Abstract
The fault shadow problem is what explorationists call the zone of unreliable seismic imaging in the footwalls of faults. Although it can occur in all types of faults, the term is usually applied to extensional faults. These problems are common‐place, but much current exploration still relies on images in which they remain. In this article I present an example of the fault shadow problem from the Wilcox trend (Eocene/Paleocene) of south Texas. The stratigraphic‐velocity alternations in this area cause a distinctive suite of problems in conventional time imaging. Explorationists can cite numerous examples of wells drilled on time highs, but significantly off structure in depth. Moreover, imaging often degrades precipitously at levels below the Middle Wilcox even when wells indicate an uncomplicated structure. I’ll begin by demonstrating, through schematic and synthetic examples, the nature of these problems and their elimination through prestack depth imaging. A real data example will then show identical ef...
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.