho apresenta duas diferentes maneiras de se realizar a migração reversa no tempo partindo da solução exata da equação completa da onda: RTM por interpolação e pelo método pseudo-analítico. No método de interpolação, a migração é aplicada utilizando-se várias velocidades constantes, seguido de um procedimento de interpolação para obter a imagem migrada através da composição das imagens computadas a partir dessas velocidades constantes. Já no método pseudo-analítico, introduz-se modificações no cálculo do operador Laplaciano visando melhorar a aproximação da derivada segunda no tempo, que são feitas por esquemas de diferenças finitas de segunda ordem, possibilitando assim propagar o campo de onda de forma estável usando-se passos maiores no tempo. A aplicabilidadedas metodologias foi testada por meio da migração de dados bidimensionais sintéticos pré e pós-empilhamento, o modelo de domo de sal da SEG/EAGE e o modelo Marmousi. Um dado real bidimensional, adquirido no Golfo do México não empilhado, também, foi usado e migrado com sucesso. Assim, através desses exemplos numéricos, mostra-se a aplicabilidade e a robustez desses novos métodos de migração reversa no tempo no imageamento de estruturas complexas com os campos de ondas propagados com passos maiores no tempo do que os usados comumente.Palavras-chave: equação da onda, migração sísmica, migração reversa no tempo, método pseudo-espectral, método pseudo-analítico, operador pseudo-Laplaciano.

Geophysics ◽  
2017 ◽  
Vol 82 (2) ◽  
pp. S129-S141 ◽  
Author(s):  
Chen Tang ◽  
George A. McMechan ◽  
Deli Wang

Angle-domain common-image gathers (ADCIGs) obtained from reverse time migration are important for velocity and reflectivity inversion. Using the Poynting vector (PV) is an efficient way to calculate ADCIGs, but it suffers from inaccuracy and instability. A well-known reason is that a PV can give only one direction per grid point per time step, and thus it cannot calculate the individual directions of overlapping wavefields. This problem can be addressed by using a multidirectional PV (MPV), which decomposes the wavefields into several “approximate” directions and then calculates PVs for each decomposed wavefield. However, the MPV still suffers from another instability problem. The PV is the product of the time and space derivatives of the wavefield, and so it will be zero when the magnitude of the wavefield is at a local peak, which means that the directions are undefined. This leads to unstable points when the wavefields are close to a local magnitude peak, and it thus reduces the quality of the ADCIGs. We have developed two methods to stabilize the MPVs. The first method makes use of the property that the seismic wavelet has a short time duration, during which the propagation direction is stable. Thus, for each point in a decomposed wavefield, a time shift is used to locate the optimal PV during a short time duration, and the optimal location coincides with the local maximum magnitude of the time derivative. Therefore, there is a time shift between the wavefield and its corresponding PV. The second method combines the existing optical flow (OF) with the multidirectional scheme to produce a multidirectional OF (MOF). The MOF is iterative, and thus it has greater computational complexity. Numerical examples show that the time-shift MPV and MOF give more accurate ADCIGs than those using MPV only.


Geophysics ◽  
2019 ◽  
Vol 84 (2) ◽  
pp. S57-S69 ◽  
Author(s):  
Qingqing Li ◽  
Li-Yun Fu ◽  
Hui Zhou ◽  
Wei Wei ◽  
Wanting Hou

Seismic waves are attenuated and distorted during propagation because of the conversion of acoustic energy to heat energy. We focus on intrinsic attenuation, which is caused by [Formula: see text], which is the portion of energy lost during each cycle or wavelength. Amplitude attenuation can decrease the energy of the wavefields, and dispersion effects distort the phase of seismic waves. Attenuation and dispersion effects can reduce the resolution of image, and they can especially distort the real position of interfaces. On the basis of the viscoacoustic wave equation consisting of a single standard linear solid, we have derived a new viscoacoustic wave equation with decoupled amplitude attenuation and phase dispersion. Subsequently, we adopt a theoretical framework of viscoacoustic reverse time migration that can compensate the amplitude loss and the phase dispersion. Compared with the other variable fractional Laplacian viscoacoustic wave equations with decoupled amplitude attenuation and phase dispersion terms, the order of the Laplacian operator in our equation is a constant. The amplitude attenuation term is solved by pseudospectral method, and only one fast Fourier transform is required in each time step. The phase dispersion term can be computed using a finite-difference method. Numerical examples prove that our equation can accurately simulate the attenuation effects very well. Simulation of the new viscoacoustic equation indicates high efficiency because only one constant fractional Laplacian operator exists in this new viscoacoustic wave equation, which can reduce the number of inverse Fourier transforms to improve the computation efficiency of forward modeling and [Formula: see text]-compensated reverse time migration ([Formula: see text]-RTM). We tested the [Formula: see text]-RTM by using Marmousi and BP gas models and compared the [Formula: see text]-RTM images with those without compensation and attenuation (the reference image). [Formula: see text]-RTM results match well with the reference images. We also compared the field data migration images with and without compensation. Results demonstrate the accuracy and efficiency of the presented new viscoacoustic wave equation.


Geophysics ◽  
2019 ◽  
Vol 84 (5) ◽  
pp. S401-S409
Author(s):  
Hong Liang ◽  
Houzhu Zhang

Reverse time migration (RTM) is implemented by solving the two-way wave equation using recorded data as boundary conditions. The full wave equation can simulate wave propagation in all directions; thus, RTM has no dip limitations and is capable of imaging complex structures. Because wavefields are allowed to travel in all directions, the source and receiver wavefields can be scattered back from strong velocity contrasts. The crosscorrelation of head waves, diving waves, and backscattered waves along a raypath can lead to strong artifacts in the RTM image. These artifacts degrade the final image quality. An inversion-based imaging condition that computes the weighted sum of a time derivative image and a spatial gradient image can significantly reduce the RTM artifacts. Based on the multiscale directional selectivity property of the wavelet transform, we have developed a new method to compute the weighting function for the inversion-based imaging condition in the wavelet domain. The unique property of this approach is that the weighting function depends on the spatial locations, wavenumber, and local directions. This multidimensional property allows us to selectively remove the RTM image artifacts while preserving useful energy. We determine the effectiveness of our method for attenuating RTM artifacts using synthetic examples.


2017 ◽  
Vol 35 (1) ◽  
Author(s):  
Juan Guillermo Paniagua Castrillón ◽  
Olga Lucia Quintero Montoya ◽  
Daniel Sierra-Sosa

ABSTRACT. Reverse time migration (RTM) solves the acoustic or elastic wave equation by means of the extrapolation from source and receiver wavefield in time. A migrated image is obtained by applying a criteria known as imaging condition. The cross-correlation between source and receiver wavefields is the commonly used imaging condition. However, this imaging condition produces...Keywords: Laguerre-Gauss transform, zero-lag cross-correlation, seismic migration, imaging condition. RESUMO. A migração reversa no tempo (RTM) resolve a equação de onda acústica ou elástica por meio da extrapolação a partir do campo de onda da fonte e do receptor no tempo. Uma imagem migrada é obtida aplicando um critério conhecido como condição de imagem. A correlação cruzada entre campos de onda de fonte e receptor é a condição de imagem comumente usada. No entanto, esta condição de imagem...Palavras-chave: Transformação de Laguerre-Gauss, correlação cruzada atraso zero, migração sísmica, condição de imagem.


Geophysics ◽  
1998 ◽  
Vol 63 (2) ◽  
pp. 589-600 ◽  
Author(s):  
Yafei Wu ◽  
George A. McMechan

A wavelet transformation is performed over each of the spatial coordinates of the scalar wave equation. This transformed equation is solved directly with a finite‐difference scheme for both homogeneous and smooth inhomogeneous media. Wavefield extrapolation is performed completely in the spatial wavelet domain without transforming back into the space domain at each time step. The wavelet coefficients are extrapolated, rather than the wavefield itself. The numerical solution of the scalar wave equation in the spatial wavelet domain is closely related to the finite‐difference method because of the compact support of the wavelet bases. Poststack reverse‐time migration is implemented as an application. The resolution spaces of the wavelet transform provide a natural framework for multigrid analysis. Migrated images are constructed from various resolution spaces.


Geophysics ◽  
2011 ◽  
Vol 76 (4) ◽  
pp. S177-S185 ◽  
Author(s):  
Ekkehart Tessmer

Reverse-time migration is based on seismic forward modeling algorithms, where spatial derivatives usually are calculated by finite differences or by the Fourier method. Time integration in general is done by finite-difference time stepping of low orders. If the spatial derivatives are calculated by high-order methods and time stepping is based on low-order methods, there is an imbalance that might require that the time-step size needs to be very small to avoid numerical dispersion. As a result, computing times increase. Using the rapid expansion method (REM) avoids numerical dispersion if the number of expansion terms is chosen properly. Comparisons with analytical solutions show that the REM is preferable, especially at larger propagation times. For reverse-time migration, the REM needs to be applied in a time-stepping manner. This is necessary because the original implementation based on very large time spans requires that the source term is separable in space and time. This is not appropriate for reverse-time migration where the sources have different time histories. In reverse-time migration, it might be desirable to use the Poynting vector information to estimate opening angles to improve the quality of the image. In the solution of the wave equation, this requires that one calculates not only the pressure wavefield but also its time derivative. The rapid expansion method can be extended easily to provide this time derivative with negligible extra cost.


2021 ◽  
Vol 11 (7) ◽  
pp. 3010
Author(s):  
Hao Liu ◽  
Xuewei Liu

The lack of an initial condition is one of the major challenges in full-wave-equation depth extrapolation. This initial condition is the vertical partial derivative of the surface wavefield and cannot be provided by the conventional seismic acquisition system. The traditional solution is to use the wavefield value of the surface to calculate the vertical partial derivative by assuming that the surface velocity is constant. However, for seismic exploration on land, the surface velocity is often not uniform. To solve this problem, we propose a new method for calculating the vertical partial derivative from the surface wavefield without making any assumptions about the surface conditions. Based on the calculated derivative, we implemented a depth-extrapolation-based full-wave-equation migration from topography using the direct downward continuation. We tested the imaging performance of our proposed method with several experiments. The results of the Marmousi model experiment show that our proposed method is superior to the conventional reverse time migration (RTM) algorithm in terms of imaging accuracy and amplitude-preserving performance at medium and deep depths. In the Canadian Foothills model experiment, we proved that our method can still accurately image complex structures and maintain amplitude under topographic scenario.


Geophysics ◽  
2021 ◽  
pp. 1-65
Author(s):  
Yingming Qu ◽  
Yixin Wang ◽  
Zhenchun Li ◽  
Chang Liu

Seismic wave attenuation caused by subsurface viscoelasticity reduces the quality of migration and the reliability of interpretation. A variety of Q-compensated migration methods have been developed based on the second-order viscoacoustic quasidifferential equations. However, these second-order wave-equation-based methods are difficult to handle with density perturbation and surface topography. In addition, the staggered grid scheme, which has an advantage over the collocated grid scheme because of its reduced numerical dispersion and enhanced stability, works in first-order wave-equation-based methods. We have developed a Q least-squares reverse time migration method based on the first-order viscoacoustic quasidifferential equations by deriving Q-compensated forward-propagated operators, Q-compensated adjoint operators, and Q-attenuated Born modeling operators. Besides, our method using curvilinear grids is available even when the attenuating medium has surface topography and can conduct Q-compensated migration with density perturbation. The results of numerical tests on two synthetic and a field data sets indicate that our method improves the imaging quality with iterations and produces better imaging results with clearer structures, higher signal-to-noise ratio, higher resolution, and more balanced amplitude by correcting the energy loss and phase distortion caused by Q attenuation. It also suppresses the scattering and diffracted noise caused by the surface topography.


2014 ◽  
Vol 962-965 ◽  
pp. 2984-2987
Author(s):  
Jia Jia Yang ◽  
Bing Shou He ◽  
Ting Chen

Based on two-way acoustic wave equation, we present a method for computing angle-domain common-image gathers for reverse time migration. The method calculates the propagation direction of source wave-fields and receiver wave-fields according to expression of energy flow density vectors (Poynting vectors) of acoustic wave equation in space-time domain to obtain the reflection angle, then apply the normalized cross-correlation imaging condition to achieve the angle-domain common-image gathers. The angle gathers obtained can be used for migration velocity analysis, AVA analysis and so on. Numerical examples and real data examples demonstrate the effectiveness of this method.


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