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Figure and Table Captions
Figure 1.
Shear wave birefringence: velocity in fracture is faster along it than
at right angles to it.
Figure 2:
Time structure of the Phosphoria. The orientation of the anticline is
140 degrees. Notice the structure indicating later faulting at 90 degree
azimuth, marked by the dashed line running diagonally across the center
of the display.
Figure
3: Azimuthally restricted prestack seismic gathers for orthogonal
azimuths at the same location. The amplitudes in the box in the gather
at left increase with increasing shot-to-receiver distance (from right
to left), while the corresponding amplitudes in the orthogonal gather
(right) have no change in amplitude. This difference is used to indicate
the fracture direction and to estimate the fracture density.
Figure
4: Oriented core analysis
displayed as a rose diagram shows the strike of open and partially open
fracture sets observed in the core taken from the Phosphoria formation
in the 34-28P well.
Figure
5: Estimated fracture strike and crack density in the Phosphoria derived
using seismic AVO at the 43-33 well location, plus interpretation. The
fracture strike distribution is far more complex than was originally
anticipated; its interpretation appears to be geologically reasonable
with most fracture orientations paralleling the major geologic features:
the anticline (140 degrees) and the fault (90 degrees). The high values
of crack density on the lower right side of the figure are due to edge
effects.
Table
1. Comparison of seismic AVO fracture strike analysis to strike analysis
from oriented core.
Introduction
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 influence production.
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Method
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 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.
Examples
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 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 seismic data. The values derived from these data may be
map-migrated to correctly position the detected fracture strikes and
crack densities. A window from the top Phosphoria to 10 milliseconds
below is used. The average value for this zone is shown on the map.
Conclusions
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 direction. If the fractures have different aperture or spacing
in different directions, then the seismic may find a weighted average.
Far example, if fractures at 0 degrees are 0.1mm thick and fractures at
60 degrees are 0.2mm thick, then the weighted average is 40 degrees.
Reference
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.
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