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GCVertical Seismic Profiling at Eldfisk Field *
Bob Hardage1
Camp 1 said, “The anticline has a true collapsed top and reserves are reduced.”
Camp 2 said, “There is a low-velocity chimney in the thick shale above the structure that creates a velocity pull down and there is no collapsed top.”
Camp 1 wanted to interpret a fault where one is drawn on the profile; Camp 2 believed that there was no fault, just a velocity-generated time sag.
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VSP ProjectA VSP project was designed to acquire information to help resolve these two opposing structural interpretations – the VSP geometry that was used is illustrated as Figure 2. An obligated field-evaluation well (Figure 1) had to be drilled and was used as a VSP receiver well to decide where to place the next evaluation well. The VSP source was offset 2.5 kilometers from the well, so that if there were a low-velocity gas cloud above the crest of the structure, the down-going VSP raypath would pass under the velocity anomaly (Figure 2). Up-going reflected VSP raypaths to the borehole receivers would still pass through part of the low-velocity zone.Because only a small part of the total VSP travel path traverses the low-velocity zone, any time delays introduced into VSP reflection events would be much less than the time delays associated with two-way travel paths through the low-velocity interval when towed-cable data are acquired. One combination of down-going and up-going towed-cable raypaths is shown in Figure 2. The VSP image that was produced is inserted into the 2-D towed-cable image in Figure 3; the VSP data show that the top of the Ekofisk Formation climbs smoothly and continuously to form an unbroken anticline crest at this location.
Although Camp 2 won the argument at this well location, the controversy of collapsed anticline crests remained in other parts of the greater Ekofisk development program. Not unexpectedly, some graben collapses were found at some crestal well positions (and were again verified by VSP imaging). The moral of this story: Properly designed VSP surveys can answer numerous questions about geological complexity near a receiver well. VSP imaging is often the best way to undershoot a shallow geological complexity to see a deeper target.
Conclusion
In this example, cost of the VSP survey was repaid many times over by the value of the information provided by the VSP data. The presence or absence of several million barrels of oil was at stake when field developers had to decide whether Eldfisk lost a big part of its structural crest.
With modern 3-D seismic technology we can do a much better job of creating reliable images of structure beneath complex velocity layering than was possible in the 1970s. However, there will still be locations – even today – where VSP imaging can provide information that is difficult to acquire using surface-based receiver technologies. |