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Real data

In order to further test our operator, we apply it to a real data line. The Alba Oil Field is located in the UK North Sea and elongates along a NW-SE axis. The oil reservoir is 9km long, 1.5km wide, and up to 90m thick at a depth of 1,900m sub sea (, ).

The producing reservoir consists of unconsolidated high-porosity turbiditic sandstone of Eocene age. The oil-bearing reservoir sand and the overlying shale have a very low P-wave acoustic impedance contrast but make a significant S-wave velocity contrast. Hence, the reservoir delineation using only normal PP-seismic data is very difficult. Therefore, the ocean bottom PS-data was acquired ().

Even though the Alba field is a 3D data set, we select one line by choosing a source line that overlaps a receiver line. There are several gaps in our selected data since we are taking a 2D line from a 3D data set.

Figure [*] shows a CMP gather from the PZ-component and the PS-component of the data. Note the gaps and irregularities in the data.

Figure [*] shows a comparison between the NMO stack and the DMO stack of the PP line. The DMO was performed by the same algorithm described here, specifying 65#65.

Figure [*] shows the PS result. It compares the PS-NMO CCP binning stack and the PS-DMO stack. The PS-DMO stack was obtained using the filter described in equation ([*]). Observe that, even though it is a flat events area, those small dips are better defined after doing PS-DMO.

Figure [*] shows the PS-DMO result using the filter described in equation ([*]), which better handles the amplitudes. Note that some strong dip energy appears. The rest of the section remains the same. Therefore, the filter in equation ([*]) produces more accurate results.

 
cmps
cmps
Figure 4
CMPS
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pp
pp
Figure 5
PP results, NMO-stack (top), DMO-stack (bottom)
[*] view burn build edit restore

 
psone
psone
Figure 6
PS results, PS-NMO CCP binning stack (top), PS-DMO stack (bottom)
[*] view burn build edit restore

 
pstwo
pstwo
Figure 7
PS-DMO considering amplitudes
[*] view burn build edit restore


next up previous print clean
Next: Discussion Up: Prucha and Biondi: STANFORD Previous: PS-DMO in the frequency-wavenumber
Stanford Exploration Project
6/7/2002