3D weak-dispersion reverse time migration using a stereo-modeling operator

Reliable 3D imaging is a required tool for developing models of complex geologic structures. Reverse time migration (RTM), as the most powerful depth imaging method, has become the preferred imaging tool because of its ability to handle complex velocity models including steeply dipping interfaces an...

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Main Authors: Li, Jingshuang, Fehler, Michael, Yang, Dinghui, Huang, Xueyuan
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: Society of Exploration Geophysicists 2015
Online Access:http://hdl.handle.net/1721.1/96309
https://orcid.org/0000-0002-8814-5495
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author Li, Jingshuang
Fehler, Michael
Yang, Dinghui
Huang, Xueyuan
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Li, Jingshuang
Fehler, Michael
Yang, Dinghui
Huang, Xueyuan
author_sort Li, Jingshuang
collection MIT
description Reliable 3D imaging is a required tool for developing models of complex geologic structures. Reverse time migration (RTM), as the most powerful depth imaging method, has become the preferred imaging tool because of its ability to handle complex velocity models including steeply dipping interfaces and large velocity contrasts. Finite-difference methods are among the most popular numerical approaches used for RTM. However, these methods often encounter a serious issue of numerical dispersion, which is typically suppressed by reducing the grid interval of the propagation model, resulting in large computation and memory requirements. In addition, even with small grid spacing, numerical anisotropy may degrade images or, worse, provide images that appear to be focused but position events incorrectly. Recently, stereo-operators have been developed to approximate the partial differential operator in space. These operators have been used to develop several weak-dispersion and efficient stereo-modeling methods that have been found to be superior to conventional algorithms in suppressing numerical dispersion and numerical anisotropy. We generalized one stereo-modeling method, fourth-order nearly analytic central difference (NACD), from 2D to 3D and applied it to 3D RTM. The RTM results for the 3D SEG/EAGE phase A classic data set 1 and the SEG Advanced Modeling project model demonstrated that, even when using a large grid size, the NACD method can handle very complex velocity models and produced better images than can be obtained using the fourth-order and eighth-order Lax-Wendroff correction (LWC) schemes. We also applied 3D NACD and fourth-order LWC to a field data set and illustrated significant improvements in terms of structure imaging, horizon/layer continuity and positioning. We also investigated numerical dispersion and found that not only does the NACD method have superior dispersion characteristics but also that the angular variation of dispersion is significantly less than for LWC. Read More: http://library.seg.org/doi/abs/10.1190/geo2013-0472.1
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spelling mit-1721.1/963092022-09-28T09:01:41Z 3D weak-dispersion reverse time migration using a stereo-modeling operator Li, Jingshuang Fehler, Michael Yang, Dinghui Huang, Xueyuan Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Fehler, Michael Reliable 3D imaging is a required tool for developing models of complex geologic structures. Reverse time migration (RTM), as the most powerful depth imaging method, has become the preferred imaging tool because of its ability to handle complex velocity models including steeply dipping interfaces and large velocity contrasts. Finite-difference methods are among the most popular numerical approaches used for RTM. However, these methods often encounter a serious issue of numerical dispersion, which is typically suppressed by reducing the grid interval of the propagation model, resulting in large computation and memory requirements. In addition, even with small grid spacing, numerical anisotropy may degrade images or, worse, provide images that appear to be focused but position events incorrectly. Recently, stereo-operators have been developed to approximate the partial differential operator in space. These operators have been used to develop several weak-dispersion and efficient stereo-modeling methods that have been found to be superior to conventional algorithms in suppressing numerical dispersion and numerical anisotropy. We generalized one stereo-modeling method, fourth-order nearly analytic central difference (NACD), from 2D to 3D and applied it to 3D RTM. The RTM results for the 3D SEG/EAGE phase A classic data set 1 and the SEG Advanced Modeling project model demonstrated that, even when using a large grid size, the NACD method can handle very complex velocity models and produced better images than can be obtained using the fourth-order and eighth-order Lax-Wendroff correction (LWC) schemes. We also applied 3D NACD and fourth-order LWC to a field data set and illustrated significant improvements in terms of structure imaging, horizon/layer continuity and positioning. We also investigated numerical dispersion and found that not only does the NACD method have superior dispersion characteristics but also that the angular variation of dispersion is significantly less than for LWC. Read More: http://library.seg.org/doi/abs/10.1190/geo2013-0472.1 National Natural Science Foundation (China) (Grant 41230210) Massachusetts Institute of Technology. Earth Resources Laboratory (Founding Members Consortium) 2015-04-01T16:29:56Z 2015-04-01T16:29:56Z 2014-12 2014-08 Article http://purl.org/eprint/type/JournalArticle 0016-8033 1942-2156 http://hdl.handle.net/1721.1/96309 Li, Jingshuang, Michael Fehler, Dinghui Yang, and Xueyuan Huang. “3D Weak-Dispersion Reverse Time Migration Using a Stereo-Modeling Operator.” GEOPHYSICS 80, no. 1 (December 5, 2014): S19–S30. © 2014 Society of Exploration Geophysicists https://orcid.org/0000-0002-8814-5495 en_US http://dx.doi.org/10.1190/GEO2013-0472.1 Geophysics Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf Society of Exploration Geophysicists Society of Exploration Geophysicists
spellingShingle Li, Jingshuang
Fehler, Michael
Yang, Dinghui
Huang, Xueyuan
3D weak-dispersion reverse time migration using a stereo-modeling operator
title 3D weak-dispersion reverse time migration using a stereo-modeling operator
title_full 3D weak-dispersion reverse time migration using a stereo-modeling operator
title_fullStr 3D weak-dispersion reverse time migration using a stereo-modeling operator
title_full_unstemmed 3D weak-dispersion reverse time migration using a stereo-modeling operator
title_short 3D weak-dispersion reverse time migration using a stereo-modeling operator
title_sort 3d weak dispersion reverse time migration using a stereo modeling operator
url http://hdl.handle.net/1721.1/96309
https://orcid.org/0000-0002-8814-5495
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