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Frequency-domain reflection waveform inversion with generalized internal multiple imaging
DOI:10.1190/GEO2020-0706.1.png)
Abstract
En 中文
Full-waveform inversion (FWI) has the potential to provide a high-resolution detailed model of the earth's subsurface, but it often fails to do so if the starting model differs significantly from the true one. Reflection waveform inversion (RWI) is a popular method for building a sufficiently accurate initial model for FWI. In traditional RWI, the low-wavenumber updates are always computed and captured by smearing the data misfit along the reflection path with the help of migration/demigration. However, the success of RWI relies heavily on accurately reproducing the data in demigration. Thus, we have introduced a new generalized internal multiple imaging-based RWI (GIMI-RWI) implementation. in which we avoid the Born modeling and update the primary reflection kernel directly. In GLMI-RWI, we store one reflection kernel for each source-receiver pair, preserving the unique wave-path for every single source-receiver trace. Subsequently, the convolution between the data residuals and the corresponding reflection kernel can build the tomographic velocity updates. In this situation, the long-wavelength tomographic updates are free of migration footprints and will contribute a smoother background velocity to reduce the cycle-skipping risk and stabilize the followed FWI process. In addition. the GIMI-RWI method is source independent because it entirely relies on the data. Using a synthetic example extracted from the Sigsbee2A model, we find the reliable performance of the GIMI-RWI technique.
Keywords:
MIGRATION VELOCITY ANALYSIS
TRAVEL-TIME INVERSION
Journal
IF:
3.2
Papers:
8.4K
Citations:
3.3W
Organization
Cited Papers
Angle-domain common-image gathers for migration velocity analysis by wavefield-continuation imaging
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Elastic reflection waveform inversion based on the decomposition of sensitivity kernels
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IF3.2
Full model wavenumber inversion: Identifying sources of information for the elusive middle model wavenumbers
GEOPHYSICS
IF3.2

