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GCGeological Input Valuable in Seismic Velocity Analysis*

 

Supratik Sarkar1

 

Search and Discovery Article #41118 (2013)

Posted March 18, 2013

 

*Adapted from the Geophysical Corner column, prepared by the author, in AAPG Explorer, January, 2013, and entitled "Previous HitTimeNext Hit to Pick? No Need to Fear 'Seismophobia' ". Editor of Geophysical Corner is Satinder Chopra ([email protected]). Managing Editor of AAPG Explorer is Vern Stefanic.

 

11Shell, Deepwater/Frontier New Ventures Business Development Group, Houston, TX ([email protected])

 

General Statement

While seismic processing shops usually are the "professionals" when it comes to velocity analysis, the interpreter may have greater insight into the cause of the poor data quality. In such cases, repacking the velocities on a tight grid with a better knowledge of the geology can provide significant improvement.

General statement

Figures

Examples

Conclusion

Acknowledgments

 

 

 

 

 

 

 

 

 

General statement

Figures

Examples

Conclusion

Acknowledgments

 

 

 

 

 

 

 

 

General statement

Figures

Examples

Conclusion

Acknowledgments

 

 

 

 

 

 

 

 

Figure Captions

Figure 1. A representative common reflection point gather illustrating (a) velocity analysis of a CMP gather (b) before, and (c) after the NMO correction. A 30 percent stretch mute is applied to the flattened gathers.

Figure 2. Example of (a) original prestack Previous HittimeNext Hit migrated vertical seismic amplitude section, and (b) the same section after performing residual velocity analysis. Note the improved stratal definition within the Chicontepec interval, as demarcated by the red bracket and also below the shallow volcanic body. The frequency spectra corresponding to each volume indicates significant frequency enhancement; (c) and (d) represent equivalent coherent energy Previous HitslicesNext Hit along the yellow horizon in (a) and (b).

Example

The following example (Figure 1) is from a tight turbidite formation in Mexico's Chicontepec Basin, where the data are often handicapped by interbed multiples from overlying shallow volcanic sills. While the deeper, non-targeted Cretaceous horizons were well resolved - appearing as coherent, broad-band reflectors - the shallower Eocene/Paleocene Chicontepec Formation reflectors of interest were "wormy" and narrow-band.

The original data were prestack Previous HittimeNext Hit-migrated using a Kirchhoff algorithm, resulting in 50-meter offset bins ranging between 50 and 3,000 meters. The preliminary interpretation of the stacked data showed significant reduction of data quality below the volcanics.

Maps of the volcanics were made to highlight the problem areas. The original migration velocities were then removed (Figure 1b) using simple reverse normal moveout, followed by a velocity analysis on a dense 375-meter x 375-meter grid. Seismic processors will recognize this workflow as comprising the key steps within a typical processing sequence - using simple software tools to generate a residual velocity analysis of the previously migrated data.

The key step was to take care beneath the volcanics to pick the slower Chicontepec reflectors rather than the strong, slightly faster interbed multiples (Figure 1a), resulting in the flattened gathers like the one shown in Figure 1c. After the residual velocity analysis, the frequency content and the signal-to-noise ratio of the dataset improved in many places within the Chicontepec interval compared to the original prestack Previous HittimeTop-migrated data. This residual velocity analysis resulted in better vertical and lateral definition of stratal units as seen by seismic amplitude as well as computed attributes (Figure 2).

Conclusion

Descriptions of several volcanic episodes in east-central Mexico, from the Late Cretaceous to Miocene, have been published. The burial history chart from the adjacent Veracruz Basin - where petroleum generation occurred from Upper Jurassic source rocks similar to those in the Chicontepec play - shows that oil generation and migration started around 20 Ma and continued through the Miocene. Since most of the oil migrated after the major volcanic activities, improving the imaging below the volcanics also provided us ideas on how the volcanic bodies enhanced fracture porosities in reservoirs in some areas - especially through enhanced seismic attribute images.

This velocity analysis also helped enormously to delineate turbidite channels, internal stratal geometries and the distribution of potential reservoir elements.

Acknowledgments

I wish to thank my adviser, AAPG member Kurt J. Marfurt from the University of Oklahoma, for his constant persistence and encouragement (to a geologist) to complete the work, part of which is reflected in this article.

I also would like to thank Pemex, as well as Sergio Chavez Perez from IMP, who provided the data for working this project. I am thankful to AASPI consortium at OU for all the support.

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