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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
The
The
Manderson 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 velocity of shear waves in a fractured medium is faster parallel to the fractures than perpendicular to them. This is known as shear wave birefringence (Figure 1). Figure 1 also shows how the AVO gradient is related to the shear-wave impedance. So AVO in a fractured zone should show the largest difference between values parallel and perpendicular to the dominant fracturing direction. The primary direction of the anticlinal fold axis is 140 degrees (Figure 2). The most dominant fracture direction may be expected to be parallel and perpendicular to the fold axis at 140 degrees or 50 degrees, respectively. The AVO azimuthal analysis uses eight azimuth ranges centered on 5, 27.5, 50, 72.5, 95, 117.5, 140 and 162.5 degrees. Because each range is a 22.5 degree azimuthal cone, the error associated with any estimated fracture strike is ±11.25 degrees. These orientations, starting at 5 degrees, are based on the estimate of the primary direction of the anticline. They give complete coverage of all possible fracture strike directions. 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 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 direction. Well 43-33P is the most prolific well in the Manderson Field, and it has the largest value of crack density. Wells 34-28P, 34-18P and 42-24P indicate that there may be correlation between crack density and open fracture aperture. Combine this with the high value observed for well 43-33P, and crack density appears to have some correlation with open fracture aperture. There
appear to be two predominant fracture strikes indicated by the azimuthal
AVO analysis: one at 90-110 degrees follows the east-west faulting
direction seen in Figure 2, the other at 230-170 degrees follows the
fold axis of the anticline. All measurements are performed on the unmigrated Fracture
strike and crack density are estimated from the
It is
important to note that this AVO method probably finds the average
fracture direction. If the fractures have different aperture or spacing
in different directions, then the
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. |
