seismic imaging of spur and groove structures in the san...
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Seismic imaging of spur and groove structures in the San Andres Formation, Midland Basin,
Texas. Gabriel Machado
1, Kurt J. Marfurt
1, Oswaldo Davogustto
1 and Matthew Pranter
2
1 Oklahoma University and
2University of Colorado
Summary
Spur and groves are reef related structures that form in the
windward side of fringing or barrier reefs owing to
different intrinsic and extrinsic mechanisms. The purpose
of this study is to characterize these structures through different seismic attributes and interpret the growth history
of the reefs within the seismic volume.
Geologic Setting
The San Andres Formation is a mainly carbonate
prograding stratigraphic unit of Guadalupian age in the
northern shelf of the Midland Basin, Texas. The lithology
includes dolomite, limestone, salt and some siliciclastics facies like silty sandstones and skeletal wackestones,
among others (Ramondetta, 1982).
The study area is located in the Diamond M field in the Scurry Reef Trend in Scurry County, Texas (Walker et al,
1991) and corresponds to the section above the Horseshoe
Atoll in the same region (see Figure 1)
The studied section corresponds to a fringing reef back
barrier lagoon sequence .Spur and grooves structures form
in the windward side of modern reefs (Wood and
Oppenheimer, 2000) with their long axes normal to the refracted waves, which can make them good
paleohydrodynamic indicators (Sneh and Friedman, 1980).
They range from 8 to 65 m in width, up to 10 m in height
and can form 45 m below sea level. Two processes are taking place in the formation of these reef structures:
organic growth of the reefs and erosion owing to backsurge
of refracted waves (Cloud, 1959).
DOI http://dx.doi.org/10.1190/segam2013-1431.1© 2013 SEGSEG Houston 2013 Annual Meeting Page 1545
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Seismic Imaging of Spur and Groove structures
Data Available
A 33 mi² survey was acquired with an inline and crossline
interval of 75 ft. Since the San Andres formation is one of
the most prolific reservoirs of Texas in the 1980s
(Ramondetta, 1982) many wells were drilled in the region, so that 165 were available with up to 65 well logs in some
of them.
Methodology
We used eight wells with P-wave sonic logs to tie with the
seismic in order to make a seismic inversion and better recognize the carbonate buildup related features, as can be
observed in Figure 2
We recognized from seismic inversion five different stages through time for the fringing reef.
Spur and grooves
Based on the seismic inversion and the known geology,
several spur and groove structures were recognized in the
seismic volume. They are easily differentiated through
different attributes, such as curvature and dip magnitude.
On Figure 3, the spur and groove structures can be seen in
the west part of the survey. The K1 most positive curvature
highlights the spurs and the K2 most negative curvature the grooves. A shorter wavelength allows viewing some of the
heterogeneities in the carbonate structures, with the same
general trend.
On Figure 4 Sobel filter similarity and dip magnitude
attributes are used. In the Sobel filter the spur and groove
structures are not well defined.
DOI http://dx.doi.org/10.1190/segam2013-1431.1© 2013 SEGSEG Houston 2013 Annual Meeting Page 1546
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Seismic Imaging of Spur and Groove structures
On the other hand, many of the spur and grooves structures
of different scales can be well observed through the dip magnitude attribute, allowing a better defining of the
steepness they have in their boundaries with each other.
Figure 5 shows the same structures through the reflector convergence attribute showing the preferential refracted
wave orientation and the direction in which these structures
were eroded by them.
Discussions
A very interesting thing happens when the spur and
grooves are observed through the reflector convergence
attribute, as shown in Figure 6. When looking at the change
of this attribute through the San Andres Formation, a very marked difference in the general orientation of the
reflectors can be observed, from southwest-west and north
at 500 ms to northeast-east at 700 ms. The attribute was co-
rendered with most positive principal curvature in black and white so the carbonate structures could be located in
the seismic image.
This change in general convergence orientation could happen in response to changes in the marine conditions
which would have affected the coral reef growth general
orientation, or due to changes in the accommodation space
inside the basin, which would also affect the carbonate structure.
Dunlap and Wood (2010) pointed at the seismic
architecture and morphology of a seismic feature similar in form to the spur and groove structures, but that must not be
mistaken with them. Sediment waves have a similar shape
in seismic time slices, but are usually normal to the basin
slope and have lower acoustic impedance, whereas the spur and groove structures have greater acoustic impedance and
are usually normal to the refracted waves that generate
them.
DOI http://dx.doi.org/10.1190/segam2013-1431.1© 2013 SEGSEG Houston 2013 Annual Meeting Page 1547
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Seismic Imaging of Spur and Groove structures
Conclusions
Spur and grooves are carbonate structures that form on the
windward side of modern fringing and barrier reefs. They
form as a combination of the coral organic growth and the erosion generated by backsurge of refracted waves that hit
the reef.
Seismic most-positive and most-negative curvature attributes clearly delineate spur and grooves in the San
Andres Formation, while reflector convergence show not
only the orientation of the carbonate but also changes in the
hydrodynamic conditions that affected their growth
Acknowledgments
Thanks to Parallel Petroleum for providing the data used in
this research. Seismic interpretation was done using
Schlumberger’s Petrel and inversion using Hampson Russell’s Strata software. Attributes were generated using
software developed as part of the OU AASPI consortium.
We thank all who helped me in attribute interpretation and
imaging – Alfredo Fernandez, Luis Castillo, Roderick Perez and Rebecca Da Silva, among others.
DOI http://dx.doi.org/10.1190/segam2013-1431.1© 2013 SEGSEG Houston 2013 Annual Meeting Page 1548
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http://dx.doi.org/10.1190/segam2013-1431.1 EDITED REFERENCES Note: This reference list is a copy-edited version of the reference list submitted by the author. Reference lists for the 2013 SEG Technical Program Expanded Abstracts have been copy edited so that references provided with the online metadata for each paper will achieve a high degree of linking to cited sources that appear on the Web. REFERENCES
Cloud, P. E. Jr., 1959, Geology of Saipan, Mariana Islands, Part 4—Submarine topography and shallow-water ecology: U.S. Geol. Survey Professional Paper 280-k, 361–445.
Dunlap, D. B., and L. J. Wood, 2010, Seismic architecture and morphology of Mesozoic -Age sediment waves, offshore Morocco, northwest Africa: 2010 GCSSEPM, in Seismic imaging of depositional and geomorphic systems, 30th annual GCSSEPM Foundation Bob F. Perkins Research Conference, L. J. Wood, T. T. Simo and N. C. Rosen, eds., 551–571.
Ramondetta, P. J., 1982, Facies and stratigraphy of the San Andres Formation, northern and northwestern shelves of the Midland Basin, Texas and New Mexico: Bureau of Economic Geology Report of Investigation No. 128.
Sneh, A., and G. M. Friedman, 1980, Spur and groove patterns on the reefs of the northern gulfs of the Red Sea: The Society of Economic Paleontologists and Mineralogists: Journal of Sedimentary Petrology, 50, 981–986.
Walker, D. A., J. Golonka, A. M. Reid, and S. T. Reid, 1991, The effects of late Paleozoic paleolatitude and paleogeography on carbonate sedimentation in the Midland Basin, Texas; Permian Basin plays: Society of Economic Paleontologists and Mineralogists, Permian Basin Chapter, Tomorrow’s Technology Today, 141–162.
Wood, R., and C. Oppenheimer, 2000, Spur and groove morphology from a Late Devonian reef: Sedimentary Geology, 133, no. 3-4, 185–193, http://dx.doi.org/10.1016/S0037-0738(00)00032-4.
DOI http://dx.doi.org/10.1190/segam2013-1431.1© 2013 SEGSEG Houston 2013 Annual Meeting Page 1549
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ded
10/1
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5. R
edis
trib
utio
n su
bjec
t to
SEG
lice
nse
or c
opyr
ight
; see
Ter
ms
of U
se a
t http
://lib
rary
.seg
.org
/