Improving subsalt image from multiazimuth TTI reprocessing at Kepler Field, Gulf of Mexico
- Bunmi Elebiju (BP E&P) | Kevin Pratt (BP) | Weiping Gou (CGG) | Yu Zeng (CGG)
- Document ID
- Society of Exploration Geophysicists
- 2016 SEG International Exposition and Annual Meeting, 16-21 October, Dallas, Texas
- Publication Date
- Document Type
- Conference Paper
- 2016. Society of Exploration Geophysicists
- Velocity, Salt, Multiazimuth, TTI, Gulf of Mexico
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- 29 since 2007
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Subsalt imaging at the Kepler field, located in deep water Gulf of Mexico, has proven to be challenging, largely because of suboptimal illumination and complicated ray bending caused by complex overburden salt. It is well understood that building an accurate velocity model is one of the prerequisites to obtain a good subsalt image. Multi-azimuth seismic data sets not only help with improving subsalt illumination, they also benefit the velocity model building process by providing more data to constrain the updates. In 2015, we leveraged all the available data azimuths in the Kepler area, and reprocessed two orthogonal wide-azimuth towed streamers (WATS) and two orthogonal narrow-azimuth towed streamers (NATS) data sets, with the goal of further improving the Kepler subsalt image.
In this paper, we demonstrate the impact of multi-azimuth data and the Kepler salt geometry on subsalt illumination through a 3D ray-tracing and finite difference modeling illumination study. The integration of a top of salt (TOS) anomaly layer into the Kepler salt velocity model significantly improved the subsalt images and reduced base of salt depth uncertainties. A Shot Patch-based 3D Angle Gather Illumination Weighting workflow further improved Kepler subsalt images and signal-to-noise ratio (S/N). The step changes in the 2015 Kepler subsalt image help with reliable subsalt mapping in the Kepler area. Although the previous subsalt 4D result was inconclusive, the new seismic volumes helps with reliable amplitude extractions and have influenced volumetric estimations, reservoir modeling, and future drilling decisions in the Kepler area.
Presentation Date: Tuesday, October 18, 2016
Start Time: 2:15:00 PM
Presentation Type: ORAL
|File Size||1 MB||Number of Pages||5|
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