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3-D Seismic in Identifying Spatially Variant Fracture Orientation in the Manderson Field, Wyoming*
By
David Gray1
Search and Discovery Article #40049 (2002)
*Adapted for online presentation from an article by the same author in AAPG Explorer (September, 1999), entitled “Using 3-D Seismic to Identity Spatially Variant Fracture Orientation in the Manderson Field." Appreciation is expressed to the author and to M. Ray Thomasson, former Chairman of the AAPG Geophysical Integration Committee, and Larry Nation, AAPG Communications Director, for their support of this online version.
1Research programmer ([email protected]), Veritas DGC Inc., Calgary (www.veritasdgc.com). Co-authors for this article are Kim Head, Veritas Exploration Services, Calgary, Kent Chamberlain, Gordon Olson, and John Sinclair, KCS Mountain Resources, Worland, Wyoming, and Chris Besler, Interactive Earth Sciences, Denver.
Abstract
Oil is produced from the Manderson Field, in Wyoming's Big Horn Basin, from a fracture system with possible significant lateral connectivity; therefore, characterizing the fractures in this field is of great importance. Amplitude Versus Offset (AVO) analysis of azimuthally restricted seismic data is used to determine the orientation and density of fractures at selected locations corresponding to well sites in the Manderson Field. The result of this analysis is compared to fracture strike analysis from oriented cores for three wells.
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The Manderson Field in Big Horn Basin, discovered in 1951, is located on a sharp, asymmetric, northwest-plunging anticline. It produces oil and gas from Pennsylvanian, Permian and Cretaceous horizons, although the Permian Phosphoria is the most productive zone. It is a complex interval consisting of a thick unit of medium-to-thick bedded, fractured carbonate. Purchased by KCS Mountain Resources in 1995, the field showed several wells with cumulative production in excess of original oil-in-place estimates. Low matrix porosity, production history and strong pressure support suggest that oil is produced from a fracture system with significant lateral connectivity. Four oriented cores and one Formation Micro-Imager (FMI) log were taken by KCS between 1996 and 1998. Analysis of fractures in the cores and the FMI show varied fracture orientations at different wells within the field. A
3-D seismic survey was undertaken in 1996 to improve structural
definition of the reservoir. The survey was reprocessed in 1998 to
further improve structural characteristics--and to detect those,
fractures that strongly The seismic data from the Manderson 3-D was acquired over a full 360 degree azimuthal range--a suitable candidate for the test of measurements of azimuthal anisotropy from pre-stack seismic data using seismic AVO techniques. This method examines differences in the AVO response with respect to azimuth to predict the primary fracture strike and the relative density of cracks. The Manderson 3-D covers the locations of three wells for which oriented cores have been analyzed for fracture azimuth. This experiment is to determine whether fracture strike and fracture density can be determined from 3-D seismic data in the Manderson Field. The requirements for this analysis are full azimuthal coverage in the 3-D seismic (excluding the edges) and sufficient source-to-receiver offsets to measure significant differences in azimuthal AVO effects in the zone of interest in the Phosphoria carbonate at 1,200-1,400 meters (approximately 6,700 feet). The five locations chosen for these tests are centered on the wells 4333P, 34-28P, 34-18P, 42-24P and 1218P. Well 43-33P is the most productive well in the field, and wells 34-28P, 34-18P, and 42-24P have fracture strike analysis. Well 42-24P was abandoned shortly after drilling, without achieving commercial production. A
modification of the AVO method of Lynn et al. (1996) is used to estimate
the fracture strike and density at these locations. The theory behind
this method is that the acoustic The
primary Azimuthal differences in AVO response are shown in the change in amplitudes with shot-receiver offset as shown in the boxes in Figure 3. These amplitudes are larger at long offsets in the gather on the left than the one on the right. The fracture azimuth predicted by the seismic data falls within the range of values estimated from the oriented core (Table 1). This azimuth appears to be the average value for the open fractures. For example, the strike orientation rose diagram for the open fractures of the 34-28P well (Figure 4) shows three significant strike directions, at 0, 60 and 105 degrees. If all these fracture strikes are averaged then 84 degrees is the expected response. The
average fracture strike (Figure 5) is a useful value, because the largest volume of
open fractures will be encountered by drilling horizontally
perpendicular to this average fracture There
appear to be two predominant fracture strikes indicated by the azimuthal
AVO analysis: one at 90-110 degrees follows the east-west faulting
Fracture strike and crack density are estimated from the seismic AVO response. The seismic AVO results show consistent fracture strikes and crack densities at the test locations, implying that these values are robust. The most predominant estimated fracture strikes at these locations coincide with the major geologic features in the area, a correlation that makes sense from a geologic standpoint. The fracture strikes derived using AVO agree with the average fracture strikes determined from oriented cores. Crack density may correlate with average fracture aperture, and it generates significantly higher values at the location of the most prolific wells in the Manderson Field.
It is
important to note that this AVO method probably finds the average
fracture
Lynn, H.B., Simon, K.M., and Bates, C.R., 1996, Correlation between P-wave AVOA and S-wave traveltime anisotropy in a naturally fractured gas reservoir. |


