The members of the Committee approve the dissertation of Ye Li ...
Transcript of The members of the Committee approve the dissertation of Ye Li ...
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To the University of Wyoming:The members of the Committee approve the dissertation of Ye Li presented on
January 31, 2014.
Ye Zhang, Chairperson
Brian F. Towler, External Department Member
Shaochang Wo
Subhashis Mallick
Erin A. Campbell-Stone
APPROVED:
Paul L. Heller, Head, Department of Geology and Geophysics
Gregory K. Brown, Dean, College of Arts & Sciences
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Li, Ye, An Uncertainty Analysis of Modeling Geologic Carbon Sequestration in a Naturally
Fractured Reservoir at Teapot Dome, Wyoming, Ph.D., Department of Geology and
Geophysics, January, 2014.
This study presents an uncertainty analysis of Geologic Carbon Sequestration modeling
in a naturally fractured reservoir at Teapot Dome, Wyoming. Structural & stratigraphic,
residual, and solubility trapping mechanisms are the focus of this study, while mineral trap-
ping is not considered. A reservoir-scale geologic model is built to model CO2 storage in the
Tensleep Sandstone using a variety of site characterization data that have been collected,
screened for accuracy, and analyzed. These data are from diverse sources, such as reservoir
geology, geophysics, petrophysics, engineering, and analogs. Because fluid flow occurs in
both matrix and fractures of the Tensleep Sandstone, both systems of heterogeneity must
be incorporated into the geologic model. The matrix heterogeneity of the geologic model is
developed through a hierarchical process of structural modeling, facies modeling, and petro-
physical modeling. In structural modeling, the framework of the reservoir is conditioned to
seismic data and well log interpretations. Based on the concept of flow units, the facies model,
which is conditioned to a global vertical facies proportion curve that acts as soft data, is
built geostatistically by the Sequential Indicator Simulation method. Then, the petrophysi-
cal properties (porosity) are modeled geostatistically within each facies through the Sequen-
tial Gaussian Simulation approach. A Discrete Fracture Network (DFN) is adopted as the
method to model the distribution of open natural fractures in the reservoir. Basic inputs for
the DFN model are derived from FMI logs, cores, and analogs. In addition, in combination
with an artificial neural network analysis, 3D seismic attributes are used as fracture drivers
to guide the modeling of fracture intensity distribution away from the boreholes. In DFN
models, power laws are adopted to define the distribution of fracture intensity, length and
aperture.
To understand the effect of model complexity on CO2 storage predictions, a suite of
increasingly simplified conceptual geologic model families are created with decreasing amount
of site characterization data: a hierarchical stochastic model family conditioned to soft data
(FAM4), a simple stochastic facies model family (FAM3), a simple stochastic porosity model
family (FAM2), and a homogeneous model family (FAM1). These families, representing
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alternative conceptual geologic models built with increasing reduced data, are simulated
with the same CO2 injection test (20 years of injection at 1,000 Mscf/day), followed by 80
years of monitoring. Using the Design of Experiment, an efficient sensitivity analysis (SA) is
conducted for all families, systematically varying uncertain input parameters, while assuming
identical well configurations, injection rates, bottom-hole pressure constraints, and boundary
conditions. The SA results are compared among the families to identify parameters that have
1st order impact on predicting the CO2 storage ratio (SR) at two different time scales, i.e.,
end of injection and end of monitoring. This comparison indicates that, for this naturally
fractured reservoir, the facies model is necessary to study the sensitivity characteristics of
predicting the CO2 storage behavior. The SA results identify matrix relative permeability,
fracture aperture of fracture set 1, and fracture aperture of fracture set 2 as the statistically
important factors. Based on the results of the SA, a response surface analysis is conducted
to generate prediction envelopes of the CO2 storage ratio, which are also compared among
the families at both times. Its results demonstrate that the SR variation due to the different
modeling choices is relatively small. At the proposed storage site, as more than 90% of
injected CO2 is probably mobile, short-term leakage risk is considered large, and it depends
on the sealing ability of top formations.
yzhang9CalloutThe Tensleep Sandstone has significant porosity and permeability in both the sandstone matrix and in the fracture networks that percolate through the matrix. Ignoring each type of heterogeneity in building and simulating CO2 storage will likely lead to biased or inaccurate CO2 predictions. However, the considerable complexity of both matrix and fracture heterogeneity also requires us to understand the level of detail that needs to be included in building the geologic model, thus resources can be used appropriately. This study explicitly models both matrix and fracture heterogeneity, and a multiple conceptual modeling approach is used to help us understand what details are important to the prediction of CO2 flow and storage. The insights gained will help us understand how fractured reservoir models should incorporate field characterization data and how matrix and fracture heterogeneity, which occurs over disparate scales and which exhibits distinctly different spatial correlation structure and connectivity, should be explicitly resolved in such models. Moreover, the uncertainty in the prediction outcomes, which propagates from both parameter and conceptual modeling uncertainty, can be quantified to understand issues such as storage efficiency and the leakage risk. The storage efficiency is evaluated in this work using the CO2 storage ratio, while the leakage risk is evaluated by examining the extent of scCO2 migration and the size of its footprint in the reservoir.
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AN UNCERTAINTY ANALYSIS OF MODELING
GEOLOGIC CARBON SEQUESTRATION IN A
NATURALLY FRACTURED RESERVOIR AT
TEAPOT DOME, WYOMING
by
Ye Li, Ph.D. candidate
A dissertation submitted to theDepartment of Geology and Geophysics
and theUniversity of Wyoming
in partial fulfillment of the requirementsfor the degree of
DOCTOR OF PHILOSOPHYin
GEOLOGY
Laramie, WyomingJanuary 2014
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Copyright c 2014
by
Ye Li
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Dedicate this work to my parents
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Contents
List of Figures viii
List of Tables xv
Acknowledgments xvi
Chapter 1 Introduction 1
1.1 Overview and Motivation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1
1.2 Thesis Organization . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7
Chapter 2 Background and Geologic Review 10
2.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
2.2 Parameters Affecting CO2 Storage . . . . . . . . . . . . . . . . . . . . . . . . 11
2.2.1 Reservoir Heterogeneity . . . . . . . . . . . . . . . . . . . . . . . . . 11
2.2.2 Fluid Flow Properties . . . . . . . . . . . . . . . . . . . . . . . . . . 11
2.3 Geology of Teapot Dome . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
2.3.1 Structural Elements . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
2.3.2 Stratigraphy and Sedimentology . . . . . . . . . . . . . . . . . . . . . 15
2.4 Geologic Characterization Datasets . . . . . . . . . . . . . . . . . . . . . . . 20
2.4.1 Seismic Data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
2.4.2 Core Data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20
2.4.3 Well Data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
2.4.4 Outcrop Analogs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
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2.4.5 Production Data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
2.5 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
Chapter 3 Geologic Modeling 23
3.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23
3.2 Static Site Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
3.2.1 Structural Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . 24
3.2.2 Property Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29
3.3 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 48
Chapter 4 Discrete Fracture Network (DFN) Modeling 52
4.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 52
4.2 Previous Fracture Studies in the Tensleep Sandstone . . . . . . . . . . . . . 54
4.3 Fracture Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 60
4.3.1 Methods & Approaches . . . . . . . . . . . . . . . . . . . . . . . . . . 62
4.3.2 Fracture Characterization Data . . . . . . . . . . . . . . . . . . . . . 63
4.3.3 Building a DFN Model . . . . . . . . . . . . . . . . . . . . . . . . . . 64
4.4 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 75
Chapter 5 Reservoir Simulation 77
5.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 77
5.1.1 Simulation of Naturally Fractured Reservoirs The Dual Porosity Ap-
proach . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 77
5.1.2 Fluid Flow Simulation in Fractured Reservoirs . . . . . . . . . . . . . 79
5.2 Reservoir Simulation for the Tensleep Sandstone . . . . . . . . . . . . . . . . 80
5.2.1 Geologic Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82
5.2.2 Fluid Properties . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 84
5.2.3 Relative Permeability . . . . . . . . . . . . . . . . . . . . . . . . . . . 89
5.2.4 Boundary Conditions . . . . . . . . . . . . . . . . . . . . . . . . . . . 92
5.2.5 Initial Conditions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92
5.2.6 Baseline Simulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92
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5.3 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97
Chapter 6 Uncertainty Analysis 99
6.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99
6.2 Overview of Design of Experiment (DoE) methodology . . . . . . . . . . . . 101
6.3 Families of Geologic Models . . . . . . . . . . . . . . . . . . . . . . . . . . . 104
6.4 Uncertainty Factors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 106
6.4.1 Uncertainty in this study . . . . . . . . . . . . . . . . . . . . . . . . . 106
6.4.2 Shared Factors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 112
6.4.3 Family Factors . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 115
6.5 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 119
Chapter 7 Results and Discussion 120
7.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120
7.2 Screening Tests . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 120
7.3 Response Surface (RS) Modeling & Verification . . . . . . . . . . . . . . . . 129
7.4 Monte Carlo (MC) analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . 130
7.5 Plume Predictions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 135
7.6 Summary & Result . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 141
7.7 Discussion & Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142
7.7.1 Discussion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 142
7.7.2 Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153
Appendix A Geologic Modeling 155
A.1 Structural Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 155
A.1.1 Prepare Input Data for Modeling . . . . . . . . . . . . . . . . . . . . 155
A.1.2 Fault Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156
A.1.3 Pillar Gridding . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156
A.1.4 Layering . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157
A.1.5 Geometrical Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . 162
A.2 Property Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
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A.2.1 Data Preparation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 164
A.2.2 Basic Geostatistics . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166
A.2.3 Right Layer Thickness . . . . . . . . . . . . . . . . . . . . . . . . . . 168
A.2.4 Facies Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170
A.2.5 Petrophysical Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . 174
Appendix B ECLIPSE Data Files 177
B.1 Basic Input File the DATA file . . . . . . . . . . . . . . . . . . . . . . . . 177
References 186
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List of Figures
1.1 A schematic diagram of the general contributions of different CO2 trapping
mechanisms over time (after [5]). . . . . . . . . . . . . . . . . . . . . . . . . 2
2.1 The hysteresis effect of relative permeability for CO2-brine (data from [49]). 12
2.2 A Teapot Dome location map. The field is located within T. 38 - 39 N., R.
78 W. (courtesy of RMOTC [52]). . . . . . . . . . . . . . . . . . . . . . . . 13
2.3 The location of the Teapot Dome field, Tensleep structure depth, and the
proposed CO2 injection well. Structural relationship between Teapot Dome
and Salt Creek fields (after [54]). . . . . . . . . . . . . . . . . . . . . . . . . 14
2.4 Teapot Dome Geologic Column (after RMOTC [60]). . . . . . . . . . . . . . 16
2.5 A schematic stratigraphic column of reservoir (Tensleep Fm.) and the caprock
(Goose Egg Fm.) (after [63] and [62]). . . . . . . . . . . . . . . . . . . . . . 18
2.6 Cores from the Teapot Dome show fractures (courtesy of RMOTC [64]). . . 19
3.1 An arbitrary cross-section through Teapot Dome (left). A depth-structure
map on the 2nd Wall Creek Sandstone (right) showing location of cross section
line (after [40]). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
3.2 An amplitude map of the Tensleep Sandstone at Teapot Dome. Basement-
cored faults are shown (after [66]). . . . . . . . . . . . . . . . . . . . . . . . . 26
3.3 The fault model of the Tensleep Sandstone at Teapot Dome and 3D seismic
data (in the time domain). Each colored surface with sticks represents a fault
interpreted according to 3D seismic data manually. The model uses 5x vertical
exaggeration. The arrow points to the north. . . . . . . . . . . . . . . . . . . 27
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3.4 The structural model of the Tensleep Sandstone. Depth is in feet at subsea
level(in the depth domain). Negative value is below sea level. Colored points
represent well tops. The model uses 5x vertical exaggeration. The arrow
points to the north. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28
3.5 Plain-light thin-section images of different petrophysical facies of the Tensleep
Sandstone (courtesy of Dr. Peigui Yin [62]). . . . . . . . . . . . . . . . . . . 32
3.6 Distribution of petrophysical facies of the Tensleep Sandstone interval of well
54-TPX-10 and comparisons to well logs (courtesy of Dr. Peigui Yin [62]). . 34
3.7 Plot of porosity vs. permeability for different facies of the Tensleep Sandstone
(data from Dr. Peigui Yin). . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
3.8 Comparison between flow units and petrophysical properties of the plot in
Figure 3.7. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37
3.9 Comparison between petrophysical facies in [62] and flow units derived in this
study. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
3.10 A North-South stratigraphic cross section of Teapot Dome demonstrates poor
correlation between facies. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 40
3.11 The experimental variogram and the variogram model of vertical facies (flow
unit 1) in the Tensleep B Sandstone interval. The gray curve represents the
auto-fitted regression curve, and the blue curve is the variogram used during
modeling process. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
3.12 An omni-directional experimental variogram and an omni-directional vari-
ogram model in horizontal direction for flow unit 1 in the Tensleep B Sand-
stone interval. The gray curve represents the auto-fitted regression curve, and
the blue curve is the variogram used during modeling process. . . . . . . . . 43
3.13 A global vertical facies proportion curve generated from all 11 wells at the
study site. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 44
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3.14 A facies model of the Tensleep B Sandstone. Colored vertical lines represent
wells with well logs or cores. The background map is the Teapot Dome base
map, which indicates the relative location of the subsurface model to the
surface. The arrow points north. . . . . . . . . . . . . . . . . . . . . . . . . 45
3.15 Porosity variograms for the Flow Unit 1 (left column) and Flow Unit 2 (right
column) groups. Square=experimental variogram; blue line=fitted variogram
model; gray line=auto-fitted regression curve. . . . . . . . . . . . . . . . . . 47
3.16 Comparison of two porosity models based on the same facies model (Fig-
ure 3.14). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
3.17 Different correlations between porosity and permeability for flow unit 1. +
R35=11 m is for +1 case, 0 R35=2.8 m is for 0 case, and -
R35=1.0 m is for -1 case respectively (they represent totally different pos-
sible porosity-permeability relations for flow unit 1), when doing screening
test and response surface analysis in later chapters. . . . . . . . . . . . . . . 50
4.1 A schematic cross plot of percent reservoir porosity versus percent reservoir
permeability (percent due to matrix versus percent due to fractures) for the
Nelsons classification. k: permeability; : porosity; m: matrix; f: fracture.
(Modified from [90].) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53
4.2 Lower-hemisphere equal-area net plot of poles to 129 representative through-
going fractures at Teapot Dome. Fractures are considered hinge-parallel if
they strike 20 from the hinge; hinge-perpendicular fractures strike 90 20
from the hinge. In this research, fractures are divided according to Coopers
classification: Fracture Set 1: the hinge-oblique; Fracture Set 2: the hinge-
perpendicular; Fracture Set 3: the hinge-parallel (after [51]). . . . . . . . . . 55
4.3 Examples of four types of fractures in cores. (a)Gouge-filled Fractures; (b)Mineral-
filled Fractures; (c) Partially-filled Fractures; (d) Open Fractures (courtesy of
Dr. Peigui Yin [94]). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57
4.4 Partially mineralized vertical extension fracture face in the Tensleep Sand-
stone, at Teapot Dome (courtesy of RMOTC [64]). . . . . . . . . . . . . . . 61
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4.5 Upper hemisphere of Schmidt stereonet. Points represent the projection of
Pole to a fracture plane interpreted from FMI logs by Koepsell (Schlumberger). 65
4.6 Fracture attributes, such as intensity, aperture, and length that are generated
through power law. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70
4.7 Discrete Fracture Networks (DFN) for Fracture Set 1 and Fracture Set 2 in 2D. 72
4.8 DFN for Fracture Set 1 in 2D (above), and the whole DFN of three fracture
sets in 3D (below). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
4.9 Fracture permeability and porosity generated from the upscaling process by
the Oda method. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 74
5.1 Dual porosity representation of a fractured reservoir (after [116]). . . . . . . 78
5.2 A typical dual porosity block of matrix containing oil and water (after [118]). 81
5.3 Relative permeability data for CO2-brine systems at in-situ conditoins for a
sample from the Viking Fm. sandstone (data from [125]). . . . . . . . . . . 90
5.4 A smoothed relative permeability based on straight-line relative permeability. 91
5.5 CO2 saturations after injection. Each grid contains two blocks: the outer
block and the inner block. The former one represents the fracture, and the
latter represents the matrix. The color indicates the molar density of CO2.
The arrow points north. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 94
5.6 (a) CO2 plume at the end of injection; (b) CO2 plume at the end of monitoring. 95
5.7 Graph showing CO2 dissolved in water, mobile in gas, and trapped in gas over
time. Horizontal axis represents years. Injection begins in 2013, and ends in
2033. Monitoring begins in 2033, and ends in 2113. . . . . . . . . . . . . . . 96
6.1 Generalized Pennsylvanian to Early Permian paleogeography shows setting
for low sea level stand. Arrow represents paleowind direction. Black box :
approximate location of Bighorn County, Wyoming. Red box: approximate
location of Powder River Basin. Dashed line: United States border. Wavy
pattern: the sea distribution. Stippled pattern: major region of the quartz-
sand erg distribution (after [157]). . . . . . . . . . . . . . . . . . . . . . . . . 108
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6.2 Satellite images to demonstrate different shapes of dunes and interdunes(after
[158]). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110
6.3 Relative permeability data for CO2-brine systems at in-situ conditions for a
sample from the Cardium Fm. sandstone (data from [125]). . . . . . . . . . 114
6.4 Factors varied in the PB design and their ranges of variation. Numbers indi-
cate family ID. Engineering (shared) factors are shared by all model families. 117
7.1 The screening test result for FAM4 at a 90% significance level. Outcome is
the SR at EOI. Statistically significant uncertainty factors in this family are
highlighted. Negative Lenth t-Ratio means increasing value of this factor will
reduce SR. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 121
7.2 The screening test result for FAM4 at a 90% significance level. Outcome is
the SR at EOM. Statistically significant uncertainty factors in this family are
highlighted. Negative Lenth t-Ratio means increasing value of this factor will
reduce SR. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 122
7.3 The Screening Design (PB Design) for FAM4. (Part 1) . . . . . . . . . . . . 125
7.4 -(Continued) The Screening Design (PB Design) for FAM4. (Part 2) . . . . . 126
7.5 -(Continued) The Screening Design (PB Design) for FAM4. (Part 3) . . . . . 127
7.6 Response Surface Design for FAM4 . . . . . . . . . . . . . . . . . . . . . . . 128
7.7 Parameter estimates of a second order polynomial RS model of storage ratio
for FAM4 at EOM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130
7.8 An example of RS predicted storage ratio versus simulated storage ratio at
PB design points for FAM4 at EOM. Comparison is for verification of the RS
fitted model. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 131
7.9 Factors varied in the PB design and their ranges of variation. Numbers indi-
cate family ID. Engineering (shared) factors are shared by all model families. 132
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7.10 Cumulative distribution function (cdf ) of the storage ratio for FAM3 (the first
row) and FAM4 (the second row): (left) end of injection; (right) end of mon-
itoring. MC w/ RS is generated with 100,000 MC simulations (exhaustive
cdf ); RS is the cdf constructed using results of the response surface design
runs. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 133
7.11 Cumulative distribution function of the RS-predicted storage ratio for all fam-
ilies: (left) end of injection; (right) end of monitoring. . . . . . . . . . . . . . 135
7.12 Top views: molar density of CO2 (mobile + trapped) as predicted by each
family at EOI, [top face of the model]: (left column) FAM3; (right colum)
FAM4; . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 137
7.13 Top views: molar density of CO2 (mobile + trapped) as predicted by each
family at EOM, [top face of the model]: (left column) FAM3; (right colum)
FAM4; . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 138
7.14 Base views: molar density of CO2 (mobile + trapped) as predicted by each
family at EOI, [bottom face of the model]: (left column) FAM3; (right colum)
FAM4; . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 139
7.15 Base views: molar density of CO2 (mobile + trapped) as predicted by each
family at EOM, [bottom face of the model]: (left column) FAM3; (right colum)
FAM4; . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 140
7.16 Comparing the porosity distribution among model families. All the scales are
the same. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 144
7.17 Comparing the permeability distribution among model families. All the scales
are the same. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145
7.18 The fracture intensity map of the Tensleep Sandstone B. 1-TPX-10 is the
proposed injection well. Color lines resent the average strikes of fracture sets.
Red: the hinge-parallel; yellow: the hinge-perpendicular; white: the hinge-
oblique. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148
7.19 The relative location of the CO2 plume at EOM. The background is a base
map of Teapot Dome. The arrow points to the north. . . . . . . . . . . . . 149
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7.20 The CO2 plume from one of simulation runs at the EOM. The model uses 5x
vertical exaggeration. The arrow points to the north. . . . . . . . . . . . . . 150
A.1 Digitizing Key Pillars directly on the 3D seismic data. . . . . . . . . . . . . . 157
A.2 The fault model for the geologic model. . . . . . . . . . . . . . . . . . . . . . 158
A.3 The framework that is generated by the Pillar Gridding process. The white
lines represent the faults built by fault modeling. The blue lines, which are
the framework of the model, constitute grid cells. . . . . . . . . . . . . . . . 159
A.4 The dialog of Make Horizons process. . . . . . . . . . . . . . . . . . . . . . 159
A.5 The dialog of Depth convert 3D grid. . . . . . . . . . . . . . . . . . . . . . 161
A.6 Corner Point grid cells generated by the structural modeling. . . . . . . . . . 163
A.7 The dialog of scale up well log. . . . . . . . . . . . . . . . . . . . . . . . . 165
A.8 Variogram anatomy (courtesy of Dr. Ye Zhang [169]). . . . . . . . . . . . . . 167
A.9 A vertical experimental (or sample) variogram. . . . . . . . . . . . . . . . . 169
A.10 A variogram model (blue line) is fitted to the experimental variogram. Vertical
range = 6.003 (in the red box). . . . . . . . . . . . . . . . . . . . . . . . . . 169
A.11 A variogram generated from a model with a layer thickness of 3 ft. . . . . . 170
A.12 A variogram generated from a model with a layer thickness of 9 ft. . . . . . 171
A.13 A dialog for Data Analysis process. . . . . . . . . . . . . . . . . . . . . . . 172
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List of Tables
4.1 Classification of Naturally Fractured Reservoirs (after [90]). . . . . . . . . . . 53
6.1 Symbols, units, and ranges of the uncertainty factors varied in the hierarchy
stochastic model conditioned to soft data. The azimuth angle is referenced
to East (0 degree). L1, L2, and L3 are modeling choices associated with a
categorical uncertainty factor (see the text for detail). SF=Shared factors;
FF=Family Factors; FU1=Flow Unit 1; FU2=Flow Unit 2. . . . . . . . . . 112
6.2 Symbols, units, and ranges of the uncertainty factors varied in the DFN frac-
ture models. FF=Family Factors; FS1=Fracture Set 1 (the hinge-oblique set);
FS2=Fracture Set 2 (the hinge-perpendicular set); FS3=Fracture Set 3 (the
hinge-parallel set). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 116
7.1 Significant factors identified by the PB Design for each family that impact
the prediction of the Storage Ratio (SR). Significance level = 90%; EOI: end
of injection; EOM: end of monitoring; FA: Fracture Aperture . . . . . . . . . 124
7.2 Summary of the RS error at the PB design points: Error = RS-predicted SR
- simulated SR at PB points. . . . . . . . . . . . . . . . . . . . . . . . . . . . 130
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Acknowledgments
There are many people and organizations that have provided me with support to complete
this dissertation. This support has come in the form of financial aid, encouragement, and
the sharing of their personal knowledge.
First and foremost, I wish to thank my advisor Dr. Ye Zhang for the guidance, patience,
and motivation throughout the study. Appreciation is also expressed to Dr. Shaochang Wo
for his efforts and guidance in my study, and for being a member of my Ph.D. committee.
I would like to thank Dr. Erin A. Campbell-Stone for her detailed revision suggestions for
improving my dissertation. Last but not least, I thank the rest of the Ph.D. committee:
Dr. Brian F. Towler and Dr. Subhashis Mallick for their time and input. Their insight and
suggestions have greatly improved my work and my knowledge over these past few years.
I would like to extend my appreciation to Dr. Shuiquan Li and Dr. Peigui Yin, from the
Enhanced Oil Recovery Institute (EORI) of the University of Wyoming, for their guidance
and support during this research.
I also wish to thank the professors and staff at the Department of Geology and Geo-
physics at the University of Wyoming for all of their support.
I am especially grateful to Carolyn Young from the Writing Center of the University of
Wyoming. She provided much help for my writing.
Without the Rocky Mountain Oilfield Testing Center (RMOTC), there would be no
data for analysis and inputs to the model. I would like to thank RMOTC and the U.S.
Department of Energy as the data source. I am also thankful to Schlumberger for supplying
Petrel/ECLIPSE software that were used in this study.
I express my gratitude to Chevron for an internship and financial support. I also would
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like to thank the funding source for this study, the U.S. National Science Foundation (EAR-
0838250).
Lastly, I sincerely thank my parents for their love and encouragement. Without their
continued support, my education would not have been possible.
Ye Li
University of Wyoming
January 2014
xvii
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Abbreviations
BC Boundary Condition
BHP Bottom-hole Pressure
DC Dolomit-sand-free, Cemented, dune sandstone facies
DDC Dolomit-sand-rich, Cemented, dune sandstone facies
DFN Discrete Fracture Network
DoE Design of Experiment
DUC Dolomite-sand-free, UnCemented, dune sandstone facies
EOI End Of Injection
EOM End Of Monitoring
EOR Enhanced Oil Recovery
EoS Equation of State
FF Family Factors
FMI Formation MicroImager
GCS Geologic Carbon Sequestration
IDC Interdune sandstone facies, Dolomite-sand-rich, Cemented
IDUC Interdune sandstone facies, Dolomite-sand-rich, UnCemented
LIDAR Light Imaging Detection And Ranging
MC Monte Carlo
NFR Natrually Fractured Reservoir
PB Plackett Burman
RMOTC Rocky Mountain Oilfield Testing Center
RS Response Surface
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SA Sensitivity Analysis
scCO2 supercritical CO2
SF Shared Factors
SGS Sequential Gaussian Simulation
SIS Sequential Indicator Simulation
SR Storage Ratio
TDS Total Dissolved Solids
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Chapter 1
Introduction
1.1 Overview and Motivation
Carbon dioxide is believed to be the main cause of global climate change. Due to human
activities, the level of CO2 in the earths atmosphere is rising, with severe implications for
the earths environment. To reduce the amount of CO2 entering the atmosphere, a variety
of actions have been proposed including CO2 capture from industrial sources and storage
underground. This disposal option is called geostorage or Geologic Carbon Sequestration
(GCS) [1]. Injection of supercritical CO2 (scCO2) into deep permeable formations (aquifers)
of mature sedimentary basins is proposed as the most viable approach [2] [3] [4]. The best
candidate formations include unminable coal seams, depleted oil and gas reservoirs, and deep
saline aquifers. This study addresses the fundamental assessment issues in the last category.
In such settings, a variety of physiochemical processes can contribute to CO2 entrapment
and storage. Depending on host rock and fluid characteristics, different trapping mechanisms
dominate at increasing time scales, i.e., cap-rock trapping (or structural & stratigraphic
trapping), residual trapping, dissolution (or solubility trapping), and reaction with solid
matrix (or mineral trapping) (Figure 1.1).
By trapping mechanisms, we mean any chemical or physical processes through which
CO2 can be stored in a geologic environment such that it is unlikely to escape. The efficiency
of long-term storage in permeable formations is directly related to each of the trapping
1
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Figure 1.1: A schematic diagram of the general contributions of different CO2 trappingmechanisms over time (after [5]).
2
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mechanisms involved. There are four major trapping mechanisms [6] (Figure 1.1). During
the injection phase, a plume of supercritical CO2 (scCO2), which is injected into a deep
aquifer, may migrate upwards driven by buoyancy, and structural & stratigraphic trapping
are the main contributors preventing the scCO2 from escaping to the surface [7]. During
injection, scCO2 moves through the formation and displaces the resident brine. However,
as it continues to migrate (i.e., after injection ceases), brine will start to replace scCO2 in a
process called imbibition, leaving some scCO2 trapped in the pores by capillary forces. This
is called residual trapping. Over time, scCO2 dissolves into formation brine and becomes
either immobilized (if the velocity of the aquifer flow is negligible) or is carried away down
hydraulic gradients if the aquifer flow is significant [6] [8] [9]. Mineral trapping is considered
the safest long-term mechanism to sequestrate CO2, as it transforms it into an immobile
solid; however, this process can be very slow, which may take millennia [10] [11]. Clearly,
the dominant CO2 trapping mechanism can change with time.
Supercritical CO2 is lighter than formation brine and will rise under buoyancy from the
point of injection. Since the success of geostorage depends on whether significant leakage
will develop in a site evaluation, it is critical to understand both the storage efficiency of
the injected scCO2 and the extent of lateral and vertical migration. At a given storage site,
both the storage efficiency of the CO2 in the subsurface and its potential leakage back to
the surface are the key performance outcomes to be considered. Because we cannot conduct
a pilot test directly in the field, at Teapot Dome and many potential sites, to evaluate CO2
geostorage because of the large cost and time requirements, mathematical modeling and
simulation are the focus of this study.
To evaluate CO2 geostorage, mathematical modeling of CO2 flow in a storage reser-
voir provides an essential quantitative tool. It lies at the heart of every GCS assessment
study; thus to date, numerous simulation studies have been conducted to model CO2 flow
in a variety of settings [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] [8] [25] [26].
Depending on the study objective, assumptions are often employed in terms of model for-
mulations, constitutive relations, and parameterizations of the subsurface environment. In
particular, aquifer homogeneity is often assumed at various scales, which is constrained by
3
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the quality and accessibility of site-specific data. However, permeability heterogeneity is
the rule rather than exception in natural aquifers [27]. It exerts important controls on CO2
migration [28] [29] [30], while studies also suggest that models incorporating high-resolution
heterogeneity are required to accurately assess the various storage mechanisms [31] [6] [32].
However, heterogeneity in simulations is frequently generated with stochastic algorithms
subject to a range of limitations, e.g., smoothness and statistical homogeneity are common
artifacts as opposed to preferential flow paths and non-stationarity exhibited by natural
aquifers. In modeling geostorage, it is thus desirable to incorporate both high-resolution and
geologically realistic heterogeneity. On the other hand, because of the homogeneity assump-
tion, effective parameters are routinely used in modeling field injections, and a fundamental
question remains: what is the impact of effective parameterizations (alternatively, the unre-
solved heterogeneity) on model predictions of CO2 flow and its storage efficiency? To answer
this question, detailed three-dimensional permeability characterization is required. However,
in deep aquifers, information on permeability is commonly lacking. Detailed measurements,
if available, are limited to those of bore-hole data, while such sampling is often too sparse to
resolve the main heterogeneity features. Permeability is also site-specific, e.g., some faults
are fluid conduits while others are barriers [33]. Without site-specific information on per-
meability (and its spatial variation), the extent of CO2 migration subsequent to injection is
difficult to quantify.
In evaluating a storage site, reservoir simulation is performed using a geologic site model
characterizing subsurface structure, facies, and other geologic heterogeneity. However, geo-
logic carbon sequestration is frequently considered a cost center. In order to resolve de-
tailed reservoir heterogeneity, increasing subsurface characterization effort is required. The
greater the detail, the higher the cost. For the type, amount, and accessibility of data at a
given site, different geologic models can be built, ranging from simple to complex. Petro-
physical properties, for instance, can be alternatively modeled assuming homogeneity [34]
or heterogeneity [35], the latter requiring advanced modeling techniques supported by ad-
ditional and often detailed data. Although such data can be obtained from drilling and
logging the aquifer or from high-resolution geophysical surveys, extensive data acquisition
4
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is not realistic at large scales where industrial CO2 storage is concerned, due to the cost
constraint in data collection and analysis. Furthermore, potential leakage from well-bores
must be minimized, limiting the number of boreholes that can be drilled. A critical issue in
GCS is therefore to determine the right types of data to collect, and, based on these data,
the right type of model to construct, leading to a cost-effective strategy of data collection
to support the building of site models. Such models, as input to reservoir simulation, will
ideally lead to adequate, or sufficiently accurate predictions of the desired outcomes, while
models are not overly detailed and thus cost-prohibitive to construct. However, there are
many uncertainty factors in modeling that can affect CO2 migration, its storage efficiency,
and leakage, including intrinsic permeability of the geologic formation and cap-rocks, relative
permeability, and relationships between porosity and permeability. These uncertainties may
be very important for controlling CO2 storage and leakage, or they may exert only a minor
influence on these performance outcomes. Given the variety of uncertainty factors, their
range of variations, and their possible interactions, how they affect CO2 storage and leakage
and what may be the most important factors for predicting these performances outcomes
over multiple time scales remain unanswered. At a given storage site, these questions have
significant implications for the types of field and laboratory characterization data to collect,
and based on these data, the types of analysis and modeling activity that should be carried
out in a GCS assessment study.
Towards this overall objective of developing cost-effective models, this study conducts an
uncertainty analysis of CO2 storage in the Tensleep Sandstone1 at Teapot Dome, Wyoming.
Even though there are several kinds of datasets, such as seismic data, well logs, core mea-
surements, and production data, much uncertainty exists concerning the three-dimensional
(3D) porosity and permeability distributions in the Tensleep Formation because much of the
data has not been interpreted and interpolated, and data limitation/uncertainty is poorly
understood. Reservoir heterogeneity, however, is known to exist in this formation, as will
be discussed in Chapter 3. The large distances between wells, furthermore, give rise to
uncertainty as to the appropriate geologic modeling method that can capture the inter-
1the Tensleep Sandstone and the Tensleep Formation are equal and interchangeable in this thesis.
5
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well heterogeneity in this reservoir. In fact, alternative modeling methods appear equally
suitable, whereas the effect of different methods on porosity/permeability prediction and
therefore CO2 storage modeling is unknown.
The goal of this study is to understand geologic complexity in modeling CO2 storage
in the Tensleep Sandstone and the associated data needs, including both site static and
dynamic data. In modeling GCS, a variety of uncertainty factors exist, including geologic
factors influencing reservoir porosity and permeability distribution, and engineering factors
influencing gas trapping and migration. The uncertainty factors that exert the most signifi-
cant impact on CO2 predictions are of the most interest these are the factors that need to
be better characterized, reducing their uncertainties and therefore uncertainty in predictions.
In building and simulating a reservoir model, nevertheless, as more complexity is built into
it, more geologic uncertainty factors can come into play [36] [37]. To address this issue, this
study evaluates multiple conceptual Tensleep Sandstone models to determine if the list of
the most important factors (i.e., those factors whose variations have significant impact on
a prediction outcome) will change with the modeling choice. In addition, because CO2 flow
is typically dominated by viscous force during injection and gravity force during monitoring,
the list of the most important factors influencing its predictions may change over time, as well
as the uncertainty in the predictions. The study outcome will therefore be evaluated over
different time scales, i.e., end of injection and end of monitoring. Finally, a large reservoir
model is built for the storage formation for which the computational challenge in carrying
out a full uncertainty analysis is significant. This study therefore adopts the efficient Design
of Experiment (DoE) and Response Surface (RS) methodology for analyzing both parameter
importance and prediction uncertainty.
The Tensleep Sandstone at this location has significant porosity and permeability in
both the sandstone matrix and in the fracture networks that percolate through the matrix.
Ignoring each type of heterogeneity in building and simulating CO2 storage will likely lead to
biased or inaccurate CO2 predictions. However, the considerable complexity of both matrix
and fracture heterogeneity also requires to understand the level of detail that needs to be
included in building the geologic model, so resources can be used appropriately. This study
6
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explicitly models both matrix and fracture heterogeneity, and a multiple conceptual model-
ing approach is used to help understand what details are important to the prediction of CO2
flow and storage. The insights gained will help understand how fractured reservoir models
should incorporate field characterization data and how matrix and fracture heterogeneity,
which occurs over disparate scales and which exhibits distinctly different spatial correlation
structure and connectivity, should be explicitly resolved in such models. Moreover, the un-
certainty in the prediction outcomes, which propagates from both parameter and conceptual
modeling uncertainty, can be quantified to understand issues such as storage efficiency and
the leakage risk. The storage efficiency is evaluated in this work using the CO2 storage ratio,
while the leakage risk is evaluated by examining the extent of scCO2 migration and the size
of its footprint in the reservoir.
1.2 Thesis Organization
This thesis is composed of seven chapters. Chapter 1 is to introduce the overview and the
motivation of this study. Chapters 2, 3, 4, and 5 describe the modeling investigations of the
Teapot Dome. Chapters 6 and 7 describe uncertainty analysis and related results.
In chapter 2, Background and Geologic Review, parameters that affect CO2 storage
are briefly discussed. An overview of the Teapot Dome geology is presented next. The
available geologic characterization datasets are introduced.
In chapter 3, Geologic Modeling, the step-by-step geologic modeling approach of the
Tensleep Formation at Teapot Dome is introduced. A hierarchical stochastic model (for the
matrix) is built through structural modeling, facies modeling, and petrophysical modeling.
First, structural modeling is discussed, which builds the main framework of the Tensleep
Formation model and provides basic geometry of grid cells. Then, property modeling, which
normally contains two main steps, facies modeling and petrophysical modeling, is presented.
The concept of facies/flow units, which is the base of facies modeling, is introduced, fol-
lowed by reservoir characterization of the Tensleep Formation. Based on the Winland R35
method [38], the Tensleep Formation is categorized into two facies/flow units. After this
7
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categorization, a facies model of the Tensleep Formation is built through the Sequential In-
dicator Simulation (SIS) approach. Based on the facies model, the petrophysical modeling
is completed via two steps: (1) a porosity model is first built for each facies (flow units)
using Sequential Gaussian Simulation (SGS); (2) a permeability model is derived from the
porosity model based on the relationship between porosity and permeability that follows the
Winland R35 equation [38].
In chapter 4, Discrete Fracture Network (DFN) Modeling, natural fractures in
reservoir rocks and their modeling are discussed. Some basic concepts related to fractures and
naturally fractured reservoirs are first introduced. Previous fracture studies in the Tensleep
Sandstone, which provide a set of preliminary understanding of the fractures as well as
necessary data for fracture modeling, are then presented. Finally, fracture characterization
data are interpreted and discussed in detail, and a discrete fracture network model is built
based on the data.
In chapter 5, Reservoir Simulation, fluid flow simulations for modeling the migration
of the injected CO2 are presented. First, basic concepts of fluid flow simulation in naturally
fractured reservoirs, such as the dual porosity approach, and the recovery processes in frac-
tured reservoirs, are introduced. The matrix model generated in chapter 3, and the fracture
model built in chapter 4, provide essential geologic information for the reservoir flow sim-
ulation. Fluid properties, relative permeability, boundary conditions and initial conditions
are discussed. Results of a baseline simulation using representative parameter values are
presented.
In chapter 6, Uncertainty Analysis, using results of reservoir flow simulation, an
uncertainty analysis of CO2 storage in the Tensleep B Sandstone2 is conducted according
to the Design of Experiments (DoE) and Response Surface (RS) principles. An overview
of DoE methodology is, first, presented. The approaches and steps of uncertainty anal-
ysis adopted in this study are then introduced. Based on the DoE, a suite of increasingly
simplified conceptual geologic model families are created with decreasing amount of site char-
acterization data: a hierarchical stochastic model family conditioned to soft data (FAM4),
2As shown in Figure 2.5, the Tensleep B Sandstone (the B Sandstone) is the main producing formationin the Tensleep Formation and is also the proposed storage interval for the CO2 sequestration experiment.
8
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a simple stochastic facies model family (FAM3), a simple stochastic porosity model family
(FAM2), and a homogeneous model family (FAM1). Within the context of model building,
two categories of uncertainty factors, shared factors and family factors, are discussed.
In chapter 7, Results and Discussion, for the CO2 storage ratio (SR), results of the
uncertainty study are presented in 4 sections: (1) screening test outcomes; (2) Response
Surface (RS) modeling and verification; (3) Monte Carlo (MC) analysis to assess the SR
uncertainty; (4) visualization of end-member CO2 plumes and footprints. In each section,
results are analyzed at two output times: end of injection (EOI) and end of monitoring
(EOM). Implication of the study outcomes and insights obtained is summarized and dis-
cussed before future works are presented.
In appendix A, Geologic Modeling, detailed operations to build the matrix geologic
model are presented. Basic steps to build a structural model are introduced first. They
include preparing input data, fault modeling, pillar gridding, layering, and geometrical mod-
eling. Then processes of how to build a property model are presented.
In appendix B, ECLIPSE Data Files, the basic input file for ECLIPSE (the DATA
file) is attached.
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Chapter 2
Background and Geologic Review
2.1 Introduction
Although deep saline aquifers in the US can provide large storage capacities to sequester
100 years of CO2 emissions from all the coal-fired power plants [39], oil and gas reservoirs
are preferred short-term targets for Geologic Carbon Sequestration (GCS), since there are
possible cost offsets from CO2 flooding in a process termed as Enhanced Oil Recovery (EOR).
The Teapot Dome Field Experimental Facility, which is fully owned by the US gov-
ernment, has been designated to conduct carbon-storage experiments. Long-term scientific
research and technical development can be guaranteed by Federal ownership. Besides, this
field has plenty of existing static and dynamic field and laboratory characterization data, in-
cluding seismic, cores, well-logs and production data, all of which are in the public domain.
These data are the basis for characterizing and interpreting structural and stratigraphic
attributes of the subsurface reservoirs at this site [40].
In this chapter a research project of uncertainty analysis of CO2 geologic sequestration in
a fractured sandstone reservoir at Teapot Dome will be discussed. First, parameters affecting
CO2 storage are introduced. Then, the geology of Teapot Dome and available datasets will
be described.
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2.2 Parameters Affecting CO2 Storage
At the field scale, simulation of CO2 storage involves a large number of variables and pa-
rameters which govern the performance of GCS. CO2 plume migration is controlled by the
complex interplay of viscous, capillary, buoyancy forces, and reservoir heterogeneity and its
structure.
2.2.1 Reservoir Heterogeneity
Geologic heterogeneity is the rule rather than the exception in natural aquifers [27]. In oil/gas
reservoirs, heterogeneity has a strong control on the hydrocarbon displacement process [41].
Studies have concluded that heterogeneity also exerts important influences on scCO2 migra-
tion [42] [28] [29] [30], while some research suggests that models incorporating high-resolution
heterogeneity are required to accurately assess the various storage schemes [31] [6] [43]. How-
ever, heterogeneity in simulation is frequently generated with stochastic algorithms subject
to a range of limitations, e.g., smoothness and statistical homogeneity are common artifacts
as opposed to preferential flow paths and non-stationarity exhibited by natural aquifers. In
modeling geostorage, it is thus desirable to incorporate both high-resolution and geologically
realistic heterogeneity. However, in deep aquifers, information on detailed heterogeneity is
commonly lacking. Detailed measurements, if available, are limited to well data, while such
sampling is often too sparse to resolve the main heterogeneity features. Without site-specific
information on permeability (and its spatial variation), the extent of the scCO2 plume sub-
sequent to injection is difficult to quantify.
2.2.2 Fluid Flow Properties
Other sources of uncertainty also exist in simulating deep injection, further contributing to
the predictive uncertainty of a modeling study. In particular, under supercritical conditions,
the fluid phase relative permeabilities (one for brine; one for scCO2) are highly uncertain.
The relative permeability of scCO2-brine systems determines CO2 injection, migration, and
the immobile CO2 due to irreducible saturation in pore space [44]. Therefore, it is a key
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Figure 2.1: The hysteresis effect of relative permeability for CO2-brine (data from [49]).
parameter in numerical simulations to predict CO2 storage [45].
Recent experiments have demonstrated hysteresis effects on the relative permeability
of scCO2-brine system between the drainage and imbibition curves [44] [46] [47]. Hysteresis
refers to irreversibility, or directional saturation phenomena as exhibited by the relative
permeability and capillary pressure when a given phase saturation is increased or decreased
[6] [48]. This phenomenon is illustrated by Figure 2.1.
A saline aquifer is a medium that is initially filled with water, and it is water wet.
During CO2 injection into the aquifer, the scCO2 is a non-wetting phase, and it follows
the drainage curve of the scCO2-brine relative permeability to invade the pore space. This
is a drainage process in which the CO2 is in the form of a continuous, connected cluster.
After CO2 injection, water displaces scCO2 under capillary pressure as water is the wetting
12
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Figure 2.2: A Teapot Dome location map. The field is located within T. 38 - 39 N., R. 78W. (courtesy of RMOTC [52]).
phase. The scCO2 will follow the imbibition curve of the relative permeability. During this
imbibition process, scCO2 gets disconnected in the form of blobs or ganglia. It is, therefore,
trapped as an effectively immobile phase [6].
2.3 Geology of Teapot Dome
The Teapot Dome oil field, also known as Naval Petroleum Reserve No.3 (NPR-3), is the
last United States government owned oil field [50]. It is 30 mi north of Casper, Wyoming,
and located at the southwestern edge of the Powder River Basin (Figure 2.2) [51]. The field
covers nearly 10,000 acres [50].
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Figure 2.3: The location of the Teapot Dome field, Tensleep structure depth, and the pro-posed CO2 injection well. Structural relationship between Teapot Dome and Salt Creekfields (after [54]).
Teapot Dome is an elongated asymmetric, doubly plunging, basement-cored, Laramide-
age anticline, which has a north-northwest axis [51]. It is considered as an extension of the
larger Salt Creek anticline, with the Salt Creek anticline to the north and the Sage Spring
Creek and Cole Creek oil fields to the south (Figure 2.3) [53].
Teapot Dome, a basement-cored anticline, is one of several productive hydrocarbon
structural traps within the Rocky Mountain region. The same types of structures can be
found in many other areas around the world [55] [56] [51]. As basement-cored anticlines can
provide excellent four-way closure, which can trap a significant amount of hydrocarbons,
they become exploration targets. Permeability anisotropy associated with such structures
directly controls final recovery of these trapped hydrocarbons [56].
14
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2.3.1 Structural Elements
Teapot Dome is a SW-verging anticline that has steep dips (20-50) on the west flank and
shallow dips (
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Figure 2.4: Teapot Dome Geologic Column (after RMOTC [60]).
Pennsylvanian Tensleep Sandstone with the overlying Goose Egg Formation is discussed in
the following because Tensleep has been chosen as the first reservoir target for the proposed
CO2 injection experiments, i.e. the target CO2 storage reservoir in this research.
The Tensleep Formation (The Tensleep Sandstone)
The Pennsylvanian Tensleep Formation covers a large extent in Wyoming, Montana, and
Colorado and is the most promising target for CO2 storage, because of its enormous volume.
The Tensleep Formation is a thick, continuous, porous and permeable eolian sandstone con-
taining oil or brine [50]. The Tensleep in the Lost Soldier and Wertz Fields in Wyoming
and its equivalent formation, Weber Sandstone, at Rangely field in Colorado have accommo-
dated injected CO2 as part of an Enhanced Oil Recovery method for roughly 20 years. The
Tensleep Sandstone, which holds two thirds of Wyomings oil, is an important producing
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unit in Wyoming [59].
Through study of analogs, Zhang [61] concluded that the Tensleep Sandstone consists
of multiple sequence boundaries as a result of frequent and high-amplitude sea level changes.
Zhang also stated that generally from bottom to top, the Tensleep Sandstone changes from
dominantly marine, with abundant crinoids and corals, thick tabular carbonate beds and
thick sandstone layers, to dominantly terrestrial, with thick eolian cross-bedded sandstones,
scarce fossils, and thick and discontinuous carbonates.
Zhang [61] stated that the Tensleep Sandstone comprises thick-bedded porous and per-
meable eolian deposits with average porosity of 8% and 80 mD average permeability. Sabkha
and shallow marine dolomites, interbedded with these eolian deposits, are thin but form
widespread extensive beds. Due to their low permeability, the dolomites act as flow baffles
or barriers. Although many vugs, fractures and stylolites are observed in dolomites, such beds
do not constitute permeable reservoir because of extremely low permeability. Sandstones,
the reservoir rocks, are separated in several intervals by these extremely low permeability
dolomites. As shown in Figure 2.5, the B Sandstone (the Tensleep B Sandstone) is the
main producing formation and is also the proposed storage interval for the CO2 sequestration
experiment [61] [50].
The Tensleep Sandstone at Teapot Dome are divided into the lithofacies of eolian dune,
interdune, and sand sheet, which are comprised of fine- to very fine-grained, quartz arenites,
with local concentration of dolomite sand grains. Lamination and grain size vary widely as a
function of the depositional environment. Porosity and permeability are therefore determined
by both the depositional units and the degree of cementation and compaction, which further
aggravate reservoir heterogeneity [62].
The Permian Phosphoria Formation, which is locally called the Goose Egg Shale, overlies
the Tensleep Sandstone as a cap rock. It is the regional seal of the Tensleep Formation across
Wyoming [50]. At the Teapot Dome field, the Goose Egg Formation comprises over 300 ft
of shale, carbonate, and anhydrite. More than 35 million barrels of oil and dissolved gas
has been trapped under this seal at Teapot Dome, indicating good evidence of its long term
sealing effectiveness [50].
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Figure 2.5: A schematic stratigraphic column of reservoir (Tensleep Fm.) and the caprock(Goose Egg Fm.) (after [63] and [62]).
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Figure 2.6: Cores from the Teapot Dome show fractures (courtesy of RMOTC [64]).
Fractures
At the Teapot Dome, both core data and outcrops indicate that the Tensleep Sandstone
contains well developed natural fractures. Fractures provide substantial permeable pathways
in these eolian sandstone reservoirs, which form dual porosity networks that are challenging
to characterize and integrate into reservoir modeling and numerical simulations. A more
detailed discussion will be presented in chapter 4 that will describe the process of building
a Discrete Fracture Network (DFN) model.
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2.4 Geologic Characterization Datasets
Teapot Dome covers nearly 10,000 acres with more than 2,200 wells, about 1,200 of which may
be accessed by public. About 600 of those total 2,200 wells are producing, and more than 400
have depths greater than 2,700 ft. Importantly, public-domain databases exist at the Teapot
Dome field. These databases include cores, well logs, mud logs, completion descriptions, and
production data. These data are fundamental to our effort of characterizing the structural
and stratigraphic attributes and reservoir heterogeneities at the subsurface [54].
2.4.1 Seismic Data
A set of full-field three-dimensional (3D) seismic data was acquired by the Rocky Moun-
tain Oilfield Testing Center (RMOTC), which is colocated with the Department of Energy
(DOE)s office that manages and operates Teapot Dome. This set of 3D seismic data, con-
sisting of 345 in-lines and 188 cross-lines with a bin size of 110 ft, is also in the public
domain [54].
A post-stack migrated volume was interpreted in time-domain by EXCEL Geophysical
Services Company in Denver, Colorado [65]. The interpreted horizons include the tops for
the Second Wall Creek formation (KF2), Fall River formation (Dakota), Lakota/Morrison
formation, Crow Mountain formation, Red Peak formation, Tensleep formation, and Precam-
brian basement. This seismic dataset also includes 2D seismic data, synthetic seismograms,
and time-depth tables. However, it does not include the interpretations of faults.
2.4.2 Core Data
There are about 35 wells that have penetrated the Tensleep Sandstone at Teapot Dome,
including 13 cored wells [54]. Sedimentary attributes and fractures have been characterized
for a subset of the cores. Porosity and permeability are tested from core samples and provide
limited information on the subsurface at the well locations. Petrophysical characterizations
and lithofacies descriptions have been carried out based on these core data [62] [64].
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2.4.3 Well Data
The 35 wells, which have penetrated the Tensleep Sandstone, all have traditional well-log
suites that have been digitized. Most of these well-log suites contain spontaneous potential
logs, resistivity logs, gamma ray logs, and porosity logs including sonic logs, density logs,
and neutron logs [60].The well-log dataset includes well headers, directional surveys, and
formation log tops, all of which are basic well data used to build geologic model of this
study.
Six recent wells have FMI (Formation Micro Imager) logs [64], which can be used to
characterize reservoir fractures (induced, open and seal) at the in-situ condition. FMI can
also be used to interpret dune cross-bedding orientations [66].
2.4.4 Outcrop Analogs
Outcrops supplement sparse subsurface data with outcrop-derived measurements. The Tensleep
Sandstone outcrops in the nearby Alcova anticline were studied in [67]. LIDAR (Light Imag-
ing Detection and Ranging), which has the ability to detect fracture planes with area 1 m2,
was adopted to characterize natural fractures in the Alcova anticline. Some key parameters,
like fracture dip, fracture azimuth, fracture spacing, and fracture height-to-length aspect
ratio, can be determined by fracture data extracted from the LIDAR dataset [67].
2.4.5 Production Data
The production data demonstrates that the Tensleep Sandstone is under strong water drive
[65]. In other words, the Tensleep Sandstone connects to a large aquifer. These data provide
a clue to the boundary condition (BC) of this reservoir.
2.5 Summary
In this chapter, we have presented an introduction to the background of Geologic Carbon
Sequestration (GCS), as well as parameters that affect GCS, and an overview of Teapot
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Domes geology. The understanding and the dataset related to Teapot Domes geology are
the basis for modeling, which will be discussed in detail in the next chapters.
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Chapter 3
Geologic Modeling
3.1 Introduction
The geologic model is also designated as the static (reservoir) model (in the oil industry,
it is also referred to as the reservoir model), because it is built on static data, such as
geological, geophysical, and petrophysical measurements and for example, well logs, core
measurements, and seismic data, etc. These data are constant and do not vary with time.
In contrast, dynamic data varies with time, like fluid saturations, bottom-hole pressure
(BHP) and formation pressure. The flow (reservoir) simulation model is also referred to as
the dynamic model that is utilized to simulate behavior of dynamic data over time.
In the lifetime of an oil field, models play a crucial and fundamental role in understand-
ing and predicting reservoirs characteristics and performance. A model is a quantitative
digital representation that incorporates every available piece of information from diverse
data sources, such as geology, geophysics, petrophysics, and engineering, to maximize the
value of these data.
The objective of model studying is to provide one or several alternative models that rep-
resent the spatial variation of geologic properties, such as facies, porosity, and permeability.
Models can normally be built by two distinct approaches: deterministic and stochastic. The
former one can provide only one definite model whereas the latter one can produce different
equiprobable static reservoir models, or different realizations [68].
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A geologic model (static model) integrating large amounts of data delivers basic input
to a flow simulation model (dynamic model). Flow simulation models based on stochastic
geological models can produce a distribution of predictions, and this procedure transfers
uncertainties from geological models to fluid flow predictions [69]. Therefore, through eval-
uating simulation outcomes, i.e., CO2 storage performance metrics, uncertainties during
modeling and simulation can be assessed.
3.2 Static Site Model
A model is a simplified representation of some aspects of the subsurface reality. As modeling
is always about simplifications, we will only focus on the important ones [70]. It is widely
believed that reservoir models can only mimic reality, not reproduce reality [71].
This chapter describes the step-by-step geologic (static site) modeling approach of the
Tensleep Formation at Teapot Dome in Wyoming. A hierarchy stochastic model is built
through processes of structural modeling, facies modeling, and petrophysical modeling.
3.2.1 Structural Modeling
The structural model describes the main framework of the Tensleep Formation at Teapot
Dome, and it provides basic geometry of grids (or cells). These grids are assigned with facies
or petrophysical attributes by following a property modeling process.
Fault Modeling of the Tensleep Sandstone Fault modeling is a procedure to generate
faults in the Tensleep Formation. The purpose of this process is to define the shape of each
fault that can be conditioned on data, such as seismic interpretation and cross section. [70].
Faults can be digitized directly on seismic data. In this study, faults were interpreted
based on the post-stack migrated 3-D seismic data. Although Petrel provides an Automatic
fault extraction function, it did not work well with the Teapot Dome data and the result was
disappointing. We had to interpret faults manually. Following previous interpretation and
information (Figure 3.1, Figure 3.2), five faults were interpreted, including a west bounding
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Figure 3.1: An arbitrary cross-section through Teapot Dome (left). A depth-structure mapon the 2nd Wall Creek Sandstone (right) showing location of cross section line (after [40]).
thrust fault (Figure 3.3).
Structural Modeling of the Tensleep Sandstone Well logs and 3D seismic interpreta-
tions at the Teapot Dome were integrated at the regional scale to obtain formation horizons
for the Tensleep Sandstone: Tensleep A Sandstone, and Tensleep C1 Dolomite (Figure 3.4).
The horizons are truncated to the west by the thrust fault. In creating the horizons, seismic
interpretations from RMOTC dataset were utilized and were constrained by well tops along
formation contacts. Based on the horizons, a 3-D structural model of the Tensleep Sandstone
was built, spanning an average thickness of approximately 100 ft. (For detailed procedures
to build this structural model please refer to Appendix A).
The completed structural model contains 18532280, total 4, 765, 600 grids with an
average grid spacing of 90 ft in the I direction, 90 ft in the J direction, and 3 ft in the
K direction. In the next step (Property Modeling), these grids will be assigned geologic
attributes to characterize reservoir heterogeneity.
During structural modeling, most of the data we used, such as the seismic data, the
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Figure 3.2: An amplitude map of the Tensleep Sandstone at Teapot Dome. Basement-coredfaults are shown (after [66]).
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Figure 3.3: The fault model of the Tensleep Sandstone at Teapot Dome and 3D seismicdata (in the time domain). Each colored surface with sticks represents a fault interpretedaccording to 3D seismic data manually. The model uses 5x vertical exaggeration. The arrowpoints to the north.
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Figure 3.4: The structural model of the Tensleep Sandstone. Depth is in feet at subsealevel(in the depth domain). Negative value is below sea level. Colored points represent welltops. The model uses 5x vertical exaggeration. The arrow points to the north.
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interpreted faults and horizons, and well tops, are in some sense definite (i.e., in this research,
it is assumed that there is no uncertainty in these data). Therefore, the structural model,
or structural-stratigraphic model, is sometimes referred to as a deterministic model.
Structural models are traditionally built based on consolidating data from well logs,
cross sections, and isopach maps. As cross sections and isopach maps are commonly created
from limited data, the accuracy and resolution of such data are not definite. Furthermore,
even though well data often have high resolution, the interpolation approach has to be
used to derive inter-well information because of a small support volume of well data. The
3-D seismic data for this research can characterize elementary structural information with
enough resolution, such as faults, horizons, and boundaries. Thus, the structural model based
on such 3-D seismic data provides the most accurate possible framework of the Tensleep
Sandstone, and grid geometry for the following property modeling.
3.2.2 Property Modeling
The property model is a process with which attribute values, discrete or continuous, are
populated into every grid cell of the structural model. It typically includes two main steps:
facies modeling and petrophysical modeling.
Facies/Flow Units In geology, a facies is a body of rocks with a set of specified character-
istics [72]. In modeling, facies has various definitions: for example, lithofacies, or lithology,
is used to define a depositional environment and/or a type of deposit; electrofacies indicates
log responses which characterize and differentiate different layers; seismic facies is the sum of
seismic attributes; petrophysical facies describes homogeneous petrophysical behavior (static
and dynamic); rock-type in reservoir engineering corresponds to a numerical expression of
elementary dynamical petrophysical grouping after homogenization [73].
Traditional discrimination of rock types is based on subjective observations; neverthe-
less, permeability can change by several orders of magnitude within a given rock type. This
means that even if we can have explicit lithofacies classification over the entire reservoir, it
cannot be utilized in reservoir simulation, because it is not able to characterize permeability
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distribution that is critical to the effective description of a reservoir.
The concept of flow units that integrate geologic and engineering data into a system
for reservoir descriptions is proposed in [74]. A flow unit is defined as the representative
volume of total reservoir rock within which geological and petrophysical properties that
affect fluid flow are internally consistent and predictably different from properties of other
rock volumes (i.e., flow units). [74] Thus, a flow unit is a reservoir volume in which fluid flow
has similar characteristics and is continuous laterally and vertically [75]. According to [74],
Flow units are defined by geological properties, such as texture, mineralogy, sedimentary
structures, bedding contacts, and the nature of permeability barriers, combined with quan-
titative petrophysical properties, such as porosity, permeability, capillarity, and fluid satu-
rations. [74] Flow units do have some relation to geologic facies but are not consequentially
consistent with facies boundaries. Studies in the subsurface and in surface outcrops also
support the notion that flow units do not always coincide with geologic lithofacies [74]. At
the microscopic scale, pore-throat attributes control fluid flow. The pore geometry is in turn
controlled by geologic properties. Flow units, which are generated by various associations
of these geologic properties, will have similar fluid flow properties. Hence, a flow unit can
contain several geologic facies types, depending on their depositional texture, mineralogical
constituent, and sedimentary structures [76] [77].
The flow unit can be utilized to divide a reservoir into appropriate zones that approxi-
mate the architecture of the reservoir at a scale that is consistent with reservoir simulations.
Therefore, critical geologic information can be incorporated into reservoir simulation with-
out greatly complicating the models [74]. After building the geologic model, the flow unit
is considered a better choice than other facies type for numerical reservoir simulation. Thus
we will use flow units to create the facies model. In the following chapter, facies is used
interchangeably with flow unit. In some literature, flow unit is also termed as hydraulic
(flow) units.
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Reservoir Characterization of Tensleep Sandstone
Reservoir Characterization of the Tensleep Sandstone Several geologists studied the
Tensleep Sandstone based on texture, mineralogy and sedimentary structure, and concluded
that it was deposited in both eolian and marine environments [78] [79] [80] [81].
Outcrop and subsurface studies show that the Tensleep Sandstone contains interbedded
eolian sandstone, marine sandstone and dolomitic sandstone. Sea level fluctuation caused
this cycle phenomena. Eolian sandstones are formed at low sea level and dolomitic sandstones
are created when the sea level rises [82] [80].
In general, every para-sequence in the Tensleep Sandstone can be divided into two units:
the lower and the upper. Marine facies dominate the lower unit while eolian facies prevail
over the upper unit. Normally, tabular-planar cross-bedding in eolian dune sandstone facies
indicates high-porosity and high-permeability zones, whereas eolian interdune facies, shore-
face/foreshore marine sandstone facies, normal marine carbonate and its equivalent dolomitic
sandstones are zones of low porosity and permeability. Nevertheless, depositional textures
and diagenetic modifications cause the eolian sandstones to be surprisingly heterogeneous.
Additionally, natural fractures make this heterogeneous situation more complex [62] [80].
As mentioned before, reservoir lithofacies in the Tensleep Sandstone can be divided into
eolian dune, inter dune, and sand sheet. Porosity and permeability change with depositional
environments. Furthermore, cementation and compaction affect the porosity and perme-
ability to intensify the heterogeneity of the reservoir. Cements in the Tensleep Sandstone
are mainly micro-crystalline dolomite and anhydrite, which can reduce porosity and cause
anisotropic permeability. Dolomite sand grains are ductile and can be distorted under me-
chanical compaction to destroy porosity and permeability as a result of the filling of the
inter-granular space. Considering this diagenetic modification, the Tensleep Sandstone is
classified into six petrophysical facies: (1) uncemented, dolomite-sand-free, dune sandstone
facies (DUC), (2) cemented, dolomite-sand-free, dune sandstone facies (DC), (3) cemented,
dolomite-sand-rich, dune sandstone facies (DDC), (4) uncemented, dolomite-sand-rich, inter-
dune sandstone facies (IDUC), (5) cemented, dolomite-sand-rich, interdune sandstone facies
(IDC), and (6) cemented, dolomite-sand-rich sand sheet facies [62] (Figure 3.5).
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(a) DUC (b) DC
(c) DDC (d) IDUC
(e) IDC (f) Sand Sheet
Figure 3.5: Plain-light thin-section images of different petrophysical facies of the TensleepSandstone (courtesy of Dr. Peigui Yin [62]).
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According to the above petrophysical facies classification, core data from the Tensleep
well 54-TPX-10 have been characterized in [62], as shown in Figure 3.6, which measured and
plotted porosity and permeability of each petrophysical facies from the Tensleep interval
(Figure 3.7).
The work from [62] indicates that the distributions of petrophysical properties between
facies are different and there is a intimate correlation between facies and petrophysical prop-
erties. In addition, there are overlaps among cemented, dolomite-sand-free, dune sand-
stone facies (DC), cemented, dolomite-sand-rich, dune sandstone facies (DDC), uncemented,
dolomite-sand-rich, interdune sand facies (IDUC), and cemented, dolomite-sand-rich, inter-
dune sandstone facies (IDC). In other words, the distributions of petrophysical properties
are not unique in some facies. Hence, flow units are adopted as an approach to characterize
facies of the Tensleep Sandstone.
Flow Units of the Tensleep Sandstone
If there is sufficient core description, such as the work in [62], we could categorize them
according to the classification of facies from [62] and build a facies model based on them.
However, we just have one well having such petrophysical facies classification. Even though
we have well log data, they could not yield an accurate clue to lithofacies or petrophysical
facies. Although Petrel provides a neural network tool to help classify well log data, it
does not lead to any satisfying results. Although the results are similar compared to the
petrophysical facies classification based on cores in [62], they are not accurate enough. As our
research is about uncertainty of modeling, we do not want to bring some extra uncertainties,
and need a definite facies classification. As a result, flow unit is chosen as an approach to
classification of facies.
Because rock types are classified according to petrophysical properties which pertain
to fluid behavior such as porosity, permeability, capillary pressure, and saturation [83], rock
types and flow units are similar because both of them are classified by properties important
to fluid flow. Therefore, we can borrow a category method from rock types to classify flow
units. There are different methods to classify rock types: for example, K-Phi cross plot;
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Figure 3.6: Distribution of petrophysical facies of the Tensleep Sandstone interval of well54-TPX-10 and comparisons to well logs (courtesy of Dr. Peigui Yin [62]).
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Figure 3.7: Plot of porosity vs. permeability for different facies of the Tensleep Sandstone(data from Dr. Peigui Yin).
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Winland method; Pittman method; and rock quality index(RQI) [84].
The Winland equation, or Winland R35, is a method to calculate pore-throat radius
using core porosity and permeability measurements. The R35 of a given rock type not only
can reflect depositional and diagenetic texture, but it can also impact fluid flow [38]. As
a result, R35 estimated from core or well logs, can be utilized to categorize zones that can
be used by both geologists and reservoir engineers. This approach is ideally suited to our
research, because the Tensleep Sandstones porosity and permeability varies with different
depositional environments and are further modified by diagenetic processes. And reservoir
simulation, which describes fluid flow in a reservoir, will be run based on a 3D geologic model
of the Tensleep Sandstone. As our research includes both geologic modeling and fluid flow
simulation, an approach that can be used in both procedures is preferred. Consequently, the
Winland equation is adopted to classify facies of the Tensleep Sandstone.
The Winland equation depicts an empirical relationship among porosity, permeability,
and pore aperture radius corresponding to the 35th percentile of mercury saturation for a
mixed suite of sandstones and carbonates. The equation is as following:
logR35 = 0.732 + 0.588 logKair 0.864 log (3.1)
where R35 is the pore aperture radius corresponding to the 35% mercury saturation,
Kair is the uncorrected air permeability (in mD), and is porosity (in %) [85] [86].
There are 12 wells that contain porosity and permeability data derived from laboratory
core tests. After a quality check, 11 wells were designated to be used in classifying flow
units. These have similar and predictable fluid flow characteristics respectively. Two flow
units with different reservoir performance are distinguished by the ranges of R35.
(1) Flow unit 1 is defined as having an R35 ranging above a threshold of 0.85 m. This
kind of flow unit corresponds to high-porosity and high-permeability zones where fluid can
easily flow.
(2) Flow unit 2 has an R35 less than 0.85 m. Such flow units correspond to a low-
porosity and low-permeability location where there are normally tight reservoirs or non-
reservoirs.
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Figure 3.8: Comparison between flow units and petrophysical properties of the plot in Fig-ure 3.7.
We compared this flow unit category to the petrophysical facies based on cores in [62],
as shown in Figures 3.8 and 3.9 .
The black line in Figure 3.8 represents R35 = 0.85. The facies of the points above this
black line are flow unit 1; the ones below this line are flow unit 2. Almost all uncemented,
dolomite-sand-free, dune sandstone facies (DUC), and some of the cemented, dolomite-sand-
free, dune sandstone facies (DC) belong to flow unit 1, whereas almost all interdune fa-
cies (uncemented, dolomite-sand-rich, interdune sandstone facies (IDUC), and cemented,
dolomite-sand-rich, interdune sandstone facies (IDC)), cemented, dolomite-sand-rich, dune
sandstone facies (DDC), and some part of cemented, dolomite-sand-free, dune sandstone fa-
cies (DC) are attributed to flow unit 2. This indicates that flow units do have some relation
with petrophysical facies, but are not absolutely consistent with them. This also testifies the
statement in [74] that flow units do not always coincide with geologic lithofacies [74].
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Figure 3.9: Comparison between petrophysical facies in [62] and flow units derived in thisstudy.
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The Relationship between Porosity and Permeability The relationship between
porosity () and permeability (k or log k) is traditionally assumed to be linear. This assump-
tion is simply based on observation. However, approaches from experiments, for instance the
Winland equation, do not illustrate that permeability is a linear function of porosity. Flow
units