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Adaptive finite difference for seismic wavefield modelling in acoustic media
Gang Yao1, Di Wu2, Henry Alexander Debens1
1Department of Earth Science and Engineering, Imperial College London, London SW7 2BP, UK.
Scientific Reports
|August 6, 2016
Summary
This study introduces a novel finite difference method for seismic wavefield modeling. The new approach enhances accuracy by adaptively optimizing finite difference coefficients for seismic imaging.
Area of Science:
- Geophysics
- Computational Seismology
- Numerical Methods
Background:
- Efficient numerical seismic wavefield modeling is crucial for advanced seismic imaging techniques like reverse-time migration and full-waveform inversion.
- Finite difference methods are a widely adopted numerical approach for forward modeling in seismology.
Purpose of the Study:
- To introduce a novel finite difference scheme for seismic wavefield modeling.
- To enhance the accuracy of finite difference operators in seismic imaging applications.
Main Methods:
- A time-to-space wavelet mapping technique is introduced to implement finite difference.
- Finite difference coefficients are computed by minimizing the discrepancy between mapped wavelet spatial derivatives and the finite difference operator.
- Coefficients are adapted based on velocity and source wavelet bandwidth to maximize operator accuracy.
Main Results:
- The novel finite difference method demonstrates superior accuracy compared to standard finite difference approaches.
- The method's performance is comparable to existing optimized finite difference schemes, such as Zhang's scheme.
- Numerical examples validate the effectiveness of the proposed adaptive coefficient computation.
Conclusions:
- The developed time-to-space wavelet mapping finite difference scheme offers improved accuracy for seismic wavefield modeling.
- This adaptive approach provides a more precise finite difference operator, beneficial for seismic imaging.
- The method presents a valuable alternative for accurate and efficient seismic data processing.
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