stereological interpretation of rock fracture traces …...stereological interpretation of rock...
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Stereological Interpretation of Rock Fracture Traces on
Borehole Walls and Other Cylindrical Surfaces
Xiaohai Wang
Dissertation submitted to the Faculty of the
Virginia Polytechnic Institute and State University
in partial fulfillment of the requirements for the degree of
Doctor of Philosophy
in
Civil Engineering
Mauldon, Matthew, Chair
Dove, Joseph E.
Dunne, William M.
Gutierrez, Marte S.
Westman, Erik C.
September 16, 2005
Blacksburg, Virginia
Keywords: fractures, cylindrical sampling, borehole, stereology, Monte Carlo method, intensity measures, conversion factors, mean fracture length and width
Copyright 2005, Xiaohai Wang
Stereological Interpretation of Rock Fracture Traces on Borehole Walls and Other Cylindrical Surfaces
Xiaohai Wang
Abstract
Fracture systems or networks always control the stability, deformability, fluid and gas
storage capacity and permeability, and other mechanical and hydraulic behavior of rock
masses. The characterization of fracture systems is of great significance for
understanding and analyzing the impact of fractures to rock mass behavior. Fracture
trace data have long been used by engineers and geologists to character fracture system.
For subsurface fractures, however, boreholes, wells, tunnels and other cylindrical
samplings of fractures often provide high quality fracture trace data and have not been
sufficiently utilized. The research work presented herein is intended to interpret fracture
traces on borehole walls and other cylindrical surfaces by using stereology. The
relationships between the three-dimension fracture intensity measure, P32, and the lower
dimension fracture intensity measures are studied. The analytical results show that the
conversion factor between the three-dimension fracture intensity measure and the two-
dimension intensity measure on borehole surface is not dependent on fracture size, shape
or circular cylinder radius, but is related to the orientation of the cylinder and the
orientation distribution of fractures weight by area. The conversion factor between the
two intensity measures is determined to be in the range of [1.0, π/2]. The conversion
factors are also discussed when sampling in constant sized or unbounded fractures with
orientation of Fisher distribution. At last, the author proposed estimators for mean
fracture size (length and width) with borehole/shaft samplings in sedimentary rocks based
on a probabilistic model. The estimators and the intensity conversion factors are tested
and have got satisfactory results by Monte Carlo simulations.
iii
Acknowledgments
I am indebted to the assistance of my dissertation committee: Dr. Matthew Mauldon, Dr.
Joseph E. Dove, Dr. William M. Dunne, Dr. Marte S. Gutierrez, and Dr. Erik C.
Westman. From my proposal to the final form of this dissertation, they have given great
amount of valuable suggestions and made the study in this Ph.D. program priceless
experience to me.
My advisor, Matthew Mauldon, whom I met two weeks after I arrived at this country,
generously provided the support for me to enroll as a Ph.D. student. In the passed four
years, he and his insights had showed me many times the lights of the way and lead me
out of the darkness of confusion and uncertainty. Though, what I have learned from him
is far beyond what I can put in words. I Thank Matthew, his wife Amy and their
daughters for their kindness and support.
Special thanks to Dr. Dunne and his student Chris Heiny in the University of Tennessee.
The collaborations with them on fracture size estimators pushed the dissertation to a new
level. Their work and suggestions as geologists have made the estimators more practical
and useful.
I also owed thanks to Jeremy Decker of Virginia Tech, who helped me testing my
program and carrying out numerous simulations. I always regret that I can not include in
my dissertation the great figures he worked out in Matlab.
I am grateful to have my friends around me in the years in Ozawa library and Rm19,
Patton Hall. My colleagues’ consideration and thoughtfulness makes the days and nights
in the office wonderful memory.
Last, but not least, I am beholden to my wife Hui Cheng, her family and my family in
China. Without their great love, this dissertation is impossible.
iv
Contents
Acknowledgments .........................................................................................iii
1 Introduction..................................................................................................1
2 Multi-dimensional intensity measures for Fisher-distributed fractures ......3
2.1 Introduction ............................................................................................................3
2.2 General form of conversions ..................................................................................4
2.3 Linear and planar sampling of fisher-distributed fractures.....................................7
2.4 Sampling on a cylindrical surface ........................................................................14
2.5 Example: 3-d fracture intensity inferred from scanline data ................................19
2.6 Discussion and Conclusions .................................................................................22
Acknowledgments ......................................................................................................22
Appendix 2.A Probability density function (pdf) )(αΑf of angle α ........................23
Appendix 2.B Numerical approach for obtaining FΑ(α) and FΒ(β) ...........................27
References...................................................................................................................28
3 Estimating fracture intensity from traces on cylindrical exposures ..........31
3.1 Introduction ..........................................................................................................32
3.2 Basic assumptions.................................................................................................35
3.3 General form of the relationship between areal intensity P21,C and volumetric
intensity P32 for right circular cylinders ..................................................................36
3.4 General case of cylindrical sampling....................................................................38
3.5 Special case: Sampling fractures of constant orientation .....................................42
3.6 Special case: fractures with uniform orientation distribution...............................45
3.7 Cycloidal Scanline Technique ..............................................................................47
3.7.1 Unbiased sampling criterion........................................................................47
3.7.2 Cycloidal scanlines......................................................................................50
3.8 Monte Carlo Simulations......................................................................................50
v
3.9 Discussion & Conclusions....................................................................................54
Acknowledgements.....................................................................................................55
Appendix 3.A Determine |cos γ| .................................................................................56
References...................................................................................................................59
4 Estimating length and width of rectangular fractures from traces on
cylindrical exposures ............................................................................62
4.1 Introduction ..........................................................................................................63
4.2 Assumptions .........................................................................................................67
4.4 Probabilistic model for occurrence of intersection types .....................................71
4.4.1 w′ > D ..........................................................................................................77
4.4.2 w′ ≤ D ..........................................................................................................79
4.4.3 Summary of fracture length and width estimators ......................................84
4.5 Examples ..............................................................................................................86
4.6 Monte Carlo simulations ......................................................................................90
4.7 Discussion & Conclusions....................................................................................96
References...................................................................................................................98
5 Conclusions and discussions....................................................................103
6 Appendix: Programs used in the dissertation ..........................................106
A. FISHER - Simulate the Fisher distribution.........................................................106
B. TRACE - Simulate fracture population sampled by a borehole ..........................107
7 Vita...........................................................................................................111
vi
List of Figures
Fig. 2.1. Geometry of linear and planar sampling of a fracture.......................................... 5
Fig. 2.2. For an isotropic fracture orientation distribution, the distributions of α and β are
proportional to the sin α and sin β, respectively. ................................................. 7
Fig. 2.3. Spherical triangle formed by n, m, and s, where n is fracture normal, m is
Fisher mean pole, and s is the sampling line....................................................... 9
Fig. 2.4. Fisher-distributed fracture normals in relation to sampling line (+). ................. 10
Fig. 2.5. pdf’s of Fisher distribution with κ = 20, 40, and 100......................................... 10
Fig. 2.6. Coefficients a, b and c for conversion factor [1/C13 ] as functions of Fisher
constant κ . ......................................................................................................... 12
Fig. 2.7. Coefficients a, b and c for conversion factor [1/C23 ] as functions of Fisher
constant κ . ......................................................................................................... 13
Fig. 2.8. Cylindrical sampling of Fisher-distributed fractures with mean pole m. The
shaded area is a slice of the cylinder surface with normal c. ............................ 15
Fig. 2.9. Cylinder axis (z), Fisher mean pole (m), and normal (c) of a slice on the
cylinder surface.................................................................................................. 16
Fig. 2.10. Coefficients a, b and c for conversion factor [1/C23,C] as functions of Fisher
constant κ . ......................................................................................................... 18
Fig. 2.11. Fracture normals (▲) and mean pole (•) in lower hemisphere projection....... 21
Fig. 2.A-1. Coordinate system for spherical triangle formed by m, s and n. .................. 24
Fig. 2.A-2 The figure shows the range, Rθ , of θ , as a function of δ, α and ρ. Angle ρ
(between m and s) is a constant. ....................................................................... 26
Fig. 3.1. Borehole or shaft sampling of fractures in a rock mass. .................................... 33
Fig. 3.2. Fracture traces on a cylindrical shaft. Intersections between fractures and the
shaft are traces (curved line segments) on the shaft surface.............................. 38
Fig. 3.3. A thin slice of the shell sampling in fractures. The total trace length on its
surface is dl. ....................................................................................................... 39
vii
Fig. 3.4. A cylindrical shell (axis Z, height = H) intersects a set of fractures with constant
orientation (normal n)........................................................................................ 43
Fig. 3.5. For cylindrical sampling in fractures with constant orientation, the correction
factor C23,C between areal intensity P21,C and volumetric intensity P32 is a
function of angle β0 between the cylinder axis and fracture normal. ................ 45
Fig. 3.6. Illustration of linear (vector) IUR sampling in 3-d space................................... 49
Fig. 3.7. The cycloid (heavy curve) is the path of a point on the circle of radius r0 as the
circle rolls from left to right along the x′-axis. .................................................. 51
Fig. 3.8. The computer program is used to generate rectangular fractures intersecting with
a borehole........................................................................................................... 52
Fig. 3.9. Illustration (to the scale) of the five cases studied. Shaded rectangles are
simulated fractures, and circles are sampling cylinders..................................... 53
Fig. 3.10. Simulation results of the conversion factor 1/ C23,C, compared with the
calculated curve by Eq.(3.19). ........................................................................... 54
Fig. 3.A-1. Unit vectors S, T, n, and nr in Cartesian coordinate system, where Z is
parallel to the borehole axis. The coordinates of unit vectors S and n are given
based on the geometry. ...................................................................................... 57
Fig. 4.1. Joints on limestone bed at Llantwit Major, Wales (photo provided by Matthew
Mauldon). Cross joints terminate at primary systematic joints. ........................ 65
Fig. 4.2. Schematic drawing of dipping sedimentary beds, with primary joints either
terminating on bedding planes or cutting across several layers......................... 65
Fig. 4.3. Borehole/shaft and rectangular fractures and their projections on the axis-normal
plane. Note true width w and apparent width w′. .............................................. 66
Fig. 4.4. A vertical borehole of diameter D intersects rectangular fractures in six ways.
The unrolled trace map is developed from the borehole wall by cutting along
fracture dip direction. Intersection types are marked beside the corresponding
traces. ................................................................................................................. 70
Fig. 4.5 Six types of intersection between projected fractures (shaded) and
boreholes/shafts (dashed circles) are shown on the axis-normal plane. ............ 71
viii
Fig. 4.6. The locus for borehole/shaft-projected fracture intersection on the axis-normal
plane is the region inside by the dashed line. ................................................... 73
Fig. 4.7. Each intersection type has a corresponding locus on the projected fracture (bold
rectangle) for the center of the borehole. In this case, w′ > D. .......................... 73
Fig. 4.8. Each intersection type has a corresponding locus on the projected fracture (bold
rectangle) for the center of the borehole. In this case, D/2 < w′ ≤ D. ................ 74
Fig. 4.9. The corresponding locus for the center of the borehole/shaft for each intersection
type around the projected fracture (bold rectangle) on the axis-normal plane for
case w′ ≤ D/2...................................................................................................... 74
Fig. 4.10. Flowchart of choosing estimators to estimate mean fracture length and width.
........................................................................................................................................... 85
Fig. 4.11. A computer program was developed to generate a population of rectangular
fractures intersected by a borehole/shaft............................................................ 92
Fig. 4.12. Comparison of computed fracture length and width vs. actual fracture length
and width for scenario 1..................................................................................... 94
Fig. 4.13. Percent error and coefficient of variation of estimators for (a) fracture length
and (b) fracture width, in comparison with observed counts of B3-type
borehole/shaft-fracture intersections.................................................................. 95
Fig. App-1. The geometry of fracture, sampling cylinder, and three different shapes of
generation region. ............................................................................................ 108
ix
List of Tables
Table 2.1. Factor 1/C13 vs. κ and ρ ................................................................................... 12
Table 2.2. Factor 1/C23 with different values of κ and ρ. ................................................. 13
Table 2.3. 1/C23,C, the conversion factor between P21 and P32 when sampling with
cylinder surface............................................................................................... 18
Table 2.4. Orientation data for a set of fractures on the Huckleberry Trail...................... 20
Table 3.1. Simulation parameters and results. .................................................................. 53
Table 4.1. Six borehole/shaft-fracture intersection types ................................................. 69
Table 4.2. Defined symbols .............................................................................................. 72
Table 4.3. Areas of regions corresponding to each borehole/shaft-fracture intersection
type from geometry......................................................................................... 76
Table 4.4. Borehole-fracture intersection counts from a borehole sampling.................... 86
Table 4.5. Borehole-fracture intersection counts from borehole sampling ...................... 89
Table 4.6. Parameters and results of Monte Carlo simulations ........................................ 93
Table App-1. Inputs for generating the Fisher distribution. ........................................... 106
Table App-2. Parameters for simulating fractures sampled by a borehole..................... 107
Table App-3. Minimum dimension of different generation regions............................... 109
x
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1
Chapter 1
1 Introduction
Characterization of rock fractures is essential in engineering geology, civil engineering,
mining engineering and oil and gas industry. Geometric and mechanical parameters of
fractures are widely used for estimating fractured rock mass strength, deformability,
permeability, and fluid storage capacity. Currently geological investigations have
provided a great amount of fracture data from boreholes, tunnels, shafts as well as other
cylindrical sampling surfaces. Therefore, the study of fracture characterization based on
cylindrical sampling of fractured rock mass is of great significance. In this dissertation,
the author intends to study the stereological relationships in cylindrical samplings,
unbiased scanline techniques and their applications, and estimation of fracture size in
sedimentary rocks. These studies are demonstrated in the following three chapters.
Chapter 2 discusses the conversions (linear fracture intensity measure P10, planar fracture
intensity measure P21 and cylindrical fracture intensity measure P21,C, to the volumetric
fracture intensity measure P32) appropriate for constant size or unbounded fractures with
a Fisher distribution of orientation. The corresponding paper is submitted to
Mathematical Geology. Chapter 3 discusses the estimating of fracture intensity, more
specifically, fracture volumetric intensity P32, from fracture trace data in cylindrical
(borehole, tunnel or shaft) samplings. The conversion factor between the cylindrical
fracture intensity measure P21,C and the fracture volumetric intensity P32, is presented in a
general form and some special cases are also discussed. The corresponding paper is for
submission to International Journal of Rock Mechanics & Mining Sciences. In Chapter 4
the author intends to develop a general model for estimating mean rectangular fracture
length and width from traces on cylinder walls. The corresponding paper is for
submission to Rock Mechanics & Rock Engineering.
2
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3
Chapter 2
2 Multi-dimensional intensity measures for Fisher-distributed
fractures
Abstract: Fracture intensity is fundamentally a three dimensional concept, relating the
total area (m2) or volume (m3) of fractures to the volume of the rock mass studied.
However, field measurements of fracture intensity in rock masses are usually either one
dimensional - along sampling lines or boreholes, or two dimensional - on tunnel walls or
trace planes. In this paper, conversions between these one and two dimensional intensity
measures, and the three dimensional intensity measure P32, are developed for constant
size or unbounded Fisher-distributed fractures, for three types of sampling domain: lines,
planes and cylindrical surfaces. Conversion factors for each of these sampling domains
are derived semi-analytically, and then computed, graphed and tabulated for a wide range
of cases. The practical significance of this work is that it enables rock engineers and
geologists to deduce 3-d fracture intensity from 1-d or 2-d field measurements.
2.1 Introduction
The Fisher distribution (Fisher, 1953) is the most commonly assumed distribution for
natural fracture orientations (Cheeney, 1983). This is largely due to its relatively simple
form, as compared to other distributions for spherical data (N. Fisher et al., 1987). The
Fisher distribution also has the advantage that it is the theoretical analogue of the normal
distribution, for spherical data. Because of these advantages, the Fisher distribution is
widely used for hydrological and geomechanical modeling in fractured rock (Cheeney,
1983; Priest, 1993).
One dimensional (1-d) and two dimensional (2-d) fracture intensity measures P10 and P21
are defined, respectively, as the number of fractures per unit length and the number of
fractures per unit area (Dershowitz & Herda, 1992; Mauldon, 1994) in the rock mass.
4
These measures are directionally dependent and are strongly affected by the relative
orientation of the fractures and the sampling domain, e.g., scanline, or planar surface. In
contrast, the three dimensional (3-d), or volumetric, fracture intensity measure P32,
defined as area of fractures per unit volume, is not directionally dependent (Dershowitz &
Herda, 1992; Mauldon, 1994). Measures P10 and P21 are easy to measure in the field, but
they cannot be used as general parameters to characterize fracture intensity because of
their directional dependence. For these reasons, the ability to convert linear intensity P10
or areal intensity P21 to the volumetric intensity P32, which is difficult to measure in the
field but directional independent, will be very useful.
Previous work (Dershowitz & Herda, 1992; Mauldon, 1994, Mauldon & Mauldon, 1997)
has developed some of the theoretical background for fracture intensity measures. In the
present paper, the authors derive conversions between field measures of fracture
intensity, P10 and P21, and the three dimensional volumetric fracture intensity measure P32
for fracture sets with the Fisher orientation distribution. This study focuses on fracture
orientation instead of fracture size; we assume fractures are either of constant size or are
unbounded. Based on this assumption, factors to convert measured 1-d or 2-d fracture
intensity for Fisher-distributed fractures to volumetric intensity are obtained semi-
analytically for sampling domains on lines, planes and cylinders.
2.2 General form of conversions
Conversions between 1-d intensity measure P10 and 3-d intensity measure P32, or between
2-d intensity measure P21 and 3-d intensity measure P32, require consideration of the
sampling bias that arises from the relative orientation of the sampling domain and the
fracture. This bias was first described by R. Terzaghi (1964), and later explored by Yow
(1987), Priest (1993), Martel (1999), and Mauldon and Mauldon (1997), among others.
In the general case, for linear or planar sampling of constant size or unbounded fractures,
P10 and P21 are related to P32 in the following ways (Dershowitz, 1992; Mauldon, 1994):
5
( ) αααπ
dfPP Α∫= |cos|0
3210 and (2.1)
( ) βββπ
dfPP Β∫=0
3221 sin , (2.2)
where α is the angle between the sampling line and the fracture normal (Fig. 2.1a); β is
the angle between the sampling plane normal and fracture normal (Fig. 2.1b); and
fΑ(α) and fΒ(β) are the probability density functions (pdf’s) of α and β, respectively. In
the following, we assume a statistically homogeneous sampling domain, and it is to be
understood that the given relationships refer to expected values of the intensity measures.
Here, for simplicity, the integrals in Eqs. (2.1) and (2.2) are each functions of a single
variable. The angles α or β are themselves functions of conventional geologic fracture
orientation parameters such as dip and dip-direction, and orientation of the sampling line
or sampling plane, and can be calculated from orientations of sampling line or plane and
fracture normal.
Fig. 2.1. Geometry of linear and planar sampling of a fracture.
(a) (b)
Sampling line
Fracture normal
α
Fracture
β
Fracture normal
Sampling plane normal
FractureSampling plane
6
Define conversion factors C13 and C23 by
( )1
013 |cos|
−
Α ⎥⎦
⎤⎢⎣
⎡= ∫ ααα
π
dfC and (2.3)
( )1
023 sin
−
Β ⎥⎦
⎤⎢⎣
⎡= ∫ βββ
π
dfC , (2.4)
so that
321013 PPC = and (2.5)
322123 PPC = . (2.6)
The integrals in Eqs. (2.3) and (2.4) are on [0, 1], so the ranges of the conversion factors
C13 and C23 are from 1 to ∞.
As an example, for the isotropic case of a uniform fracture orientation distribution,
αα sin)( 21=Αf and ββ sin)( 2
1=Βf (Fig. 2.2), for α and β in the range [0, π].
Introducing these pdf’s into (3) and (4), respectively, we have 1
021
)( 13 |cos|sin−
⎥⎦
⎤⎢⎣
⎡= ∫
π
ααα dC isotropic and (2.7)
( )1
0
1
0
221
)( 23 2cos141sin
−−
⎥⎦
⎤⎢⎣
⎡−=⎥
⎦
⎤⎢⎣
⎡= ∫∫ ββββ
ππ
ddC isotropic , (2.8)
which, combining with Eqs. (2.5) and (2.6), yield (Dershowitz, 1985)
32)( 10 21 PP isotropic ⎟
⎠⎞
⎜⎝⎛= and (2.9)
32)( 21 4PP isotropic ⎟
⎠⎞
⎜⎝⎛=
π. (2.10)
7
Fig. 2.2. For an isotropic fracture orientation distribution, the distributions of α and β are
proportional to the sin α and sin β, respectively.
Eqs. (2.9) and (2.10) imply that for uniformly distributed fractures (the isotropic case),
P32 is twice the average scanline frequency and 1.27 times the mean areal trace length
intensity. In the following, we determine the conversion factors C13 and C23 for the case
of Fisher-distributed fractures.
2.3 Linear and planar sampling of fisher-distributed fractures
The probability density function of the Fisher distribution is given as (N. Fisher et al,
1987)
(a) (b)
Fracture
Sampling line
Fracture normal
α
length ∝ sinα
Samplingplane
Fracture
Fracture normal
Sampling plane normal
βlength ∝
8
)0( )( πδδκδ κκ
δκ
≤≤−
= −∆ eeSinef
Cos
, (2.11)
where δ is the angle between a fracture normal and the Fisher mean pole (Fig. 2.3); f∆(δ)
is the probability density function of δ; and κ is the Fisher constant related to the amount
of dispersion (κ has high values for low dispersion and low values for high dispersion).
Because of the radial symmetry of the Fisher distribution about its mean pole, we express
its probability density function as a function only of δ for a given dispersion constant.
The local azimuth of the Fisher mean pole is uniform on [0, 2π] and is independent of δ.
Fig. 2.4 shows a set of fracture normals following the Fisher distribution, in upper
hemisphere projection. Fisher mean pole m corresponds to a plane with dip 80º and dip-
direction 45º. The Fisher dispersion constant κ in this case is equal to 60.
The theoretical range of κ is from 0 to ∞, with low values indicating a high degree of
dispersion. As κ approaches 0, the fractures approach a uniform orientation distribution.
Typical graphs of the pdf of the Fisher distribution are shown in Fig. 2.5.
In order to obtain the conversion factor between 1-d intensity measure P10 and 3-d
intensity measure P32, we need to know fΑ(α) , the probability density function of angle α
between the sampling line and the fracture normal.
Based on the geometry of the spherical triangle formed by the fracture normal n, the
Fisher mean pole m and the sampling line s (Fig. 2.3), the theoretical probability density
function fΑ(α) is given by (see Appendix 2.A):
δδκ
ρδαρδ
απ
α κκ
δκ
δ
deeSinef
Cos
R−Α −−−
= ∫ 222 )coscos(cossinsin
sin 1)( (2.12)
for α in the range ρδαρδ +≤≤− || , where the range of integration Rd is given by:
],-[ αραρδ +=R , if ρα ≤ , or
]2 ,0[ ραδ −=R , if ρα > . (2.13)
9
The integral in Eq. (2.12) cannot, however, be expressed in closed form. We use
numerical simulation to find the set of values of the conversion factor, following the
procedure described in Appendix 2.B.
Fig. 2.3. Spherical triangle formed by n, m, and s, where n is fracture normal, m is
Fisher mean pole, and s is the sampling line. The spherical angles α, δ, and ρ are,
respectively, the angles between n & s, m & n, and m & s.
10
Fig. 2.4. Fisher-distributed fracture normals in relation to sampling line (+).
Fig. 2.5. pdf’s of Fisher distribution with κ = 20, 40, and 100.
01234567
0 10 20 30 40 50 60 70 80 90Angular deviation δ (deg.) from Fisher mean pole
κ = 100
κ = 40
κ = 20
f(δ)
North
20º
Fisher Mean Pole m(dip 80º, dip -direction 45º)
Upper Hemisphere Equal Area
Sampling line s (trend 225º, plunge 45º)
Small circle with α = 20º
Fracture normal ni
11
Tabulated values of the factor 1/C13 (= P10/P32) are shown in Table 2.1 as a function of
the Fisher constant κ and angle ρ. The reciprocal of C13, rather than C13, is tabulated in
order that values range between 0 and 1. When κ is relatively small (κ < 1), indicating
that fracture orientations have close to a uniform distribution, the factor 1/C13 is close to
0.50, which agrees with Eq. (2.9). The factor 1/C13 can be fitted to the family of curves
given by cbaC += )cos(/1 13 ρ (Fig. 2.6). Regression coefficients a, b and c can be
computed for κ ≥ 1, according to the logarithmic expression given in Fig. 2.6. For κ < 1,
it is recommended to treat the distribution as uniform and to use the conversion factor
given by Eq. (2.9).
Following the procedure described in Appendix B, the conversion factor 1/C23 (= P21/P32)
is also computed numerically. The values of the factor 1/C23 are tabulated in Table 2.2 as
a function of κ and ρ. As with the case of linear sampling, for a given value of ρ, the
conversion factor 1/C23 is relatively insensitive to changes in κ for κ > 50. When κ is
relatively small (κ < 1), the factor is close to 0.79, which agrees with Eq. (2.10). The
conversion factor 1/C23 can be fitted to the family of curves given by
cdbaC +−= )2/sin(/1 23 πρ (Fig. 2.7). Regression coefficients a, b, c and d can be
computed for κ ≥ 1, according to the logarithmic expression given in Fig. 2.7. For κ < 1,
it is recommended to treat the distribution as uniform and to use the conversion factor
given by Eq. (2.10).
12
Table 2.1. Factor 1/C13 vs. κ and ρ
ρ κ 0.1 1 2 5 10 50 100 200 500 ∞ 0 0.50 0.53 0.62 0.79 0.90 0.98 0.99 0.99 1.00 5 0.50 0.53 0.62 0.79 0.89 0.97 0.98 0.99 0.99
10 0.50 0.53 0.61 0.78 0.88 0.96 0.97 0.98 0.98 20 0.50 0.53 0.59 0.75 0.84 0.91 0.92 0.93 0.93 30 0.50 0.52 0.56 0.68 0.77 0.84 0.85 0.85 0.85 40 0.50 0.51 0.54 0.62 0.67 0.74 0.75 0.75 0.75 50 0.50 0.51 0.51 0.54 0.57 0.62 0.62 0.63 0.63 60 0.50 0.49 0.48 0.47 0.45 0.47 0.48 0.48 0.48 70 0.50 0.48 0.45 0.39 0.34 0.32 0.32 0.32 0.32 80 0.50 0.48 0.44 0.34 0.26 0.18 0.16 0.16 0.16 90 0.50 0.48 0.44 0.33 0.24 0.11 0.08 0.06 0.04
Cos ρ
Fig. 2.6. Coefficients a, b and c for conversion factor [1/C13 ] as functions of Fisher
constant κ . The equations for a, b and c shown in the figure are for κ > 1.
0.0
0.5
1.0
1.5
2.0
2.5
3.0
0.1 1 10 100 1000κ
Coe
ffici
ent
a b
c
cbaC += )cos(/1 13 ρ
2.0951 + )ln( 0.1655
- = κ
b
0.0507 + )ln( 0.1247 = κ
a
0.5988 + )ln( 0.0551- = κ
c
13
Table 2.2. Factor 1/C23 with different values of κ and ρ.
ρ κ 0.1 1 2 5 10 50 100 200 500 ∞ 0 0.79 0.77 0.70 0.53 0.39 0.19 0.14 0.11 0.07 5 0.79 0.77 0.70 0.54 0.40 0.21 0.17 0.14 0.12
10 0.79 0.77 0.70 0.54 0.43 0.25 0.22 0.20 0.20 20 0.79 0.77 0.72 0.58 0.49 0.38 0.37 0.36 0.36 30 0.79 0.78 0.74 0.64 0.58 0.53 0.52 0.52 0.52 40 0.79 0.78 0.76 0.71 0.68 0.66 0.66 0.66 0.66 50 0.79 0.78 0.78 0.77 0.77 0.77 0.77 0.78 0.78 60 0.79 0.79 0.79 0.82 0.85 0.87 0.87 0.87 0.87 70 0.79 0.80 0.82 0.87 0.90 0.94 0.94 0.94 0.94 80 0.79 0.80 0.83 0.90 0.94 0.98 0.98 0.99 0.99 90 0.79 0.80 0.83 0.91 0.95 0.99 0.99 1.00 1.00
Sin ρ
Fig. 2.7. Coefficients a, b and c for conversion factor [1/C23 ] as functions of Fisher
constant κ . The equations for a, b, c and d shown in the figure are for κ > 1.
0.0
0.5
1.0
1.5
2.0
2.5
0.1 1 10 100 1000κ
Coe
ffici
ent
b
a
c d
cdbaC +−= )2/sin(/1 23 πρ
0.0351 + )ln( 0.1064=
κa
0.8112 + )ln( -0.0771= κ
c
2.1745 + )
ln( -0.1376
=
κ
b
1.0783 + )ln( -0.1297
= κ
d
14
2.4 Sampling on a cylindrical surface
In this section we discuss the conversion factor between the areal intensity measure
obtained by sampling rock fractures on the surface of a cylinder, and the volumetric
intensity measure P32. Again, constant size or unbounded Fisher-distributed fractures are
assumed. The practical significance of this case arises, on one hand, from the availability
of fracture trace data obtained from borehole image or FMI and FMS logs (Dershowitz et
al., 2000), and on the other hand, from fracture trace maps obtained from circular tunnel
walls (Mauldon and Wang, 2003).
Let P21,C denote fracture trace length per unit area on the cylinder surface. For constant
size or unbounded Fisher-distributed fractures, the relationship between P21,C and
volumetric measure P32 is a function only of the angle ψ between the Fisher mean pole m
and the cylinder axis z (Fig. 2.8) because of the circular symmetry of the sampling
surface with respect to the cylinder axis. Define C23,C as the conversion factor between
P21,C and P32 for cylinder sampling, with
32,21,23 PPC CC = . (2.14)
For a slice of the cylinder surface, such as the shaded area in Fig. 2.8, the normal c of the
surface element makes an angle δ with the mean fracture pole m. Let 213223 / PPC =
denote the conversion factor between P21 and P32 for a sampling plane which has the
same normal as the slice (e.g., vector c in Fig. 2.8), then
( )∫ ∆=max
min
)(/1/1 23,23
δ
δ
δδ dfCC C , (2.15)
where f∆(δ) is the pdf of δ and the integration is carried out over the full range of δ. It
should be noted that C23 in Eq. (2.15) is a function of δ and refers to a specific slice (such
as the shaded strip in Fig. 2.8).
15
We adopt the Cartesian coordinate system shown in Fig. 2.9, where the xy plane is
perpendicular to the cylinder axis z, and for convenience, the x axis is selected to be
perpendicular to the zm plane. If m and c are unit vectors, then
θψδ cossincos =•= cm , (2.16)
from which
⎟⎟⎠
⎞⎜⎜⎝
⎛= −
ψδθ
sincoscos 1
. (2.17)
where θ is the angle between the y-axis and c. Note that θ is uniformly distributed on [0,
2π] because of the radial symmetry of the cylinder (Fig. 2.9). The pdf )(θΘf of θ is
given by
πθ
21)( =Θf . (2.18)
Fig. 2.8. Cylindrical sampling of Fisher-distributed fractures with mean pole m. The
shaded area is a slice of the cylinder surface with normal c.
zm
coδ
ψ
16
Fig. 2.9. Cylinder axis (z), Fisher mean pole (m), and normal (c) of a slice on the
cylinder surface. The xyz cylinder coordinate system is also shown.
And the cdf )(δ∆F of δ is
∫ Θ∆ =<∆=θ
θθδδR
dfProbF
)()( )( , (2.19)
where Rθ is the range of θ corresponding to ∆ < δ, with limits determined by Eq. (2.17)
for specified ψ and δ. Noting the symmetry of the range of θ with respect to y-axis, and
utilizing Eq. (2.17),
∫⎟⎠⎞⎜
⎝⎛
∆
−
=ψδ
θπ
δsincos1cos
0 212)( dF , (2.20)
from which
⎟⎟⎠
⎞⎜⎜⎝
⎛= −
∆ ψδ
πδ
sincoscos1)( 1F , ,20 πθ ≤≤ ( ) ( )ψπδψπ +≤≤− 2/2/ . (2.21)
The pdf )(δ∆f of δ is found by differentiation as
xc
y δ
z
m
ψ
θ o
(0, sin ψ, cos ψ)
(sin θ, cos θ, 0)
1
17
( ) 2/122 sin/cos1sinsin1)()(
ψδψ
δπ
δδ−
=′= ∆∆ Ff , ( ) ( )ψπδψπ +≤≤− 2/2/ . (2.22)
Substituting Eq. (2.22) into Eq. (2.15), we obtain
( ) ( )∫−
=max
min
2/12223,23sin/cos1sin
sin/11/1δ
δ ψδψ
δδπ
dCC C , (2.23)
where ( ) ( )ψπδδψπδ +=≤≤−= 2/2/ maxmin and where (1/C23) is already given
numerically in Table 2.2.
With Table 2.2 and Eq. (2.24), the conversion factor 1/C23,C is computed numerically, and
is tabulated in Table 2.3 as a function of κ and ψ. It is interesting to note that when angle
ψ (between the Fisher mean pole and the cylinder axis) is around 60º, the conversion
factor 1/C23,C is relatively insensitive to κ and has the value ≈ 0.79, which is also the
value obtained (π/4) on any sampling surface for a uniform fracture orientation
distribution, as is implied by Eq. (2.10).
The conversion factor 1/C23,C increases to 1.0 if the cylinder axis is close to the Fisher
mean pole, and decreases to 0.64 (2/π, the theoretical solution for κ → ∞) if the cylinder
axis is perpendicular to the mean pole. The factor 1/C23,C can be fitted to a family of
curves given by cbaC C += )cos(/1 ,23 ψ (Fig. 2.10). Regression coefficients a, b and c can
be computed for κ ≥ 1 according to the logarithmic expression given in Fig. 2.10. For κ <
1, it is recommended to treat the distribution as uniform and the conversion factor1/C23,C
≈ 0.79.
18
Table 2.3. 1/C23,C, the conversion factor between P21 and P32 when sampling with
cylinder surface.
ψ κ
0.1 1 2 5 10 50 100 500 5 0.79 0.81 0.83 0.91 0.95 0.99 0.99 1.00
10 0.79 0.81 0.83 0.91 0.95 0.99 0.99 1.00 20 0.79 0.81 0.83 0.90 0.93 0.97 0.97 0.98 30 0.79 0.80 0.82 0.88 0.91 0.95 0.95 0.95 40 0.79 0.80 0.81 0.85 0.88 0.91 0.91 0.92 50 0.79 0.79 0.80 0.83 0.84 0.86 0.86 0.87 70 0.79 0.79 0.78 0.77 0.77 0.77 0.76 0.77 90 0.79 0.79 0.77 0.75 0.73 0.70 0.70 0.70
Fig. 2.10. Coefficients a, b and c for conversion factor [1/C23,C] as functions of Fisher
constant κ . The equations for a, b and c shown in the figure are for κ > 1.
0.0
0.5
1.0
1.5
2.0
2.5
0.1 1 10 100 1000κ
Coe
ffici
ents
a
b
c
cbaC C += )cos(/1 ,23 ψ
0.0359 + )ln( 0.0274= κa
2.1971 + )ln( -0.0944= κb
0.8045 + )ln( 0.0026= κc
19
2.5 Example: 3-d fracture intensity inferred from scanline data
Table 2.4 contains the orientation data for a set for 19 subparallel fractures. Fracture
orientation data were collected along a 400 ft straight scanline (trend 180º, plunge 0º) on
a rock slope along a former railroad alignment, on the Huckleberry Trail near
Blacksburg, Virginia. Fig. 2.11 shows the fracture normals in lower hemisphere
projection. The fractures are thought to be of approximately the same size, and
orientations to follow the Fisher distribution. Since all fractures belong to a well-defined
set, the “Terzaghi bias” associated with sampling along a straight scanline (Priest, 1993)
is approximately the same for all fractures, and is therefore neglected here.
Let the y-axis be directed horizontally to the north, the x-axis horizontally to the east, and
the z-axis vertically upward. The Fisher mean pole and dispersion constant can be
estimated as follows (Cheeney, 1983).
(1) The arithmetic means of the direction cosines are calculated from
NncNmcNlc iiil ∑∑∑ === nm , (2.24)
where here the total number of fractures N = 19.
(2) The length of the mean vector R is calculated from:
222nml cccR ++= , (2.25)
(3) Direction cosines of the estimated Fisher mean pole are computed from:
RcnRcmRcl nml === , (2.26)
20
Table 2.4. Orientation data for a set of fractures on the Huckleberry Trail.
Direction cosines of
normals Number Dip
Dip-Direction l m n
1 80 44 0.684 0.708 0.174 2 84 76 0.965 0.241 0.105 3 80 44 0.684 0.708 0.174 4 80 270 0.985 0.000 -0.174 5 88 260 0.984 0.174 -0.035 6 82 48 0.736 0.663 0.139 7 88 227 0.731 0.682 -0.035 8 86 244 0.897 0.437 -0.070 9 86 238 0.846 0.529 -0.070
10 89 75 0.966 0.259 0.017 11 86 256 0.968 0.241 -0.070 12 76 43 0.662 0.710 0.242 13 75 58 0.819 0.512 0.259 14 74 50 0.736 0.618 0.276 15 70 42 0.629 0.698 0.342 16 90 248 0.927 0.375 0.000 17 90 66 0.914 0.407 0.000 18 86 252 0.949 0.308 -0.070 19 84 240 0.861 0.497 -0.105
totals 15.942 8.766 1.100 arithmetic means 0.839 0.461 0.058
(4) If R has magnitude greater than about 0.65, the Fisher constant κ can be
approximated by:
)1(1 R−=κ , (2.27)
In this example, the direction cosines of the mean pole are estimated to be:
060.0 481.0 875.0 === nml , (2.28)
which gives a mean plane with dip-direction 61.2º and dip 86.5º. The angle ρ between the
Fisher mean pole and the scanline is calculated to be about 61.0º. The mean resultant
length R is 0.96, from Eq. (2.25), and the Fisher constant is estimated by Eq. (2.27),
which gives κ = 24.6. A similar procedure for computing the Fisher parameters is given
by Goodman (1989), who takes R to be the resultant vector rather than the mean.
21
Fig. 2.11. Fracture normals (▲) and mean pole (•) in lower hemisphere projection.
We can calculate the (direction dependent) fracture frequency P10 along the scanline by
dividing the total number of fractures N by scanline length L: 1
10 048.040019 −=== ftLNP . (2.29)
By using Table 2.1, Fig. 2.6, or the curves defined by the coefficients in Fig. 2.6, we can
interpolate the value of 1/C13. In this example, ρ ≈ 61.0º and κ ≈ 24.6, so 1/C13 ≈ 0.46
and C13 ≈ 2.17. The volumetric intensity measure P32 (fracture area per unit rock mass
volume) can be determined for this fracture set by multiplying C13 and P10, giving 11
101332 10.0) 048.0)(17.2( −− =≈= ftftPCP (2.30)
N
Mean
lower hemisphere
equal area +
Scanline
22
2.6 Discussion and Conclusions
Fracture intensity is a key input for computer models that deal with flow through a
fractured rock mass. Fracture intensity (P32) is inherently three-dimensional, but is
usually approximated via measurements on 1-d or 2-d sampling domains. Conversions
from 1-d or 2-d intensity, however, necessarily depend on the orientation (or orientation
distribution) of the sampling domain with respect to the fracture orientation distribution
of the rock mass. In this paper, conversion factors between 1-d and 2-d fracture intensity
measures (P10 and P21) and the 3-d intensity measure (P32) are discussed for the cases of
constant size or unbounded Fisher-distributed fractures. The needed conversion factors
for linear, planar and cylindrical sampling domains are computed semi-analytically, with
the aid of Monte Carlo simulation. For linear sampling and planar sampling, the
conversion factors C13 and C23 are determined to be in the range of [1.0, ∞]. For
cylindrical surface sampling of constant size or unbounded Fisher-distributed fractures,
the conversion factor C23,C is determined to be in the range of [1.0, π/2]. These
conversion factors are graphed and tabulated for a wide variety of cases.
In practice, straight scanlines run on a rock mass exposure, as well as straight small-
diameter boreholes, can be considered linear sampling. Rock exposures such as rock
slopes, or mine drift walls, are typical examples of planar sampling of fractures. Tunnel,
shaft or borehole walls give rise to cylindrical surface sampling of fractures. After
collecting fracture data on a sampling domain, e.g., a scanline, a planar rock slope, or a
borehole, engineers and geologists can estimate the volumetric intensity measure P32 by
using the conversion factors presented in this paper.
Acknowledgments
Support from the National Science Foundation, Grant Number CMS-0085093, is
gratefully acknowledged.
23
Appendix 2.A Probability density function (pdf) )(αΑf of angle α
Angles ρ, α, and δ between Fisher mean pole m and sampling line s, sampling line s and
fracture normal n, and fracture normal n and Fisher mean pole m, respectively, are
shown in Fig. 2.3 and Fig. 2.A-1.
To simplify determination of the pdf of α, we define a coordinate system as shown in Fig.
2.A-1, in which m is perpendicular to the xy plane, and s is in the zy plane. Vectors s'
and n' are the projections of s and n on xy plane, respectively. The angle between s' and
n' is defined as θ. For the spherical triangle formed by m, n, and s, the following
relationship holds (Ayres, 1954):
ρδρδθα coscossinsincoscos += , (2.A-1)
so that,
⎟⎟⎠
⎞⎜⎜⎝
⎛ −= −
ρδρδα
θsinsin
coscoscoscos 1
. (2.A-2)
The probability density function of angle α depends on δ and θ (ρ being kept constant in
the derivation). For the Fisher distribution, the joint pdf of angle δ and θ is given by (N.
Fisher et al., 1987)
)0( )(2
),(, πδπ
δκθδ κκ
δκ
≤≤−
= −Θ∆ eeSinef
Cos
. (2.A-3)
24
Fig. 2.A-1. Coordinate system for spherical triangle formed by m, s and n.
Angle θ is uniformly distributed in the range [0, 2π] and is independent of angle δ.
Therefore the pdf of θ is
πθ 2/1)( =Θf , (2.A-4)
from which,
)0( )( πδδκδ κκ
δκ
≤≤−
= −∆ eeSinef
Cos
. (2.A-5)
The pdf of angle α can be derived through its cumulative distribution function (cdf).
Given δ, the cdf of α is
o
Xy
z
n
ms
n′s′θ
αδρ
25
∫ ΘΑ =≤Α=θ
θθδαδαδ RdfProbF )()|()|(| , (2.A-6)
where Rθ is the range of θ when Α ≤ α. Given δ, α increases from the minimum of |δ-ρ|
to the maximum of δ+ρ when θ increases from 0 to π. Fig. 2.A-2 shows the relationship
among angles α, δ, ρ, and also the range of θ. Note that Rθ is symmetric about the y-axis.
Below is the determination of Rθ with different range of α, δ, and ρ.
:ρα ≤
lse
/2 )( if /2],,-[ /2 )( if ],,-[
0
],0[ max
eR ⎩
⎨⎧
≥+≥++
∈
⎪⎩
⎪⎨⎧
= παρπαρπαραραρ
δθθ ,
:ρα ≥
=θR⎪⎪⎩
⎪⎪⎨
⎧⎩⎨⎧
≥+<++−
∈/2 )( if /2],,-[ /2 )( if ],,[
],0[ max παρπαρπαρραρα
δθ
]- [0, 2 αρδπ ∈
/2] ),[ 0 παρδ +∈
(2.A-7)
where θmax is the upper limit of θ, which is determined by Eq.(2.A-2), from which
⎟⎟⎠
⎞⎜⎜⎝
⎛ −= −
ρδρδαθ
sinsincoscoscoscos 1
max . (2.A-8)
Then
θπ
δα ρδρδα
δ dF ∫ ⎟⎟⎠
⎞⎜⎜⎝
⎛ −
Α
−
=≤Α sinsincoscoscoscos
0|
1
212)|( , ρδαρδ +≤≤− || , (2.A-9)
from which,
⎟⎟⎠
⎞⎜⎜⎝
⎛ −=≤Α −
Α ρδρδα
πδαδ sinsin
coscoscoscos1)|( 1|F , ρδαρδ +≤≤− || , and (2.A-10)
222||)coscos(cossinsin
sin)|()|(ρδαρδπ
αδαδα δδ−−
=≤Α′= ΑΑ Ff ,
ρδαρδ +≤≤− || . (2.A-11)
26
Then, the pdf of α is
δδκ
ρδαρδ
απ
δδδαα κκ
δκ
δδδ
deeSinedfff
Cos
RR−∆ΑΑ −−−
== ∫∫ 222|)coscos(cossinsin
sin 1)()|()(
ρδαρδ +≤≤− || , (2.A-12)
where Rd is given by
],-[ αραρδ +=R , if ρα ≤ , or
]2 ,0[ ραδ −=R , if ρα > . (2.A-13)
Fig. 2.A-2 The figure shows the range, Rθ , of θ , as a function of δ, α and ρ. Angle ρ
(between m and s) is a constant. Angles δ and α are the semi-apical angles of small
circles about z and y, respectively. Rθ delimits the intersection of the above-mentioned
small circles, projected into the xy plane.
Rθ
27
Appendix 2.B Numerical approach for obtaining FΑ(α) and FΒ(β)
Rewrite Eqs. (2.3) and (2.4) as
( )1
013 cos
−
⎥⎦
⎤⎢⎣
⎡= ∫ αα α
π
dFC , and (2.B-1)
( )1
023 sin
−
⎥⎦
⎤⎢⎣
⎡= ∫ ββ β
π
dFC , (2.B-2)
where FΑ(α) and FΒ(β) are the cdf’s of α and β, respectively. Numerical evaluation of the
finite integrals in the equations gives the conversion factors C13 and C23, using the
procedure described below for FΑ(α). FΒ(β) can be obtained through a similar procedure.
1. Set the mean pole and the Fisher constant κ for the Fisher distribution.
2. Generate a set of Fisher-distributed fracture normals by using the cdf of the Fisher
distribution, given by (Dershowitz, 1985)
)0( 1
)( πδκδ κ
δκ
≤≤−
=∆ eeF
Cos
, (2.B-3)
Fig. 2.4 shows a simulated population of 3000 fracture normals with the Fisher
mean pole corresponding to a plane with dip 80º and dip-direction 45º, and κ = 60.
for a detailed description of the simulation procedure, see Priest (1993).
3. For a given sampling orientation, draw small circles (Fig. 2.4) with values of α at
fixed increments.
4. The cdf FΑ(α) of α, is calculated empirically by the number of fracture normals
falling inside small circles divided by the total number of fracture normals. For
instance, in Fig. 2.4, 104 out of 3000 fracture normals are inside the small circle
with α = 20º. Therefore the cdf FΑ(α) of α, evaluated at α = 20º, is
0.035 3000104)20( ==°=Α αF . (2.B-4)
28
References
Ayres, F. Jr. (1954) “Schaum’s Outline Series of Theory and Problems of Plane & Spherical Trigonometry”. McGraw-Hill
Cheeney, R. F. (1983) “Statistical methods in geology for field and lab decisions”, Allen & Unwin Ltd. London. UK
Dershowitz, W.S. (1985) “Rock Joint System” Ph.D. Dissertation, MIT, Cambridge, Mass.
Dershowitz, W.S. and H.H. Einstein (1988) “Characterizing rock joint geometry with joint system models” Rock Mechanics and Rock Engineering 21: 21–51
Dershowitz, W. S. and Herda, H. H. (1992) “Interpretation of fracture spacing and intensity” Proceedings of the 33rd U.S. Symposium on Rock Mechanics, eds. Tillerson, J. R., and Wawersik, W. R., Rotterdam, Balkema. 757-766.
Dershowitz, W., J. Hermanson & S. Follin, M. Mauldon (2000) “Fracture intensity measures in 1-D, 2-D, and 3-D at Aspo, Sweden”, Proceedings of Pacific Rocks 2000, eds. Girard, Liebman, Breeds & Doe
Einstein, H. H. and Baecher, G. B. (1983) “Probabilistic and statistical methods in engineering geology” Rock Mechanics and Rock Engineering 16: 39-72.
Fisher, N. I., T., Lewis, B.J.J. Embleton (1987) “Statistical analysis of spherical data”. Cambridge University Press, Cambirdge UK
Fisher, R. A. (1953) “Dispersion on a sphere” Proc. Roy. Soc. London, Ser. A, 217: 295-305
Goodman, R. E. (1989) “Introduction to Rock Mechanics”. John Wiley & Sons, New York.
Martel, S.J. (1999) “Analysis of fracture orientation data from boreholes”. Environmental and Engineering Geoscience. 5: 213-233.
Mauldon, M. (1994) “Intersection probabilities of impersistent joints”, International Journal of Rock Mechanics and Mining Science & Geomechanics Abstracts, 31(2): 107-115.
Mauldon, M., J. G. Mauldon. (1997) “Fracture sampling on a cylinder: from scanlines to boreholes and tunnels”. Rock Mechanics and Rock Engineering. 30: 129-144.
Mauldon, M., M.B. Rohrbaugh, W.M. Dunne, W. Lawdermilk (1999) “Fracture intensity estimates using circular scanlines”. In Proceedings of the 37th US Rock Mechanics Symposium, eds. R.L. Krantz, G.A. Scott, P.H. Smeallie, Balkema, Rotterdam. 777-784.
29
Mauldon M., W. M. Dunne and M. B. Rohrbaugh, Jr. (2001) “Circular scanlines and circular windows: new tools for characterizing the geometry of fracture traces”. Journal of Structural Geology, 23(3): 247-258
Mauldon M. and X. Wang (2003) “Measuring Fracture Intensity in Tunnels Using Cycloidal Scanlines” Proceedings of the 12th Panamerican Conference on Soil Mechanics and Geotechnical Engineering and the 39th U.S. Rock Mechanics Symposium.
Owens, J.K., Miller, S.M., and DeHoff, R.T. (1994) “Stereological Sampling and Analysis for Characterizing Discontinuous Rock Masses”. Proceedings of 13th Conference on Ground Control in Mining. 269-276.
Priest, S.D. (1993) “Discontinuity Analysis for Rock Engineering”. Chapman and Hall, London.
Russ, J. C., DeHoff, R. T. (2000) “Practical Stereology” Kluwer Academic/Plenum Publishers, New York
Terzaghi, R.D. (1965) “Sources of errors in joint surveys”. Geotechnique. 15: 287-304.
Yow, J.L. (1987) “Blind zones in the acquisition of discontinuity orientation data”. International Journal of Rock Mechanics and Mining Sciences and Geomechanics Abstracts. Technical Note. 24: 5, 317-318.
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31
Chapter 3
3 Estimating fracture intensity from traces on cylindrical
exposures Abstract
Fracture intensity is a fundamental parameter when characterizing fractures. In the field,
a great amount of fracture data is collected along boreholes, circular tunnel or shaft walls.
The data reveal some characteristics of fractures in rock masses; however, it has not been
sufficiently interpreted. In this paper, we discuss estimating of fracture intensity, more
specifically, fracture volumetric intensity P32, from fracture trace data in cylindrical
(borehole, tunnel or shaft) samplings. We built up the relationships between the 2-d
fracture intensity measure and the 3-d fracture intensity measure theoretically.
Stereological analyses show that the conversion factor between the two intensity
measures is not dependent on fracture size, shape or circular cylinder radius, but is related
to the orientation of the cylinder and the orientation distribution of fracture area. It is also
found that the fracture volumetric intensity measure P32 is always 1.0 to 1.57 times of
fracture trace length per unit borehole surface area (P21,C). The technique of using
cycloidal scanlines to estimate the fracture volumetric intensity is also discussed. A
computer program is developed to generate synthetic fractures sampled by a circular
cylinder and the derived conversion factor between the two intensity measures is tested
by Monte Carlo simulations.
Key words: cylindrical sampling, fracture networks, stereology, rock mass, intensity
measures, conversion factors
32
3.1 Introduction
Natural rock masses are commonly dissected by discontinuities such as fractures, faults
and bedding planes, which influence or even control the behavior of rock masses
(Goodman, 1989; Priest, 1993). Therefore, characterization of the fracture system in a
rock mass, including properties such as fracture orientation, shape, size, aperture, and
intensity (ISRM, 1978), is necessary for many engineering applications. Examples of
such applications include hydrocarbon extraction, control of contaminants in landfills,
tunneling, and rock slope engineering.
Fracture intensity, which represents the amount of fractures in the rock mass, is one of
the fundamental parameters for characterizing fracture systems. Fracture intensity can be
interpreted in several ways, corresponding to a set of fracture abundance measures,
depending on the dimension of the sampling domain. (Dershowitz, 1984, 1992; Mauldon
1994). The most commonly used measure is the frequency of fractures, defined as
number of fractures per unit length. Frequency, which is also referred to as the one-
dimensional (1-d, linear) intensity, P10, is often measured along a scanline (Fig. 3.1(a)) of
fixed orientation on a planar exposure, or along the length of a borehole. The sampling
bias (R. Terzaghi 1965) induced by scanline or borehole measurements of fracture
frequency, or P10, remains a problem with scanline measurements. The major difficulty
with implementing frequency data as a fracture intensity measure has to do with the so-
called “blind zone” (Terzaghi, 1965; Yow, 1987), which refers to fracture orientations
that are “not seen” or under-sampled by a borehole or scanline. The geometric
(“Terzaghi”) correction factor for fractures in the blind zone can lead to gross distortion
of the data (Yow, 1987). A review of scanline sampling is presented by Priest (1993,
2004).
On cylindrical exposures such as borehole walls, circular tunnel or shaft walls, the
fracture system is revealed in a two-dimensional (2-d) form. Besides features of fractures
such as orientation, aperture, or infilling that can be measured directly on cylindrical
33
exposures, the intensity, pattern, and termination relationships of fracture traces on the
cylindrical exposure surfaces provide much more information about fracture networks
than a one-dimensional exposure (scanline) does.
Fig. 3.1. Borehole or shaft sampling of fractures in a rock mass. (a) Vertical shaft
intersects several fractures, which yield traces on the cylinder surface and on the face of
the rock mass; horizontal scanline on the rock face intersects three fracture traces. (b)
Unrolled trace map developed from the borehole or shaft wall.
Rock mass
Scanline
Borehole
Fractures
Fracture trace on the slope
Fracture traces total length = l
Unrolled (developed) trace map (total area A)
(a) (b)
34
To explore the relationships between fracture traces on a cylindrical surface and the 3-d
fracture system, we introduce the following notation. Let P21,C denote the two-
dimensional (2-d, areal) fracture intensity on the circular sampling cylinder surface,
defined as trace length per unit sampling surface area. The subscript C denotes the
cylindrical sampling domain. P21,C is determined as the sum of trace length on tunnel or
borehole walls divided by the total surface area of tunnel or borehole walls. In Fig. 3.1(b),
for instance, assume the total trace length on the unrolled trace map is l and the total area
of the unrolled trace map is A. Then the areal fracture intensity is simply P21,C = l / A.
For a fractured rock mass, this measure is a function of tunnel or borehole size and
orientation, as well as the fracture orientation distribution (weighted by fracture size).
Therefore it is also a directionally biased measure, as is as the linear intensity measure
P10.
Let P32 denote the three-dimensional (3-d, or volumetric) fracture intensity, defined as
fracture area per unit volume of rock mass. P32 is independent of the sampling process
and is an unbiased measure of fracture intensity (Dershowitz, 1992; Mauldon 1994).
Interpreted as an expected value, P32 is also scale independent. P32 is a crucial parameter
for numerical analyses in models such as the discrete fracture flow and transport model
(Dershowitz et al., 1998). However, P32 is impossible to measure directly in an opaque
rock mass.
This paper proposes approaches to utilize fracture trace data collected on the cylindrical
exposures of rock mass, such as borehole walls, tunnel or shaft walls, to estimate
volumetric fracture intensity of the rock mass. This determination is based on the derived
relationship (conversion factor) between the fracture areal intensity on a cylindrical
surface (P21,C) and the fracture volumetric intensity measure (P32).
Following stereological principles (Russ and DeHoff, 2000) we first discuss the general
form of the conversion factor between the areal intensity P21,C on circular cylinder
surface and fracture volumetric intensity measures P32. Theoretical solutions for the
conversion factor between the two measures are derived in the case of cylindrical
35
sampling of constant orientated fractures, and also sampling of fractures with a uniform
distribution. The conversion factor can be calculated analytically if the fracture
orientation distribution with respect to its area is known. Secondly, another approach to
estimate fracture volumetric intensity, based on the cycloidal scanline technique, is also
discussed. By counting the intersections between cycloidal scanlines and fracture traces
on the circular cylinder surface, the fracture volumetric intensity can be estimated
without knowing the orientation of fractures. Finally Monte Carlo simulations are carried
out to verify the derived correction factors.
3.2 Basic assumptions
In this paper, we study a fractured rock mass sampled by a borehole or tunnel/shaft by
using stereology. For convenience, we make the following assumptions with respect to
the geometry of the sampling domain, e.g., the surface of the tunnel/shaft or borehole;
and of fractures in the rock mass.
a) The surface of the sampling domain is a right circular cylinder, long in relation to
its diameter. Borehole, tunnel or shaft ends are not included in the sampling
domain.
b) Fractures are planar features with negligible thickness. No assumptions are made
regarding the spatial distribution of fractures, or fracture shape. In particular, it is
not necessary that fracture centers follow a Poisson process, or that fractures have
the shape of circular or elliptical discs.
c) No prior assumptions are made about fracture size, or orientation distribution;
however, for the first method discussed below, the fracture orientation distribution
in terms of area must be known.
d) The sampling domain is independent of the rock mass fracture network to be
characterized. What this means in practical terms is the borehole/shaft or tunnel is
emplaced without consideration of fracture locations.
36
The above assumptions are fairly standard in engineering analysis of fractured rock
masses (Priest & Hudson, 1976; Warburton, 1980; Cheeney, 1983; Dershowitz, 1984;
Priest 1993; Mauldon & Mauldon, 1997). Furthermore, these assumptions are applicable
in most rock engineering situations either because of the lack of knowledge of
underground fracture networks before boreholes are excavated or, because the location of
a tunnel or shaft is predetermined, based on external factors.
In accordance with principles of stereology, the 1-d, 2-d and 3-d fracture intensities
discussed in this paper refer to expected values, if not specified otherwise. The acronym
IUR - isotropic, uniform, random – denotes, in general, desirable properties of
stereological samples (Russ and DeHoff, 2000; Mauton 2002). In the present situation,
isotropy is ensured in the plane perpendicular to the borehole/shaft/tunnel axis by the
circular symmetry of the cylinder; the directional relationship between the cylinder axis
and the fracture system, however, is not in general, one of isotropy, except in the special
case of a uniform fracture orientation distribution. One of the primary tasks of this paper
is to account for the directional relationship between cylinder and fractures, with respect
to the determination of fracture intensity.
3.3 General form of the relationship between areal intensity P21,C and
volumetric intensity P32 for right circular cylinders
In this section, we relate the volumetric fracture intensity measure P32 (fracture area per
unit rock mass volume) to the areal fracture intensity measure P21,C as measured on a
cylinder (fracture trace length per unit sampling surface area). The relationship is
presented here in a general form.
We define a geometric correction factor, C23,C by
CC PCP ,21,2332 = , (3.1)
37
where the subscript 23 denotes conversion from a two-dimensional to a three-
dimensional measure, and the subscript C denotes a cylindrical surface sampling domain.
The conversion factor C23,C is a function of cylinder orientation and the fracture
orientation distribution; it does not depend on cylinder radius, as demonstrated in next
section.
The geometric meaning of this conversion factor can be illustrated using a simple model
of a cylindrical surface sample (Fig. 3.2), in which five fractures are sampled by a
vertical shaft of radius r and height H. Let l denote the total summed trace length on the
shaft surface. Given a population of fractures, l is a function of cylinder orientation,
radius r, and height H; and the area-weighted fracture orientation distribution.
Consider a thin cylindrical shell (Fig. 3.2) with radius r. The shell thickness dr is taken to
be infinitesimal, so that the area of fractures contained inside the shell, Afractures, can be
approximated as
drlCA Cfractures ⋅⋅= ,23 . (3.2)
where C23,C is the geometric correction factor. If the fractures are perpendicular to the
circular cylinder surface at the intersections, this correction factor is 1.0 (and the
expression is exact). Otherwise, it is greater than 1.0.
The volumetric fracture intensity measure P32, fracture area per unit volume, for the shell
can be expressed as
drHrA
P fractures
⋅⋅=
π232 (3.3)
Substituting Eq. (3.2) into (3.3), we obtain
CCC PCHr
lCP ,21,23,2332 2=
⋅=
π . (3.4)
38
Fig. 3.2. Fracture traces on a cylindrical shaft. Intersections between fractures and the
shaft are traces (curved line segments) on the shaft surface
This is the general form of the relationship between the 2-d intensity measure for trace
length and the 3-d intensity measure for fracture area in a rock mass. In the following we
derive the correction factor C23,C for the general case of fractures that are distributed
according to a known probability density function for fracture orientation with respect to
fracture area. Then we discuss two special cases: fractures of constant orientation and
fracture orientations uniformly distributed in the rock mass.
3.4 General case of cylindrical sampling As discussed in section 2, the sampling cylinder’s radius, orientation and location is
assumed independent of the rock mass and fracture geometry. Let f(α,β) denote the
probability density function (pdf) of fracture orientation weighted by area, where β is the
acute angle between the sampling cylinder axis (Z-axis in Fig. 3.3(a)) and the normal n to
a fracture; and α is the angle between the Y-axis and the projection of the fracture normal
n onto the XY plane (Fig. 3.3(a)).
Shaft with radius r, shell thickness dr
H Fracture traces, total
39
Fig. 3.3. A thin slice of the shell sampling in fractures. The total trace length on its
surface is dl. (a) A cylindrical shell (axis Z) intersects a set of fractures with orientation
distributed as f(α,β). For a fracture with unit normal n, α is the angle between Y-axis and
the projection of n on the XY plane; β is the angle between n and Z. (b) A portion (unit
height) of a slice from the shell is taken out for study. The ith fracture intersected with the
portion has a unit normal ni and the trace of this fracture on the circular cylinder surface
is represented by a unit vector Ti. The figure above shows the vectors in a lower
hemisphere projection.
Y
Z
Y
Z
β
X α
S
n
dθ
dr
θ
Y
Z
rdθ
1γi
ni
npi S
Ti
(a)
Y
S
Z
npi
Ti θ
ni
βi
γi LH
(b)
40
Consider a thin, narrow slice of unit length, width = rdθ and thickness = dr, taken out
from the shell (Fig. 3.3(b)). Let dli denote the length of the trace of fracture i on the
outside surface of the slice; let Ti be the unit vector representing the direction of the
corresponding fracture trace on the slice surface; and let npi denote the unit normal to a
plane passing through the trace, and perpendicular to the slice surface (npi is the
normalized vector of the cross product S×Ti). Finally, let γi be the angle between npi
and the normal ni of fracture i. Then the infinitesimal area dAi of fracture i inside the
slice is
i
ii
drdldA
γcos⋅
= . (3.5)
Notice that γi varies for different fractures intersecting the same slice, and for the same
fracture intersecting by different slices from the cylindrical shell.
The expected area dAi of fracture i inside the unit length slice can also be expressed in
terms of P32 and the probability density function f(α,β),
drrdfPdA iii ⋅⋅⋅⋅= θβα 1),(32 , (3.6)
where αi and βi are the angles representing the orientation of the normal to fracture i in
the coordinate system shown in Fig. 3.3(a). Equating Eqs. (3.5) and (3.6), the expected
trace length dli of fracture i on the unit slice surface is found to be,
iiii rdfPdl γθβα cos),(32= . (3.7)
The expected total length dl of fracture trace segments on the outer cylindrical surface
contained within the slice of height H is the integration of trace lengths of all fractures
intersecting the slice, with respect to fracture orientation:
βαγβαθβα
ddfHrdPdl cos),(,
32 ∫∫= . (3.8)
41
where γ is the angle between the normal n to a fracture and the normal np to the plane
passing through the trace of the fracture and perpendicular to the slice surface. Note that
γ is a function of θ, α and β (Appendix 3.A) and that, in this context, θ and dθ are
constant.
Denote the integral in Eq. (3.8) as
βαγβαβα
ddfIo cos),(,∫∫= , (3.9)
where Io is a function of f(α, β) and the orientation of the cylinder axis. For this general
case, γcos is determined in Appendix 3.A as
( )αθββγ −+= 222 sinsincoscos , (3.10)
so that
oIHrdPdl ⋅= θ32 . (3.11)
The expected total trace length l on the cylindrical sampling surface is obtained by
integrating dl over all values of θ,
∫∫ ==π
θ2
032 dIHrPdll o .
(3.12)
The fracture areal intensity on the cylinder surface can be expressed as
∫∫ ===ππ
θπ
θππ
2
0
322
0
32,21 222
dIPdIrHHrP
rHlP ooC
(3.13)
Then the conversion factor C23,C relating areal intensity on a cylinder to volumetric
intensity (c.f. Eq. (3.1)) is given by
42
12
0,23 2
−
⎥⎦
⎤⎢⎣
⎡= ∫
π
θπ dIC oC . (3.14)
For this general case, Eq. (3.14) shows that the conversion factor C23,C is dependent
neither on the size of the circular cylinder surface, nor on fracture shape. It is a function
of the orientation of cylinder axis and the area-weighted fracture orientation pdf f(α,β).
The range of the conversion factor will be discussed in the next section.
3.5 Special case: Sampling fractures of constant orientation
When a cylindrical surface samples a set of fractures with constant orientation, we can
always choose the Y-direction so that cylinder axis Z, fracture normal n, and the Y-axis
are coplanar (Fig. 3.4). In this coordinate system, angle α between Y and the projection
of n on the XY plane is 0. Let β0 denote the acute angle between n and Z (Fig. 3.4). It is
a constant in this context.
For fractures with constant orientation, γcos is determined to be (Appendix 3.A)
θβγ 20
2 cossin1cos −= . (3.15)
Note that γcos is not a function of either α or β. Then the integral in Eq.(3.10) is
βαβαγβαγβαβαβα
ddfddfIo ∫∫∫∫ ==,,
),(coscos),(
θβγ 20
2 cossin1cos −== . (3.16)
43
Fig. 3.4. A cylindrical shell (axis Z, height = H) intersects a set of fractures with constant
orientation (normal n). β0 is the angle between the fracture normal and the cylinder axis.
From Eq. (3.14),
12
0
20
212
0,23 cossin122
−−
⎥⎦
⎤⎢⎣
⎡−=⎥
⎦
⎤⎢⎣
⎡= ∫∫
ππ
θθβπθπ ddIC oC (3.17)
Evaluating the above integral using Mathematica (Wolfram Research, Inc, 2004), we
obtain
Y
Z
β0n
H
X
44
)(sincossin1 02
2
0
20
241 βθθβ
π
EllipticEd =−∫ , (3.18)
where )(sin 02 βEllipticE is a complete elliptic integral of the second kind.
Combining Eqs. (3.18) and (3.14), the conversion factor C23,C relating areal intensity on
a cylinder to volumetric intensity is
[ ] 10
2,23 )(sin
2−
= βπ EllipticEC C . (3.19)
The conversion factor C23,C takes on values ranging from 1 to π/2 for β0 ranging from 0º
to 90º, respectively (Fig. 3.5). Note in particular that fracture volumetric intensity P32 is
equal to fracture areal intensity P21,C on the cylinder surface if fractures are perpendicular
to the sampling cylinder(C23,C = 1); and P32 is 1.57 times fracture areal intensity P21,C on
the cylinder surface if fractures are parallel to the cylinder axis (C23,C = π/2).
It should be noted that the case above of constant fracture orientation is the least isotropic
of all orientation distributions and that the above orientations of the fractures relevant to
the cylinder i.e. parallel and perpendicular to the cylinder axis, also represent extreme
cases. Therefore, for a general case of fracture orientation distribution, the conversion
factor C23,C is in the range [1, π/2] as well. This result is very important to rock
engineering practitioners, especially when there is not much information about the
fracture orientation distribution with respect to area. Since the range of the conversion
factor C23,C is fairly small (1.0 to 1.57), it will be convenient and will not cause major
errors to approximate the fracture volumetric intensity P32 by using Eq. (3.19) or Fig. 3.5,
where β0 is estimated as the average acute angle between fractures and the sampling
cylinder axis.
Finally, for the special case of constant fracture orientation, Eq. (3.19) shows clearly that
the conversion factor C23,C is only a function of the angle between the cylinder axis and
45
the fracture normal. It is independent of the radius of the sampling cylinder, as well as of
fracture shape and size.
Fig. 3.5. For cylindrical sampling in fractures with constant orientation, the correction
factor C23,C between areal intensity P21,C and volumetric intensity P32 is a function of
angle β0 between the cylinder axis and fracture normal. The elliptic integral required to
obtain the curve was evaluated using Mathematica.
3.6 Special case: fractures with uniform orientation distribution
We apply the general result of the conversion factor C23,C to the isotropic case, in which
fracture orientations are uniformly distributed with respect to area.
In this case,
0 1 2 3 4 5 6 7 8 9β0 (degree)
Cor
rect
ion
fact
or C
23,C
π /2
1.
1.1
1.2
1.3
1.4
1.5
1.6
46
Therefore, the integral in Eq.(3.9) is
( ) βααθββπβ
βαγβα
πβ
β
πα
α
βα
dd
ddfIo
∫ ∫
∫∫=
=
=
=⎥⎦
⎤⎢⎣
⎡−+=
=
2/
0
2
0
222
,
sinsincos2
sin
cos),(
(3.22)
And from Eq. (3.14),
( )1
2
0
2
0
2
0
222
12
0,23
sinsincos2
sin2
2
−=
=
=
=
=
=
−
⎥⎥⎦
⎤
⎢⎢⎣
⎡−+=
⎥⎦
⎤⎢⎣
⎡=
∫ ∫ ∫
∫πθ
θ
πβ
β
πα
α
π
θβααθββπβπ
θπ
ddd
dIC oC
(3.23)
The definite integral in Eq. (3.23) was evaluated in Mathematica (Wolfram Research, Inc,
2004), which gives
( )2
9348.4sinsincos2
sin 22
0
2
0
2
0
222 πθβααθββπβπθ
θ
πβ
β
πα
α
≈=−+∫ ∫ ∫=
=
=
=
=
=
ddd (3.24)
So,
πββα
2sin),( =f , and from Appendix 3.A (3.20)
( )αθββγ −+= 222 sinsincoscos . (3.21)
47
( )
[ ] π
πθ
θ
πβ
β
πα
α
ππ
θβααθββπβπ
412
12
0
2
0
2
0
222,23
2/2
sinsincos2
sin2
=≈
⎥⎥⎦
⎤
⎢⎢⎣
⎡−+=
−
−=
=
=
=
=
=∫ ∫ ∫ dddC C
(3.25)
This result can be compared with the results for plane sampling of isotropically
distributed fractures (Dershowitz, 1984), namely
32)( 21 4PP isotropic ⎟
⎠⎞
⎜⎝⎛=
π, (3.26)
where P21(isotropic) is the trace length per unit area of sampling plane.
3.7 Cycloidal Scanline Technique
In this section we discuss a sampling technique that uses a special curved scanline based
on a cycloid, which automatically takes care of the directional bias described by Terzaghi
(1965). By correctly deploying cycloidal scanlines on the cylindrical surface, we can
make an unbiased estimate of fracture volumetric intensity with no need to know the
orientation of fractures (either ahead of time or at the time of sampling).
3.7.1 Unbiased sampling criterion
As mentioned earlier, a basic strategy in stereology involves the use of IUR (Isotropic-
Uniform-Random) sampling (Russ and Dehoff, 2000). A perfectly isotropic 2-d
sampling surface is a sphere, on which the surface area is distributed uniformly with
respect to direction. Similarly, on a plane, a circular scanline is a perfectly isotropic 1-D
48
sampling domain, with length segments uniformly distributed in every direction
(Mauldon et al., 2001). IUR scanlines produce unbiased samples automatically, and thus
obviate the need for any bias correction.
Fig. 3.6(a) shows uniformly distributed unit vectors (directed line segments) on a
hemisphere. Let ψ denote the angle (colatitude) between a unit vector and axis Z. If the
unit vectors have a uniform orientation distribution, the probability p(ψ ) of choosing a
line segment of unit length and along a vector with colatitude ψ ′ must be proportional to
l(ψ) = 2π sin (ψ ) (Fig. 3.6(a)). Choosing a normalizing constant such that ∫p(ψ ) dψ
has the value unity when integrated over all values of ψ (0 to π) for vectors uniformly
distributed in all orientations), we have
ψψ sin)( 21=p (3.27)
As an alternative to selecting scanline orientations from a probability distribution, it is
possible to specify a curved scanline (Fig. 3.6(b)) that utilizes all values of ψ (0 ≤ ψ ≤ π)
with differential scanline arc lengths dL(ψ) proportional in all cases to sinψ , or
ψψ sin)( ∝dL . (3.28)
One form of scanline that has this property is the cycloid, which we discuss in the next
section.
49
Fig. 3.6. Illustration of linear (vector) IUR sampling in 3-d space. (a) Uniformly oriented
unit vectors on a hemisphere. (b) Length-scaled vectors on the cylinder surface.
From stereological principles, (Russ and DeHoff, 2000; Dershowitz, 1984; Mauldon and
Wang 2003), linear fracture intensity P10(unbiased) measured on the cylindrical surface by
such unbiased sampling probes (scanlines) has the following relationship with the
volumetric fracture intensity P32.
3221
)(10 PP unbiased = . (3.29)
(a)
l = 2πsin ψsin ψ ψ
Z
Z
Cycloidal curve
(b)
50
3.7.2 Cycloidal scanlines
Mathematically, a cycloid is the locus of a point on the rim of a circle rolling along a
straight line, as shown in Fig. 3.7. For a generating circle of radius r0, the coordinates of a
point on the cycloid are given by:
⎩⎨⎧
−=−=
)cos1()sin('
0
0φφφ
rzrx
(3.30)
where φ is the angle of rotation of the circle.
One of the properties of a cycloid is that for any point on the cycloid with angle ψ
between Z and the tangent to the cycloid, the incremental arc length dl′ is proportional to
sinψ ( ψψdrld sin4 0=′ ). Therefore the cycloid as a sampling probe satisfies Eq. (3.28)
and can be used as a directionally unbiased (IUR) sampling probe for measuring fracture
intensity on the walls of a borehole or tunnel/shaft. In other words, cycloids can be used
as scanlines on (right-circular) cylindrical surfaces without the need to correct for
directional sampling bias, and without the need to know fracture orientation. In practice,
cycloidal scanlines can be modified in various ways for more efficient deployment (Russ
and DeHoff, 2000; Mauldon and Wang 2003), as long as the correct relationship between
arc length and orientation is maintained. The fracture volumetric intensity P32 can then
be estimated by Eq. (3.29) - which in terms of expected values is an exact expression.
3.8 Monte Carlo Simulations
A computer program was developed in Visual C++ and used to generate a population of
synthetic fractures, of rectangular shape, intersecting a cylindrical surface such as the
wall of a borehole, tunnel or shaft (Fig. 3.8). The fracture traces are computed and shown
on the unwrapped cylindrical surface (right-hand window in Fig. 3.8). For each
simulation, the total number of generated fractures, the area of each fracture, as well as
the size of the generation region were recorded, in order to calculate the volumetric
51
fracture intensity P32. Total fracture trace length on the circular cylinder surface was also
recorded to calculate P21,C, the 2-d intensity on the sampling circular cylinder, by
dividing by total cylinder surface area.
Fig. 3.7. The cycloid (heavy curve) is the path of a point on the circle of radius r0 as the
circle rolls from left to right along the x′-axis.
Five cases are chosen, to represent different fracture sizes and shapes intersecting a
cylinder of constant size (Fig. 3.9). In each case, the angle β0 between fracture normal
and cylinder axis, is set to be 0º, 30º, 60º, and 90º, respectively. Ten simulations were run
for each fracture orientation. The parameters for each case and the results of the
simulations are listed in Table 3.1. For comparison, the conversion factor C23,C calculated
by Eq. (3.19) for each β0 is also listed in Table 3.1. In all the simulations, fracture
volumetric intensity P32 was set constant, P32 = 1.0.
Z
Generating circle
Cycloid
ψdψ
φ
X′
r0
dl′
ψψdrld sin4 0=′
52
The simulation results are plotted in Fig. 3.10, where they are compared with the curve of
C23,C computed by Eq. (3.19). The simulations show that for fractures with constant
orientation, the areal fracture intensity measure on a cylindrical surface P21,C (trace length
per unit cylinder surface area), is related to the volumetric fracture intensity P32 (fracture
area per unit volume), only by angle β0 between the fracture normal and the cylinder axis.
The conversion factor is independent of the cylinder radius, as well as of the size or shape
of fractures. The derived conversion factor, expressed by Eq. (3.19), is also verified from
the simulations.
Fig. 3.8. The computer program is used to generate rectangular fractures intersecting with
a borehole. Fracture orientation can be set to constant or vary according to given
parameters.
Fractures
Borehole Trace map
53
Fig. 3.9. Illustration (to the scale) of the five cases studied. Shaded rectangles are
simulated fractures, and circles are sampling cylinders (radius is constant 10 for all
simulations).
Table 3.1. Simulation parameters and results.
Average C23,C for each case
Fracture
length l
Fracture
width w
Aspect
ratio l /w β0 = 0º β0 = 30º β0 = 60º β0 = 90º
Case 1 100 100 1.0 1.00 1.04 1.31 1.53
Case 2 10 10 1.0 1.01 1.07 1.29 1.56
Case 3 20 20 1.0 1.01 1.06 1.28 1.62
Case 4 100 20 5.0 1.04 1.09 1.32 1.56
Case 5 20 4 5.0 0.99 1.06 1.30 1.57
Average C23,C for each angle β0 1.01 1.07 1.30 1.57
C23,C calculated by Eq. (3.19) 1.00 1.07 1.30 1.57
Case # 1 2 3 4 5
Cylinder radius 10 10 10 10 10
Fracture length l 100 10 20 100 20
Fracture width w 100 10 20 20 4
Aspect ratio l /w
1 1 1 5 5
54
Fig. 3.10. Simulation results of the conversion factor 1/ C23,C, compared with the
calculated curve by Eq.(3.19).
3.9 Discussion & Conclusions
In this paper, we used stereological principles to study the conversion factor between the
2-d fracture intensity measure on a cylinder surface and the 3-d fracture volumetric
intensity measure. The derived conversion factor between the two intensity measures is
not dependent on fracture size, shape or circular cylinder radius, but is related to the
orientation of the cylinder and the distribution of fracture area with respect to its
orientation.
0 1 2 3 4 5 6 7 8 9
Case 1 Case 2 Case 3 Case 4 Case 5
1.6
1.5
1.4
1.3
1.2
1.1
1.0
C23,C calculated by Eq.(3.19)
C23,C from simulations
β0 (degree)
Con
vers
ion
fact
or C
23,C
55
By studying a special case of cylindrical sampling of fractures with constant orientation,
it is found that the fracture volumetric intensity measure P32 is always 1.0 to 1.57 times of
fracture trace length per unit borehole surface area (P21,C). The two values are also the
minimum and maximum limit of the conversion factor between the two measures in a
general case of cylindrical sampling of fractures, which provides a very practical means
in the field to estimate fracture volumetric intensity.
Based on Isotropic-Uniform-Random principle of stereology, cycloidal scanlines, as
directional unbiased probes to estimate the fracture volumetric intensity, is also
introduced in this paper.
A computer program simulating synthetic fractures sampled by a circular cylinder was
developed and the derived conversion factor between the two intensity measures is
confirmed by Monte Carlo simulations.
Acknowledgements
Partial support from the National Science Foundation, Grant Number CMS-0085093, is
gratefully acknowledged.
56
Appendix 3.A Determine |cos γ|
Fig. 3.A-1 shows the unit vectors S, T, n, nr in a Cartesian coordinate system.
In this coordinate system, Z represents the borehole or sampling circular cylinder axis. n
is the normal to a fracture and it makes an acute angle β with Z-axis. α is the angle
between Y-axis and the projection of n on XY. S is a unit normal to a small slice of the
circular cylinder surface, which is parallel to the circular cylinder axis, and it makes an
angle θ with Y-axis. T is a unit vector parallel to the intersection of two planes whose
normals are S and n respectively (Fig. 3.A-1). nr is the unit normal to a plane containing
both T and S.
Let vector T′ be the cross product of n and S.
( )[ ]zyx
zyxSnT
ˆsinsinˆsincosˆcoscos0cossin
coscossinsinsinˆˆˆ
αθβθβθβθθ
βαβαβ
−−+−=
=
×=′
(3.A-1)
Then unit vector T will be the normalized T′.
( )[ ] TzyxT ′−−+−= ˆsinsinˆsincosˆcoscos αθβθβθβ (3.A-2)
where
( )( )αθββ
αθβθβθβ
−+=
−++=′222
222222
sinsincos
sinsinsincoscoscosT.
(3.A-3)
57
Fig. 3.A-1. Unit vectors S, T, n, and nr in Cartesian coordinate system, where Z is
parallel to the borehole axis. The coordinates of unit vectors S and n are given based on
the geometry.
Let vector n′r be the cross product of S and T, which gives a unit vector.
( )
( ) ( ) zT
yT
xT
TTT
zyx
TSnr
ˆcosˆsinsinsinˆcossinsin
sinsinsincoscoscos0cossinˆˆˆ
′+
′−
+′−−
=
′−−
′′−
=
×=′
βθαθβθαθβ
αθβθβθβθθ
(3.A-4)
Then nr is the same as n′r.
Z
YX S T
n r
n
(sinθ, cosθ, 0)
(sinβ sinα, sinβ cosα, cosβ)
58
|cos γ| is given by the dot product of nr and n.
( ) ( )
( )
( )( )αθββ
θαθββ
θαθββββ
βθαθβθαθβ
γ
−+
−+=
′−+
=
⎟⎟⎟
⎠
⎞
⎜⎜⎜
⎝
⎛
⎟⎟⎠
⎞⎜⎜⎝
⎛
′′−
′−−
=
⋅=
222
22
22
sinsincos
sinsinsincos
sinsinsincoscossin
0cossinsinsincossinsin
cos
T
TTT
nnr
(3.A-5)
In the special case that fractures are of constant orientation, we can always rotate the
coordinate system around Z-axis and make n inside ZY plane. Then angle α, the angle
between Y-axis and the projection of n on XY, turns to be zero. Let β0 denote the acute
angle between n and Z, which is a constant in this special case.
Therefore, |cos γ| given by Eq. (3.A-5) will be simplified as follows.
θβ
θββ
θββθββγ
20
2
20
20
2
20
20
2
20
20
2
cossin1
sinsincos
sinsincossinsincoscos
−=
+=
+
+=
(3.A-6)
59
References
Cheeney, R. F., (1983) “Statistical methods in geology for field and lab decisions”, Allen & Unwin Ltd. London. UK
Dershowitz, W.S. (1984) “Rock joint systems”. Ph.D. Thesis, Massachusetts Institute of Technology, Cambridge, Massachusetts.
Dershowitz, W.S. and H.H. Einstein, (1988) “Characterizing rock joint geometry with joint system models” Rock Mechanics and Rock Engineering 21: 21–51
Dershowitz, W. S. and Herda, H. H. (1992) “Interpretation of fracture spacing and intensity” Proceedings of the 33rd U.S. Symposium on Rock Mechanics, eds. Tillerson, J. R., and Wawersik, W. R., Rotterdam, Balkema. 757-766.
Dershowitz, W.S., Lee, G., Geier, J., Foxford, T., LaPointe, P., and Thomas, A. (1998) “FracMan, Interactive discrete feature data analysis, geometric modeling, and exploration simulation”, User documentation, version 2.6, Seattle, Washington: Golder Associates Inc.
Einstein, H. H. and Baecher, G. B. (1983) “Probabilistic and statistical methods in engineering geology” Rock Mechanics and Rock Engineering 16: 39-72.
Goodman, R. E. (1989) “Introduction to Rock Mechanics”. John Wiley & Sons, New York.
ISRM, Commission on Standardization of Laboratory and Field Tests. (1978) “Suggested methods for the quantitative description of discontinuities in rock masses”. International Journal of Rock Mechanics and Mining Science, 15: 319-368
Martel, S.J. (1999) “Analysis of fracture orientation data from boreholes”. Environmental and Engineering Geoscience. 5: 213-233.
Mauldon, M. (1994) “Intersection probabilities of impersistent joints”, International Journal of Rock Mechanics and Mining Science & Geomechanics Abstracts, 31(2): 107-115.
Mauldon, M., J. G. Mauldon. (1997) “Fracture sampling on a cylinder: from scanlines to boreholes and tunnels”. Rock Mechanics and Rock Engineering. 30: 129-144.
Mauldon M., W. M. Dunne and M. B. Rohrbaugh, Jr. (2001) “Circular scanlines and circular windows: new tools for characterizing the geometry of fracture traces”. Journal of Structural Geology, 23(3): 247-258
60
Mauldon M. and X. Wang (2003) “Measuring Fracture Intensity in Tunnels Using Cycloidal Scanlines” Proceedings of the 12th Panamerican Conference on Soil Mechanics and Geotechnical Engineering and the 39th U.S. Rock Mechanics Symposium.
Mauton, Peter R. (2002) “Principles and practices of unbiased stereology: an introduction for bioscientists”. Johns Hopkins University Press.
Owens, J.K., Miller, S.M., and DeHoff, R.T. (1994) “Stereological Sampling and Analysis for Characterizing Discontinuous Rock Masses”. Proceedings of 13th Conference on Ground Control in Mining. 269-276.
Priest, S. D. & Hudson, J. (1976) “Discontinuity spacing in rock”. Int. J. Rock Mech. Min. Sci. Geomech. Abstr. 13: 135-148
Priest, S.D. (1993). “Discontinuity Analysis for Rock Engineering”. Chapman and Hall, London.
Russ, J. C., DeHoff, R. T. (2000) “Practical Stereology” Kluwer Academic/Plenum Publishers, New York
Terzaghi, R.D. (1965) “Sources of errors in joint surveys”. Geotechnique. 15: 287-304.
Warburton, P. M. (1980) “A stereological interpretation of joint trace data”. Int. J. Rock Mech. Min. Sci. Geomech. Abstr., 17: 181-190
Wolfram Research, Inc. (2004). Mathematica, Version 5.1, Champaign, IL.
Yow, J.L. (1987) “Blind zones in the acquisition of discontinuity orientation data”. International Journal of Rock Mechanics and Mining Sciences and Geomechanics Abstracts. Technical Note. 24: 5, 317-318.
61
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62
Chapter 4
4 Estimating length and width of rectangular fractures from
traces on cylindrical exposures Abstract
This study focuses on estimating length and width of subsurface fractures in sedimentary
rocks. Fractures in sedimentary rock are typically elongated along their strikes and their
shapes can be considered rectangles. The study shows how information about length and
width of rectangular fractures can be discerned from study of borehole/shaft-fracture (or
core-fracture) intersections. Based on the possible geometric relations between a fracture
and a sampling cylinder, six types of intersection: transection, long-edge, short-edge,
corner, single piercing, and double piercing, are defined. The probabilities of occurrence
of these intersection types are related to the length and width of the fractures and
borehole/shaft diameter. The mean length and width of the fractures are estimated
directly from the observed counts of different types of intersection in a borehole/shaft or
rock core. A computer program is developed to generate synthetic fractures sampled by a
circular cylinder and the derived estimators are tested by Monte Carlo simulations, which
show satisfactory results.
Key words: cylindrical rock exposures, fracture networks, fracture length and width,
rectangular fractures
63
4.1 Introduction
Rock engineers, geologists, and hydrologists have long made use of fracture trace data
from planar rock exposures to extract characterization of rock fractures and fracture
systems, and procedures for inferring the three-dimensional (3-d) fracture geometry from
traces have been the subject of considerable research (Priest & Hudson, 1976; Cruden,
1977; Baecher et al., 1977; ISRM, 1978; Warburton 1980; Cheeney, 1983; Einstein &
Baecher, 1983; Kulatilake & Wu, 1984; LaPointe & Hudson 1985; Dershowitz &
Einstein, 1988; Dershowitz & Herda, 1992; Priest 1993, 2004; Mauldon et al. 1994;
Zhang & Einstein, 1998; Mauldon et al. 2001; Zhang et al., 2002). For subsurface rock
masses, large planar exposures are, however, rare. Direct measures from cylindrical
exposures, such as circular tunnel and shaft walls, borehole images (Dershowitz et al.,
2000), rock bores, as well as geophysical surveys, often provide the main sources of
subsurface fracture data, for characterization of fracture systems.
Common practice for borehole sampling of fractures (here used as a generic term for
discontinuities of all types) is to treat the borehole as a one-dimensional (1-d) sampling
domain, equivalent to a scanline. Fracture frequency is then taken to be inversely
proportional to the probability of the observed fractures being intersected by the 1-d
sampling line (Terzaghi, 1965; Priest & Hudson, 1976; Dershowitz & Einstein, 1988;
Priest, 1993). If the ratio of sampling cylinder (i.e. borehole) diameter to the average size
of fractures is, however, greater than about 20%, the sampling domain effectively takes
on a higher dimension – either 2-d or 3-d – depending on whether fractures are sampled
using the cylinder surface only, or using the cylinder volume (Mauldon & Mauldon,
1997). Yet another form of 2-d sampling has been described, making use of virtual 2-d
boreholes applied to a subsurface cross-section. (Narr, 1993; Pascal et al., 1997; Fouché
& Diebolt, 2004). Methods have been proposed to use borehole data to determine
fracture orientation distribution (Martel, 1999), average spacing (Narr 1996), 3-d fracture
intensity (Owens et al., 1994; Mauldon & Wang, 2003), fracture surface roughness
(Thapa et al., 1996) and fracture size (Stone, 1984; Mauldon, 2000; Zhang & Einstein,
64
2000; Özkaya, 2003; Wang et al., 2004, 2005). The present paper addresses inference of
fracture size, and also shape.
A wide variety of fracture geometry (or fracture system) models have been proposed in
the literature (e.g. Ruhland, 1973; LaPointe & Hudson, 1985; Dershowitz et al., 1998),
and most of these make assumptions about fracture shape and size distribution. The
Baecher model (Baecher et al. 1977; Dershowitz & Einstein, 1988), for example, assumes
circular disks with lognormally distributed radii. Orthogonal fracture models may
comprise either unbounded (e.g. Snow, 1965) or bounded (e.g. Müller, 1963; Gross, 1993)
joints. Field observations and mechanical consideration lend support to fracture models
for layered sedimentary rocks in which termination and propagation relationships (and
hence fracture size) are governed by elastic properties of the layers, boundary conditions
during fracturing and other mechanical and geometric factors (Engelder, 1993; Gross et
al., 1995). In particular, late forming fractures are likely to be normal to and terminate at
the primary fractures (or mechanical layer boundaries, Fig. 4.1), which may be either
bedding planes or systematic joint sets (Price, 1966; Helgeson & Aydin 1991; Gross,
1993; Engelder & Gross, 1993; Gross et al., 1995; Engelder & Fischer, 1996; Ruf et al.,
1998; Bai & Pollard 2000; Cooke & Underwood, 2001). One of the commonly observed
fracture patterns is that in which the late-forming cross joints propagate between and
orthogonal to preexisting primary joints (e.g. Fig. 4.1) in a “ladder” pattern (Gross, 1993;
Engelder & Gross, 1993). Field observations have also confirmed that fractures in
sedimentary rock are commonly perpendicular to bedding and elongated in one direction
(typically along strike, as shown schematically in Fig. 4.2) (Price, 1966; Suppe, 1985;
Priest, 1993). In all such cases, the shapes of fractures can be approximated as rectangles.
Estimates of (and models for) fracture size are usually predicated on assumed fracture
shape, such as circular disks (Baecher et al. 1977; Mauldon, 2000; Özkaya, 2003),
elliptical disks (Zhang & Einstein, 2002), or rectangles (Narr 1996; Wang et al. 2004,
2005).
65
Fig. 4.1. Joints on limestone bed at Llantwit Major, Wales (photo provided by Matthew
Mauldon). Cross joints terminate at primary systematic joints.
Fig. 4.2. Schematic drawing of dipping sedimentary beds, with primary joints either
terminating on bedding planes or cutting across several layers.
Rock mass
Bedding planes Fractures (joints)
66
In this paper we focus on fractures in sedimentary rocks, in which fracture shape is
assumed to be rectangular; and we introduce methods to estimate the mean length and
width of fractures by using borehole/shaft-fracture intersection (trace) data. For
convenience, the derivations are based on the model of a vertical borehole/shaft sampling
a layered rock mass that contains strike-elongated fractures. The results can also be
applied, however, to a general orientation of the borehole/shaft, as long as the
assumptions discussed in Section 2 are applicable.
A simple model for borehole/shaft sampling of fractures in sedimentary rock is shown in
Fig. 4.3, in which fracture long axes align in the direction perpendicular to the borehole
axis. Consider a fracture of length l and width w (Fig. 4.3). The apparent width w′ is
defined as the width of the fracture when projected onto a plane normal to borehole axis
(the axis-normal plane in Fig. 4.3), and is related to fracture true width by
Fig. 4.3. Borehole/shaft and rectangular fractures and their projections on the axis-normal
plane. Note true width w and apparent width w′. (a) vertical borehole/shaft; (b) general
case of a skew borehole/shaft
(a)
l
w′
w
Axis-normal plane
w′
w
(b)
l
Axis-normal plane
Ground surface Ground surface
BoreholeBorehole ϕ
ϕ
67
ϕcosww =′ . (4.1)
where angle ϕ is the minimum angle between the fracture and the axis-normal plane (Fig.
4.3), i.e. the true dip in the case of a vertical borehole/shaft.
4.2 Assumptions
We make the following assumptions regarding fracture geometry, the borehole/shaft
sampling domain and the interrelationship between sampling domain and fracture system.
a) Fractures are planar rectangular objects with negligible thickness.
b) A shaft or a borehole is considered to be a right circular cylinder of diameter D,
oriented normal to the fracture elongation direction (or to strike when the
borehole/shaft is vertical).
c) The sampling domain refers to the cylindrical surface of the borehole/shaft.
d) The shaft/borehole is assumed to be long compared to its diameter. The end (or
ends) is not included in the cylindrical surface sampling domain.
e) Fracture length is greater than borehole/shaft diameter and also greater than the
apparent width w′of the fracture. Note that if the latter condition is not the case,
the length and width can be interchanged.
f) The location of the borehole/shaft is independent of the locations of fractures in
the rock mass to be explored. This is the case when we have little knowledge of
fracture networks before the excavation of a borehole or a shaft. Statistically, this
assumption ensures that the portion of the rock mass intersected by the cylindrical
surface of the borehole/shaft corresponds to a uniformly distributed, random
68
sample. Isotropy is achieved automatically with respect to directions
perpendicular to the borehole/shaft axis.
4.3 Borehole/shaft-fracture intersection types
Six types of intersection: transection, long-edge, short-edge, corner, single-piercing, and
double-piercing, are defined, based on the possible geometric relations between a
rectangular fracture and a borehole/shaft (Table 4.1). Corresponding to each intersection
type are characteristic types of fracture trace on the unrolled borehole surface (Fig. 4.4).
It may be observed that type A intersections can occur only if fracture apparent width w′
is greater than borehole/shaft diameter D. Type C1 and C2 intersections can occur only if
w′ is less than borehole/shaft diameter D. Note that Wang et al. (2004) used a slightly
different terminology, referring to transactions as complete intersections. A simple
illustration of all six intersection types is shown in Fig. 4.5, in which rectangular fractures
and boreholes/shafts are projected onto the axis-normal plane, on which boreholes/shafts
project as circles.
For the model discussed in this paper – rectangular fracture elongated along strike – we
can identify each of the six intersection types from fracture traces on the borehole/shaft
surface or unrolled trace map (Table 4.1, Fig. 4.4). Note that in Table 4.1, the
characteristics of each intersection type are based on knowing fracture dip-direction (cut
line along fracture dip-direction). If fractures are perpendicular to the borehole/shaft, this
direction can not be determined. In this case, only A-type (Transection) and C2-type
(double piercing) intersections can be easily identified; and it will be difficult to apply the
estimators discussed in this paper.
69
Table 4.1. Six borehole/shaft-fracture intersection types
Intersection
type
Symbol Example
in Fig. 4.4
Trace (or traces) on
borehole/shaft surface
Trace (or traces) on the
unrolled trace map with cut
line along dip-direction
Transection A 1 Full ellipse Full sine curve
Long-edge B1 2 Partial ellipse,
symmetric with respect
to dip-direction or anti-
dip-direction
Partial segments of sine curve,
symmetric with respect to cut
line or anti-dip-direction
Short-edge B2 3 Partial ellipse, centered
with respect to strike
Partial segments of sine curve,
centered along strike
Corner B3 4 Partial ellipse, not
symmetric with respect
to any direction
Partial segments of sine curve,
not symmetric with respect to
any direction
Single
piercing
C1 5 Single partial ellipse,
similar to one of the
paired C2 traces
Single partial segments of sine
curve, similar to one of the
paired C2 traces
Double
piercing
C2 6 Paired partial ellipse,
symmetric with respect
to dip-direction or anti-
dip-direction
Paired partial segments of sine
curve, symmetric with respect
to dip-direction or anti-dip-
direction
70
Fig. 4.4. A vertical borehole of diameter D intersects rectangular fractures in six ways.
The unrolled trace map is developed from the borehole wall by cutting along fracture dip
direction. Intersection types are marked beside the corresponding traces. (a) borehole and
fractures; (b) Unrolled trace map. Coordinate axis θ is defined with θ = -π/2 at the cut
line. If the cut line were taken along strike, the angular coordinate θ would be from 0 to
2π.
(a) (b)
Borehole axis direction
Cut line Cut line
θπ/2 π 3π/2 0 -π/2
D
Cut line
1A
1
6 6hC2 C26
3B23
22B1 B1
2Dip direction
hC1
55
4B34
71
Fig. 4.5 Six types of intersection between projected fractures (shaded) and
boreholes/shafts (dashed circles) are shown on the axis-normal plane. (a) D < w′; (b) D ≥
w′
4.4 Probabilistic model for occurrence of intersection types
We define symbols in Table 4.2.
In this section, we discuss the probabilities of occurrence of each borehole/shaft-fracture
intersection type. The key to the probabilistic model is that, on the axis-normal plane, the
center of a borehole/shaft must be inside a specific region around the projected fracture in
order for an intersection to occur (Fig. 4.6). Each intersection type, therefore, has a
B3
A B2
B1
Boreholes (diameter D < w′)
l
w′
Projected Fracture
(a)
C2 C1
(b)
l
w′
Boreholes (diameter D ≥ w′)
72
corresponding locus with respect to the projected fracture on the axis-normal plane (Figs.
4.7–4.9).
Table 4.2. Defined symbols
Symbol Definition
α Aspect ratio of a fracture: wl /=α .
N~ Number of occurrences of borehole/shaft-fracture intersections. N~ with a subscript (e.g. B1, B2…) indicates the number of occurrences for a specific intersection type (or several types).
H Length of the borehole/shaft.
λ′ Expected frequency of borehole/shaft-fracture intersections: HN /~=λ . λ′ with a subscript (e.g. B1, B2…) indicates the expected frequency of intersections for a specific intersection type (or several intersection types).
λ′(l, w′) Expected frequency of borehole/shaft-fracture intersections when sampling in fractures of constant size (the projected fracture has the dimension of l × w′ on the axis-normal plane).
∆ Area of a region on the axis-normal plane corresponding to an intersection type (or several intersection types). ∆ with a subscript (e.g. B1, B2…) indicates a specific intersection type (or several intersection types).
fL,W′(l,w′) Joint probability density function (pdf) of fracture length and fracture apparent width.
µl and µw′ Expected values of fracture length and apparent width, respectively. For constant fracture orientation, ϕµµ secww ′= , where µw is the mean fracture width.
73
Fig. 4.6. The locus for borehole/shaft-projected fracture intersection on the axis-normal
plane is the region inside by the dashed line. If the center of borehole/shaft is inside the
region, an intersection occurs.
Fig. 4.7. Each intersection type has a corresponding locus on the projected fracture (bold
rectangle) for the center of the borehole. In this case, w′ > D.
w′
l
D/2
B1
B1
B2B2
B3 B3
B3B3
A
D/2 Projected fracture
D/2
D/2
l
w′
Region of intersection
Projected Fracture
Borehole/shaft location
74
Fig. 4.8. Each intersection type has a corresponding locus on the projected fracture (bold
rectangle) for the center of the borehole. In this case, D/2 < w′ ≤ D.
Fig. 4.9. The corresponding locus for the center of the borehole/shaft for each intersection
type around the projected fracture (bold rectangle) on the axis-normal plane for case w′ ≤
D/2.
Projected fracture
C1
w′C1
C2
B1
l
B2, B3 B2, B3
B1
C2D/2
D/2 D/2
l Projected fracture
B2, B3B2, B3
w′
B1
C2 C1C1
B1D/2
D/2 D/2
75
The regions, separated by dashed lines in Figs. 4.7–4.9, each define the possible locus of
the center of a borehole/shaft, corresponding to each intersection type (e.g. A-type, B1-
type, B2-type, B3-type, C1-type and C2-type). For instance, when the center of the
borehole/shaft falls into the shaded region marked as A, a transection intersection will
occur and a full cosine trace will be induced on the trace map. Consider a fracture of
dimension l × w projected on the axis-normal plane so that its projection has size of l × w′.
Then the area of the region for each intersection type as well as the area of all intersection
regions can be determined from simple geometry (Table 4.3).
If the last assumption in Section 4.2 holds, the location of a borehole/shaft is independent
of the location of fractures. If we were to introduce a Cartesian coordinate system on the
axis-normal plane, with origin at the borehole/shaft center, the locations of projected
fractures would be uniform on that plane (this holds even when projected fractures
overlay). In other words, projected fractures on the axis-normal plane have the same
probability to be at any point on that plane. Therefore, for a rectangular fracture, the
frequency λ of any type of intersection is proportional to the area of the corresponding
region on the axis-normal plane (Figs. 4.7-4.9). For fractures of constant orientation and
size, this can be expressed as the equations below.
∆=ηλ (4.2)
where λ is a frequency (Table 4.2), ∆ is an area (Tables 4.2 and 4.3), and η is identical to
the 3-d fracture density P30 (Dershowitz, 1992), i.e., number of fractures per unit volume
of the rock mass. P30 is assumed to be constant.
There are three cases to consider for the probabilistic model, depending on the relative
magnitudes of borehole/shaft diameter D and fracture apparent width w′. In each case,
fractures are assumed to be of constant orientation.
76
Table 4.3. Areas of regions corresponding to each borehole/shaft-fracture intersection
type from geometry
Area Case 4.4.1: w′ > D Case 4.4.2.1: D ≥ w′ > D/2 Case 4.4.2.2: w′ ≤ D/2
∆A 2DwDDllw +′−−′ NA NA
∆B1 42
22 DDDl π
−− 4
222
2 DDwDlw π−+′−′ * =∆ + 21 CB 4
2DwDDllw π−′−+′
∆B2 42
22 DDwD π
−−′ ⎟⎠⎞
⎜⎝⎛ ′
+−′ −
DwDDwD 12
2cos
4π
22 wDw ′−′−
∆B3 43 2
2 DD π+ ⎟
⎠⎞
⎜⎝⎛ ′
−+′ −
DwDDwD 12
2cos2
43π
222 wDw ′−′+
*2
22
32DwDBB
π+′=∆ +
2212 cos wDwDwD ′−′+⎟
⎠⎞
⎜⎝⎛ ′
− −
∆C1 NA 2212 cos wDwDwD ′−′−⎟
⎠⎞
⎜⎝⎛ ′− 2212 cos wDw
DwD ′−′−⎟
⎠⎞
⎜⎝⎛ ′−
∆C2 NA 2DDwDllw −′++′− * =∆ + 21 CB 4
2DwDDllw π−′−+′
∆total 4
2DwDDllw π+′++′
* Area of combined regions
77
4.4.1 w′ > D
In this case, the apparent widths of all fractures are greater than the borehole/ shaft
diameter D. When these relatively large fractures intersect a borehole/shaft, a transection
intersection (type A) may occur. Piercing intersection (C types), on the other hand, are
impossible.
For fractures of constant orientation and size with projected size of l × w′ on the axis-
normal plane, if the fracture density is η, from Eq. (4.2) and Table 4.3, the frequencies,
here interpreted as expected values (Owens et al., 1994), of B1, B2 and B3 intersection are
given by,
( ) ( )4/12, 211 πηηηλ +−=∆=′ DDlwl BB (4.3)
( ) ( )4/12 , 222 πηηηλ +−′=∆=′ DwDwl BB (4.4)
and
( ) ( )4/31 , 233 πηηλ +=∆=′ Dwl BB . (4.5)
For a set of fractures with constant orientation but varied size, let fL,W′(l, w′) denote the
joint pdf of fracture length and apparent width. The expected value of frequency λB3 is
obtained by integrating the right side of Eq. (4.5) over all values of l and w′ (in this case,
w′ ≤ l < ∞; D < w′ < ∞), noticing that λB3(l, w′) in Eq. (4.5) is expressed as a function
independent of fracture size.
The constant η can then be expressed as
( ) ( )
( )4/31
,4/31
2
,,
23
πη
πηλ
+=
′′+= ∫∫′
′
D
wdldwlfDwl
WLB (4.6)
78
Similarly, the expected value of frequencies λB1 and λB2 can be obtained by integrating
the right side of Eqs. (4.3) and (4.4), respectively, over all values of l and w′ (in this case,
w′ ≤ l < ∞; D < w′ < ∞). Noticing that the right side of Eq. (4.3) is not a function of w′
and the right side of Eq. (4.4) is not a function of l.
where µl and µw′ are the mean fracture length and the mean fracture apparent width,
respectively.
Substituting Eq.(4.7) into Eqs. (4.8) and (4.9), the mean fracture length µl and the mean
fracture apparent width µw′ can be determined as:
( ) ⎥⎦
⎤⎢⎣
⎡+++= ππ
λλµ 434
8 3
1
B
Bl
D,
and
(4.10)
( )4/3123
πλη+
=D
B . (4.7)
( )
( ) ( )
( )4/12
,4/1
,2
2
,,
2
,,1
πηµη
πη
ηλ
+−=
′′+−
′′=
∫∫
∫∫
′′
′′
DD
wdldwlfD
wdldwlDlf
l
wlWL
wlWLB
and
(4.8)
( )
( ) ( )
( )4/12
,4/1
,2
2
,,
2
,,2
πηµη
πη
ηλ
+−=
′′+−
′′′=
′
′′
′′
∫∫
∫∫
DD
wdldwlfD
wdldwlfwD
w
wlWL
wlWLB
(4.9)
79
( ) ⎥⎦
⎤⎢⎣
⎡+++=′ ππ
λλµ 434
8 3
2
B
Bw
D. (4.11)
Note that the expected values of fracture length and apparent width are proportional to
borehole diameter D, and are linear functions of the ratios of expected frequency of B1-
type and B2-type intersections over B3-type intersections, respectively.
4.4.2 w′ ≤ D
When fractures are narrow, or sufficiently steep that their apparent widths are smaller
than borehole/shaft diameter, piercing intersections (C types) may occur, whereas a
transection intersection (type A) is impossible. These narrow fractures are called piercing
fractures. Piercing fractures can pierce a borehole/shaft in either of two ways: singly or
doubly, as fracture #5 (doubly piercing) and fracture #6 (singly piercing) show in Fig.
4.4(a). Both single piercing and double piercing fractures intersect the borehole with two
long edges and leave similar traces on borehole/shaft walls, except that double piercing
fractures have paired traces (Fig. 4.4(b)). Double piercing fractures are easily identified
on unrolled trace maps derived from shaft surface or borehole imagery; and the amplitude
h of the traces (Fig. 4.4(b)) can be used to determine the apparent width of fractures by
ϕtan/hw =′ . (4.12)
80
4.4.2.1 D/2 < w′ ≤ D
The procedure to determine the length of piercing fractures with apparent widths greater
than the radius and less than the diameter of the sampling borehole/shaft is as follows.
For fractures of constant orientation and size with projected size of l × w′ on the axis-
normal plane, if the fracture density is η, from Eq. (4.2) and Table 4.3, consider the
following combinations of frequencies, as functions of fracture size.
( ) ( ) ( )[ ]
4/22
,,,
2
21
21
DwD
wlwlwl
CBtotal
CBtotal
πηη
η
λλλ
+′=
∆−∆−∆=
′−′−′
(4.13)
and
( ) ( ) [ ]( )4/12
2,2,2
2121
πηη
ηλ
+−=
∆+∆=′∆+′
DDl
wlwl CBCB
(4.14)
For a set of fractures with constant orientation but varied size, the expected value of the
linear frequency combination (λtotal - λB1 - λC2) can be obtained by integrating right side
of Eq. (4.13) over all values of l and w′(in this case, w′ ≤ l < ∞; D/2 < w′ ≤ D), noticing
that the combination, given fracture size, is not a function of l.
( )
( ) ( )
2/2
,4/2
,2
2
,,
2
,,21
DD
wdldwlfD
wdldwlfwD
w
wlWL
wlWLCBtotal
πµη
πη
ηλλλ
+=
′′+
′′′=−−
′
′′
′′
∫∫
∫∫
(4.15)
Note that the mean apparent width µw′ can be estimated directly by averaging all values
of w′ determined by Eq.(4.12). Then the constant η can be estimated by
81
2/2 221
DD w
CBtotal
πµλλλη
+−−
=′
. (4.16)
The expected value of the linear frequency combination (λB1 + 2λC2) can be obtained by
integrating right side of Eq. (4.14) over all values of l and w′(w′ ≤ l < ∞; D/2 < w′ ≤ D),
noticing that the combination, given fracture size, is not a function of w′.
( )
( ) ( )
( )4/12
,4/1
,22
2
,,
2
,,21
πηµη
πη
ηλλ
+−=
′′+−
′′=+
∫∫
∫∫
′′
′′
DD
wdldwlfD
wdldwllfD
l
wlWL
wlWLCB
(4.17)
Substituting Eq. (4.16) into Eq. (4.17) yields,
( )2121 2/2)4/1(22 CBtotal
w
lCB D
D λλλπµ
πµλλ −−+
+−=+
′ . (4.18)
Finally, the mean fracture length l can be determined as
( ) ( )ππµλλλ
λλµ +++−−
+= ′ 4
84/2
21
21 DDwCBtotal
CBl .
(4.19)
4.4.2.2 w′ ≤ D/2
The fractures in this case are very narrow piercing fractures or very steep fractures (angle
ϕ close to 90°) whose apparent widths are smaller than borehole/shaft radius. This
scenario is rare in borehole samplings, but may occur for shafts or tunnels. The regions
separated by the dashed lines in Fig. 4.9 show the locus of the center of a borehole/shaft
82
corresponding to each intersection type (e.g. C1-type, C2-type, B1-type, B2 and B3-type)
for this case.
For fractures of constant orientation and size with projected size of l × w′ on the axis-
normal plane, if the fracture density is η, consider the total borehole/shaft-fracture
intersection frequency and the following linear combination of frequencies from Eq. (4.2)
and substitute for areas from Table 4.3, we have
( ) ( )4/ , 2DwDDllwwl totaltotal πηηλ +′++′=∆=′ (4.20)
( ) ( ) ( )2/2
,,2
2121
DwD
wlwl CBtotalCBtotal
πηη
ηλλ
+′=
∆−∆=′−′ ++
(4.21)
For a set of fractures with constant orientation but varied size, the expected value of the
frequency combination (λtotal - λB1+C2) can be obtained by integrating right side of Eq.
(4.21) over all values of l and w′(in this case, w′ ≤ l < ∞; 0 ≤ w′ ≤ D/2), noticing that the
combination, given fracture size, is not a function of l.
( )
( ) ( )
2/2
,2/
,2
2
,,
2
,,21
DD
wdldwlfD
wdldwlfwD
w
wlWL
wlWLCBtotal
πηµη
πη
ηλλ
+=
′′+
′′′=−
′
′′
′′+
∫∫
∫∫
.
(4.22)
Again, the mean apparent width µw′ can be estimated by averaging all w′ determined by
Eq.(4.12). Then constant η can be estimated by
2/2 221
DDw
CBtotal
πµλλη
+−
=′
+ . (4.23)
83
The expected value of the total frequency λtotal is expressed as
( ) ( )∫∫′
′ ′′+′++′=wl
WLtotal wdldwlfDwDDllw,
,2 ,4/πηλ .
(4.24)
The integral in Eq.(4.24) is difficult to evaluate unless we know or could assume the joint
pdf of fracture length and apparent width. For instance, if we assume:
a) Fracture length is constant (and equal to l*). Then the integral in Eq.(4.24) is
simplified as follows.
( ) ( )
( ) ( )
( ) ( )
( ) ( )4/
,4/
,
,4/
**
,,
*
,,
*
,,
2
DlDDl
wdldwlfwDlD
wdldwlfwDl
wdldwlfDwDDllw
w
wlWL
wlWL
wlWLtotal
πηµη
πη
η
πηλ
+++=
′′′++
′′′+=
′′+′++′=
′
′′
′′
′′
∫∫
∫∫
∫∫
(4.25)
Substituting Eq. (4.23) into Eq. (4.25), l* can be determined.
w
w
CBtotal
total
DDDl
′
′
+ ++
⎥⎦
⎤⎢⎣
⎡−
−=
µπµ
λλλ 4/12 2
21
* . (4.26)
b) Fracture aspect ratio is constant (α* = l / w′ = µl / µw′).
Then Eq.(4.24) is expressed as
84
where E(w′2) is the second moment of fracture apparent width probability density
function, which can be estimated by averaging all w′2 determined by Eq.(4.12).
Substituting Eq. (4.23) into Eq. (4.27), α* can be solved.
( ) w
w
CBtotal
total
DwEDD
′
′
+ +′+
⎥⎦
⎤⎢⎣
⎡−
−=
µπµ
λλλα 2
2
21
* 4/12
(4.28)
Finally, the mean fracture length can be estimated as:
w
ww
CBtotal
totalwl DwE
DD′
′′
+′
+′+
⎥⎦
⎤⎢⎣
⎡−
−==
µµπµ
λλλµαµ
)(4/12
2
22
21
* (4.29)
4.4.3 Summary of fracture length and width estimators
The estimators discussed in this section (Eqs. (4.10, 4.11, 4.19, 4.26, 4.29)) are
categorized in three cases, depending on the relative magnitudes of borehole/shaft
diameter D and fracture apparent width w′. Judgment should be made to determine
which estimator(s) will be applied to estimate fracture length and apparent width. The
flowchart in Fig. 4.10 shows how this procedure is carried out. Note that if there are no
C-type intersections, it is much likely that fracture apparent width is greater than
( ) ( )
( )
( ) ( )
( ) ( )
( ) ( ) 4/1
,4/
,1
,
,4/
2*2*
,,
2
,,
*
,,
2*
,,
2*2*
DDwE
wdldwlfD
wdldwlfwD
wdldwlfw
wdldwlfDwDwDw
w
wlWL
wlWL
wlWL
wlWLtotal
πηµαηηα
π
α
ηα
πααηλ
+++′=
′′+
′′′++
′′′=
′′+′+′+′=
′
′′
′′
′′
′′
∫∫
∫∫
∫∫
∫∫
(4.27)
85
borehole/shaft diameter. Estimators for the case 4.4.1 (Eqs. (4.10, 4.11)), therefore, can
be used to estimate fracture length and apparent width. If there are no A-type
intersections, on the other hand, it is much likely that fracture apparent width is less than
borehole/shaft diameter. Estimators for the case 4.4.2 (Eqs. (4.19, 4.26, 4.29)), can be
used, depending on whether the measured fracture apparent width is greater than
borehole/shaft radius or not.
In practice, when using the estimators, the ratios of expected frequencies can be replaced
by the ratios of the corresponding observed intersection counts. This is demonstrated in
the following example.
Fig. 4.10. Flowchart of choosing estimators to estimate mean fracture length and width.
Unrolled borehole/shaft trace map
Identify intersection types and their counts
No C-type intersections
Case 4.4.1: w′ > D
Both A and C intersections
Use judgment
Mean fracture length: Eq. (4.10) Mean fracture width: Eq. (4.11)
No A-type intersections
Case 4.4.2: w′ ≤ D
Determine mean fracture apparent width µw′ by averaging all w′ calculated by Eq. (4.12)
µw′ > D/2 ? Case 4.4.2.1
Case 4.4.2.2
Yes
NoMean fracture length: Eq. (4.19)
Mean fracture length: Eq. (4.26) or Eq. (4.29)
86
4.5 Examples
Example 1: suppose a 600.0 feet long, 6.0 inch in diameter vertical borehole was drilled
in a sedimentary rock mass. From borehole image, three sets of fractures were observed,
with an average dip of 35.0°, 60.0°, and 80.0°, respectively. The borehole-fracture
intersection types were identified by unrolled borehole images, and the counts of
intersections for each intersection type are listed in Table 4.4.
Table 4.4. Borehole-fracture intersection counts from a borehole sampling
Intersection counts Intersection type
Set 1 Set 2 Set 3
A 18 0 0
B1 105 233 58
B2 38 78 34
B3 57 63 62
C1 0 0 0
C2 0 55 21
Total number of intersections 218 429 175
Average dip 35.0 60.0 80.0
Borehole length (ft.) 600.0
Borehole diameter (in.) 6.0
Estimated mean fracture length l (ft) 2.0 2.4 1.0
Estimated mean fracture apparent width w′ (ft) 1.0 0.4 0.1
Estimated mean fracture width w (ft) 1.2 0.8 0.6
Estimated mean squared fracture width w′2 (ft2) 0.015
Estimated Aspect Ratio (l/w) 1.6 3.0 1.7
87
For fracture set 1, no C-type intersections were found. Therefore, we use estimators Eqs.
(4.10) and (4.11) for the case 4.4.1 (w′ > D) to estimate mean fracture length and width.
The ratios of expected intersection frequencies are replaced by the ratios of intersection
counts.
( )
( )
( )
ftin
NND
D
B
B
B
Bl
0.2.9.23
4342570
80.6
434~~
8
4348
3
1
3
1
==
⎥⎦⎤
⎢⎣⎡ +++=
⎥⎦
⎤⎢⎣
⎡+++≈
⎥⎦
⎤⎢⎣
⎡+++=
ππ
ππ
ππλλµ
(4.30)
and
( )
( )
( )
ftin
NND
D
B
B
B
Bw
0.1.1.12
4342518
80.6
434~~
8
4348
3
2
3
2
==
⎥⎦⎤
⎢⎣⎡ +++=
⎥⎦
⎤⎢⎣
⎡+++≈
⎥⎦
⎤⎢⎣
⎡+++=′
ππ
ππ
ππλλµ
(4.31)
Assume that fractures in set 1 are of constant orientation (dip = 35°), fracture true width
is estimated by
ftftww 2.1)35cos(/0.1cos/ =°== ′ ϕµµ . (4.32)
For fracture set 2, no A-type intersections were identified and the average fracture
apparent width is µw′ = 0.4 ft by averaging all values of fracture apparent width
88
determined by Eq. (4.12). We use estimator Eq. (4.19) for case 4.4.2.1 (D/2 < w′ ≤ D) to
estimate the mean fracture length.
( ) ( )
( ) ( )
( ) ( )
ftin
DDNNN
NN
DD
wCBtotal
CB
wCBtotal
CBl
4.2.5.28
480.64/0.68.0
55110204552110
48
4/~~~~2~
48
4/2
21
21
21
21
==
+++−−
×+=
+++−−
+≈
+++−−
+=
′
′
ππ
ππµ
ππµλλλ
λλµ
(4.33)
Assume that fractures in set 2 are of constant orientation (dip = 60°), fracture true width
is estimated by
ftftww 8.0)60cos(/4.0cos/ =°== ′ ϕµµ . (4.34)
For fracture set 3, no A-type intersections were identified and the average fracture
apparent width is µw′ = 0.1 ft by averaging all values of fracture apparent width
determined by Eq. (4.12) and E(w′2) = 0.015 ft2. By assuming that fractures are of
constant aspect ratio, we use estimator Eq. (4.29) for case 4.4.2.2 (w′ ≤ D/2) to estimate
the mean fracture length.
( )
( )
( )
ft
DwEDD
NNN
DwEDD
w
ww
CBtotal
total
w
ww
CBtotal
totall
0.1
1.05.0015.04/1.05.05.01.01
21581751752
)(4/1~~
~2
)(4/12
22
2
22
21
2
22
21
=
×+×+×
⎥⎦⎤
⎢⎣⎡ −
−−×
=
+′+
⎥⎦
⎤⎢⎣
⎡−
−≈
+′+
⎥⎦
⎤⎢⎣
⎡−
−=
′
′′
+
′
′′
+
π
µµπµ
µµπµ
λλλµ
(4.35)
89
Assume that fractures in set 3 are of constant orientation (dip = 80°), fracture true width
is estimated by
ftftww 6.0)80cos(/1.0cos/ =°== ′ ϕµµ . (4.36)
Example 2: a 10.4 inch in diameter borehole was drilled in a sedimentary rock mass.
From borehole FMI image, a set of fractures was observed, with an average dip of 82.3°.
The borehole-fracture intersection types were identified and the counts of intersections
for each intersection type are listed in Table 4.5.
Table 4.5. Borehole-fracture intersection counts from borehole sampling
Intersection type Intersection counts
A 17
B1 103
B2 21
B3 23
C1 0
C2 98
Total number of intersections 262
Average dip 82.3°
Borehole diameter (in) 10.4
Estimated mean fracture length l (in) 59.0 ~ 65.9
Estimated mean fracture apparent width w′ (in) 3.1
Estimated mean fracture width w (in) 23.1
Estimated mean squared fracture width w′2 (in2) 14.5
Estimated Aspect Ratio (l/w) 2.5 ~ 2.8
90
Although both A-type and C-type intersections were identified for this fracture set, C-
type intersection counts (98) are much higher than A-type intersection counts (17).
Therefore, w′ ≤ D (case 4.4.2) is assumed to be more suitable for this case. The average
fracture apparent width is µw′ = 3.1 in by averaging all values of fracture apparent width
determined by Eq. (4.12) and E(w′2) = 14.5 in2. Since µw′ is less than borehole radius (5.2
in), assuming that fractures are of constant aspect ratio, we use estimators Eq. (4.29) for
case 4.4.2.2 (w′ ≤ D/2) to estimate the mean fracture length.
( )
( )
( )
in
DwEDD
NNN
DwEDD
w
ww
CBtotal
total
w
ww
CBtotal
totall
0.591.34.105.14
4/1.34.104.101.3198103262
2622
)(4/1~~
~2
)(4/12
22
2
22
21
2
22
21
=×+
×+×⎥⎦⎤
⎢⎣⎡ −
−−×
=
+′+
⎥⎦
⎤⎢⎣
⎡−
−≈
+′+
⎥⎦
⎤⎢⎣
⎡−
−=
′
′′
+
′
′′
+
π
µµπµ
µµπµ
λλλ
µ
(4.37)
Assume that fractures are of constant orientation (dip = 82.3°), fracture true width is
estimated by
ininww 1.23)3.82cos(/1.3cos/ =°== ′ ϕµµ . (4.38)
4.6 Monte Carlo simulations
Monte Carlo simulations were carried out using a computer program developed in Visual
C++. The program generates a population of synthetic rectangular fractures intersected
by a borehole/shaft (Fig. 4.11). Fracture traces are computed (right-hand side window in
Fig. 4.11) and used to determine the occurrence of each borehole/shaft-fracture
91
intersection type. For each simulation, the size (length and width) of fractures and the
dimensions of borehole (length and diameter) are constant; and the total number of
generated fractures, the area of each fracture, as well as the size of the generation region,
were recorded. The observed counts of intersection types are used to estimate fracture
length and width by using Eqs. (4.10) and (4.11), or Eqs. (4.12) and (4.19), depending on
the relative size of borehole/shaft diameter D and fracture apparent width w′.
Twenty-seven scenarios (Table 4.6) were simulated by systematically changing fracture
dip ϕ (0º, 30º, and 60 º), length l (2, 10, and 20) and aspect ratio α (1, 2, and 10). For all
cases, the cylinder (borehole/shaft) diameter was held constant (D = 0.2), and the fracture
intensity P32 was held constant at 1.0 [L-1]. Depending on the mean size of the fracture,
the number of fractures varied from one scenario to the next. For each scenario, fifty
simulations were run; and the average estimated fracture length and width, and average
percent error, variance and coefficient of variation are listed in Table 4.6.
An example of simulation results for scenario 1 is shown in Fig. 4.12. In this scenario,
the length and width of the generated fractures are both set to be 2.0, i.e., the fractures are
square. In 50 simulations, there are an average of 354 B1-type intersections, 353 B2-type
intersections and 65 B3-type intersections observed. The estimated fracture length and
width are 2.04 and 2.02, by using Eqs. (4.10) and (4.11), respectively.
Overall, the simulation results (Table 4.6) show that the derived equations produce
reasonable, good estimates of fracture length and width (absolute percent error is less
than 15% of the actual fracture size). The largest errors occur for scenarios 4, 7, 13, 16,
22, and 25, in which the data are distorted by very low or even no occurrence of B3-type
intersections observed in some simulations. The comparison of percent error and
coefficient of variation versus observed B3-type intersection counts (Fig. 4.13) shows a
big increase of both error and variation of the estimators when the observed B3-type
intersection counts drops from 26 to 7. This suggests that cares should be taken when
92
applying these estimators in practice, especially when fractures are much larger than
borehole/shaft diameter and the counts of B3-type intersections is very low.
Fig. 4.11. A computer program was developed to generate a population of rectangular
fractures intersected by a borehole/shaft. In the simulation shown above, number of
fractures generated = 4796; fracture length = 2; aspect ratio = 1; dip/dip direction = 30
deg/north; borehole length = 10; borehole diameter = 0.2; fracture area per unit rock mass
volume = 5.0. The trace analysis produced 36 A-type intersections; 6 B1-type
intersections; 6 B2-type intersections; 1 B3-type intersections; 0 C1-type intersections; 0
C2-type intersections.
Borehole
Trace map
Fractures
123
4
5
6
7
8
9
1011
93
Table 4.6. Parameters and results of Monte Carlo simulations
Ave
rage
d nu
mbe
r of
inte
rsec
tions
Est
imat
ed fr
actu
re
leng
th [L
]
Est
imat
ed fr
actu
re
wid
th [L
]
Sce
nario
Dip
Frac
ture
leng
th [L
]
Frac
ture
wid
th [L
]
Asp
ect R
atio
App
aren
t wid
th [L
]
Num
ber o
f fra
ctur
es
gen
erat
ed
Frac
ture
den
sity
(P30
) [L-3
]
A
B1
B2
B3
C2
Tota
l
Ave
rage
Abs
olut
e pe
rcen
t er
ror
Var
ianc
e
Coe
ffici
ent o
f va
riatio
n
Ave
rage
Abs
olut
e pe
rcen
t er
ror
Var
ianc
e
Coe
ffici
ent o
f va
riatio
n
1 0° 2 2 1 2 3673 0.25 1569 354 353 65 0 2341 2.0 2% 0.08 14% 2.0 1% 0.08 14%
2 0° 2 1 2 1 4754 0.50 1443 735 329 134 0 2640 2.0 2% 0.03 9% 1.0 1% 0.01 8%
3 0° 2 0.2 10 0.2 19562 2.50 0 3660 45 665 0 4369 2.0 1% 0.01 5% 0.2 1% 0.00 2%
4 0° 10 10 1 10 3295 0.01 1917 77 78 3 0 2075 12.2 22% 55.56 61% 12.3 23% 56.94 62%
5 0° 10 5 2 5 4150 0.02 1884 157 79 6 0 2125 11.7 17% 60.40 66% 6.0 21% 21.01 76%
6 0° 10 1 10 1 16832 0.10 1566 794 66 26 0 2451 10.9 9% 4.76 20% 1.1 6% 0.04 19%
7 0° 20 20 1 20 3249 0.00 1955 40 41 1 0 2036 11.6 42% 12.00 30% 11.5 43% 10.77 29%
8 0° 20 10 2 10 4077 0.01 1939 79 40 1 0 2058 20.3 2% 62.12 39% 10.3 3% 16.46 39%
9 0° 20 2 10 2 16505 0.03 1783 400 37 7 0 2227 24.4 22% 137.81 48% 2.4 21% 1.18 45%
10 30° 2 2 1 1.73 3673 0.25 1374 366 316 66 0 2121 2.1 4% 0.07 13% 2.1 5% 0.07 12%
11 30° 2 1 2 0.87 4754 0.50 1198 730 276 134 0 2338 2.0 1% 0.03 9% 1.0 1% 0.01 8%
12 30° 2 0 10 0.17 19562 2.50 0 3162 27 610 239 4038 2.0 0% 0.01 4% 0.2 0% 0.00 0%
13 30° 10 10 1 8.66 3295 0 1654 81 70 2 0 1807 13.4 34% 59.92 58% 13.4 34% 61.76 58%
14 30° 10 5 2 4.33 4150 0.02 1623 156 65 6 0 1850 10.5 5% 44.11 63% 5.1 2% 12.34 69%
15 30° 10 1 10 0.87 16832 0.10 1308 793 55 28 0 2184 10.1 1% 3.67 19% 1.0 1% 0.03 18%
16 30° 20 20 1 17.3 3249 0.00 1692 39 34 1 0 1766 10.5 47% 14.20 36% 10.8 46% 16.40 38%
17 30° 20 10 2 8.66 4077 0.01 1677 81 34 1 0 1794 19.3 3% 70.41 43% 9.7 3% 21.64 48%
18 30° 20 2 10 1.73 16505 0.03 1513 396 32 7 0 1947 22.4 12% 101.61 45% 2.3 13% 1.09 46%
19 60° 2 2 1 1 3673 0.25 717 365 163 64 0 1309 2.1 5% 0.06 12% 2.1 4% 0.06 12%
20 60° 2 1 2 0.5 4754 0.50 539 725 128 133 0 1525 2.0 1% 0.02 7% 1.0 1% 0.00 7%
21 60° 2 0.2 10 0.1 19562 2.50 0 1847 6 381 896 3130 2.0 1% 0.01 4% 0.2 0% 0.00 0%
22 60° 10 10 1 5 3295 0.01 943 79 37 2 0 1062 14.1 41% 63.84 57% 13.2 32% 55.09 56%
23 60° 10 5 2 2.5 4150 0.02 901 156 40 6 0 1103 11.3 13% 64.42 71% 5.9 19% 13.07 61%
24 60° 10 1 10 0.5 16832 0.10 590 788 26 27 0 1432 10.2 2% 4.14 20% 1.0 2% 0.05 21%
25 60° 20 20 1 10 3249 0.00 971 41 20 1 0 1033 11.8 41% 17.73 36% 11.5 43% 20.33 39%
26 60° 20 10 2 5 4077 0.01 949 81 20 1 0 1051 21.7 9% 51.16 33% 11.3 13% 25.64 45%
27 60° 20 2 10 1 16505 0.03 800 398 17 7 0 1223 22.9 14% 123.09 48% 2.3 14% 0.92 42%
Diameter of borehole/shaft [L] 0.2
Fracture area per unit rock mass volume (P32) [L-1] 1
Simulations per scenario 50
94
Fig. 4.12. Comparison of computed fracture length and width vs. actual fracture length
and width for scenario 1. Fracture dip = 0°; length = 2.0; aspect ratio = 1.0.
0
1
2
3
0 10 20 30 40 50
Simulations
Leng
th
Estimated LengthAverage Estimated LengthActual Length
0
1
2
3
0 10 20 30 40 50
Simulations
Wid
th
Computed WidthAverage Estimated WidthActual Width
95
Fig. 4.13. Percent error and coefficient of variation of estimators for (a) fracture length
and (b) fracture width, in comparison with observed counts of B3-type borehole/shaft-
fracture intersections.
(a)
(b)
0
100
200
300
400
500
600
700
0%
10%
20%
30%
40%
50%
60%
70%
80%
# of B3 intersectionsAbsolute percent errorCoefficient of variation
Scenarios
B3
inte
rsec
tion
coun
ts
Per
cent
err
or o
r co
effic
ient
ofva
riatio
n
26 B3 intersection
7 B3 intersection
0
100
200
300
400
500
600
700
0%
10%
20%
30%
40%
50%
60%
70%
80%
# of B3 intersectionsAbsolute percent errorCoefficient of variation
Scenarios
B3
inte
rsec
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coun
ts
Per
cent
err
or o
r co
effic
ient
ofva
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n
26 B3 intersection
7 B3 intersection
96
The fracture apparent widths in Scenario 12 and 21 are 0.17 and 0.10, respectively, which
are less than borehole diameter (0.2). The estimators (Eqs. (4.12) and (4.19)) for case D
≥ w′ > D/2 give very good estimates for fracture width and length (Table 4.6). In
addition, estimator (Eq. (4.10)) for case w′ > D were also used to estimate fracture length
and resulted an estimated length of 1.9 and 1.8 for scenario 12 and 21, respectively. The
percent errors are 4% and 10%, respectively, which implies that it will not cause major
errors by using Eq. (4.10) to estimate fracture length even if fracture apparent width is
smaller than borehole/shaft diameter.
4.7 Discussion & Conclusions
The goal of this study was to develop a general model for estimating mean rectangular
fracture length and width from traces on cylinder walls. Fractures in sedimentary rocks
are commonly elongated along strike and terminated on bedding planes or primary joint
sets, therefore assumed rectangular in shapes. From the geometric relations between a
fracture and a borehole/shaft, six types of intersection are defined. The features of each
intersection type described in the paper can be used to identify the six intersection types
from unrolled borehole/shaft trace maps. The occurrences of the intersection types are
related to fracture size and borehole/shaft diameter, assuming independence between
locations of borehole/shaft and the fractures.
Three cases regarding relations between fracture apparent width and the borehole/shaft
diameter are discussed. For each case, estimators are derived to estimate mean fracture
length and width based on probabilistic models. The estimators are confirmed by Monte
Carlo simulations, which gave satisfactory results. It is also pointed out in the paper that
caution should be used when applying the estimator to the cases that the size of the
sampled fractures is much larger than the diameter of boreholes/shafts.
97
Acknowledgements
Partial support from the National Science Foundation, Grant Number CMS-0085093, is
gratefully acknowledged. Also should be acknowledged are Chris Heiny from University
of Tennessee and Jeramy Decker from Virginia Tech, who helped carrying out
simulations.
98
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Chapter 5
5 Conclusions and discussions
Based on the stereological analyses and numerical simulation results of sampling
fractures by a line, a plane, and most important, cylindrical surfaces, the following
conclusions are drawn:
1. For linear sampling in constant sized or unbounded fractures with orientation
given by the Fisher distribution, the conversion factor C13 [1.0, ∞] between the
fracture linear intensity and the volumetric intensity is a function of the angle
between the sampling line and the Fisher mean pole, and the Fisher constant κ.
2. For planar sampling in constant sized or unbounded fractures with orientation
given by the Fisher distribution, the conversion factor C23 [1.0, ∞] between the
fracture areal (planar) intensity and the volumetric intensity is a function of the
angle between the normal of the sampling plane and the fracture Fisher mean pole,
and the Fisher constant κ.
3. For cylindrical surface sampling in constant sized or unbounded fractures with
orientation given by the Fisher distribution, the conversion factor C23,C [1.0, π/2]
between the fracture areal (cylindrical surface) intensity and the volumetric
intensity is a function of the angle between the axis of the sampling cylinder
(borehole) and the fracture Fisher mean pole, and the Fisher constant κ.
4. For a general case of cylindrical surface sampling of fractures, the conversion
factor C23,C [1.0, π/2] between the fracture areal (cylindrical surface) intensity and
the volumetric intensity is only a function of orientation of cylinder axis relative
to the fracture system and the pdf of fracture orientation weighted by area. It is
independent of fracture size or shape, or the sampling cylinder size.
104
5. Cycloidal scanlines, when deployed on the cylinder surface in a certain pattern,
give directional unbiased estimates of fracture volumetric intensity. Fracture
orientation information is not required by using this technique.
6. Fractures in sedimentary rocks can be approximated rectangular in shapes and the
estimators for their mean length and width are derived for three cases. The
estimators are independent of fracture size distributions.
The author also recommends the following work to be done in the future.
1. Interpretation of fracture traces to estimate other fracture properties, such as
roughness, connectivity, and so on, by means of stereology.
2. Study on fracture trace length distribution on borehole walls. It may be another
way to make estimates of fracture size, based on the assumptions of fracture
shapes.
3. Apply the conversion factors of fracture intensities and the estimators of fracture
size to real fracture trace data. Find ways to verify the obtained results.
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6 Appendix: Programs used in the dissertation
Two programs were used in this dissertation to carry out Monte Carlo simulations.
A. FISHER - Simulate the Fisher distribution
This program was developed by using Microsoft Excel. The inputs for this program are
listed in the table below.
Table App-1. Inputs for generating the Fisher distribution.
Input Range
Fisher constant, κ [0.1, 700]
Number of fracture poles, N [0, 3000]
Fisher mean pole dip [0, 90]
Fisher mean pole dip-direction [0, 360]
To simulate a fracture normal given by the Fisher distribution, first we rotate the Fisher
mean pole to be upward (Fig. 2.A-1). A random number (between 0 and 1) is generated,
and by using the cdf of the Fisher distribution (Eq. (2.B-3)), angle δ, the angle between a
fracture normal and the Fisher mean pole, is calculated. This angle and another generated
random number between 0 and 360 define a unique orientation in the coordinate system
shown in Fig. 2.A-1. The dip and dip-direction of the simulated fracture are then
calculated from the paired angles by rotating the upward axis back to the Fisher mean
pole. An example of the simulated Fisher distributed fracture normals is shown in Fig.
2.4. This program was used to study linear and planar samplings of the Fisher distributed
fractures.
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B. TRACE - Simulate fracture population sampled by a borehole
The program was developed in Visual C++. OpenGL was used to visualize the simulated
fracture population and the borehole in three-dimensional graphics (Figs. 3.8 and 4.11).
In this program, fractures are rectangular in shape and borehole is considered as a
cylinder. The parameters user may change are listed in Table App-2.
Table App-2. Parameters for simulating fractures sampled by a borehole.
Parameter Range
Fracture length, f_l > 0
Fracture aspect ratio, α > 1.0
Fracture width, f_w f_w = α × f_l
Fracture Dip, or dip of the Fisher mean pole [0, 90]
Fracture dip-direction, or dip-direction of the Fisher
mean pole [0, 360]
Fisher constant, κ > 0
Generation region shape Box, Cylinder, Ball
Fracture volumetric intensity, P32 > 0
Number of fractures, N > 0
Borehole (sampling cylinder) length, c_l > 0
Borehole (sampling cylinder) radius, c_r > 0
Borehole plunge [0, 90]
Borehole trend [0, 360]
User may fix the number of fractures to be generated or fix fracture volumetric intensity
and let the program calculate the number of fractures. The generation region, i.e., a box,
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a cylinder, or a ball (Fig. App-1), is a region in which the centers of generated fractures
are located. The sampling region refers to the region that the sampling cylinder (borehole)
is within. The relationship between sampling region and generation region is showed in
Fig. App-1. Note that the maximum fracture dimension is: max_f_l = 22 __ lfwf + ;
the maximum sampling cylinder dimension is max_c_l = 22 _4_ rclc + .
Fig. App-1. The geometry of fracture, sampling cylinder, and three different shapes of
generation region.
l_Box l_Cylinder
R_Cylinder
R_Ball
Generation CylinderGeneration Box Generation Ball
2 c_r
c_l f_w
f_l
max_f_l
Largest fracture Sampling cylinder
max_c_l
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Given dimensions of the largest fracture and sampling cylinder, the minimum size of
generation region varies with the shape of the region. The dimensions for different
shaped generation regions are listed in Table App-3.
Table App-3. Minimum dimension of different generation regions
Region shape Length Radius
Box lflc _max__max_ + -
Cylinder lclflclc _max_/)_max__(max__ + lfRc _max__ +
Ball - 2/)_max__(max_ lflc +
In three shapes of generation region, generation box is the simplest. The algorithm of
calculating fractures truncated by the region boundaries is also simple. Generation
cylinder is for the case that no rotation of the sampling cylinder is involved, while
generation ball allows rotation of the sampling cylinder.
After generating a set of synthetic fractures, the program computes the intersections
between the sampling cylinder and the rectangular fractures. Fracture traces are shown
on an unrolled trace map (Figs. 3.8 and 4.11). The outputs (in a text file) of the program
includes: fracture volumetric intensity (either set by the user, or calculated by the
program), fracture areal intensity on the borehole surface (calculated by the program by
dividing the total trace length by the cylinder area), and count of each intersection type.
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7 Xiaohai Wang
EDUCATION
Ph.D., Civil Engineering, Virginia Polytechnic Institute and State University, December 2005
Ph.D., Rock Mechanics & Rock Engineering, Institute of Soil & Rock Mechanics, Chinese Academy of Sciences, September 1999
M.S., Mining Engineering, Taiyuan University of Technology, 1996 B.S., Mining Engineering, Taiyuan University of Technology, 1993
RESEARCH AND WORK EXPERIENCE
Research
Research assistant, Department of Civil & Environmental Engineering, Virginia Tech, Blacksburg, VA August 2001 – September 2005 • Characterization of rock fractures based on cylindrical samples, supported by National
Science Foundation • Scanline bias estimate and techniques to minimize the directional bias in cylindrical
sampling • Techniques to estimate fracture size and aspect ratio in sedimentary rocks • Computer simulation of rock mass fractures with three-dimensional visualization • Computer program to deploy unbiased scanlines on fracture trace maps and characterize
fractures
Research Fellow, Institute of Soil & Rock Mechanics, Chinese Academy of Sciences, Wuhan, China August 1998 – May 2001 • Integration of Three-dimensional Strata Information System (3DSIS), supported by
Chinese Academy of Sciences • Strata geological structure analysis and modeling Research Assistant, Department of Mining Engineering, Shanxi Mining Institute, Taiyuan, Shanxi, China August 1994 – July 1996 • Fractals of distribution features of rock mass fissures, supported by Shanxi Natural
Science Foundation
Teach
Teaching Assistant, Department of Civil & Environmental Engineering, Virginia Tech, Blacksburg, VA May 2004 – July 2004 • Assist teaching the Intensive Summer Course in Geology Engineering & Rock
Mechanics for the US Army Corps of Engineers Work
112
Programmer, Institute of Soil & Rock Mechanics, Chinese Academy of Sciences, Wuhan, China August 1999 – May 2001 • Develop the visualization module for program Three-dimensional Limit Equilibrium
Method in Slope Stability Analysis • Design and develop the program Supporting System in Deep Foundation Excavation
PUBLICATIONS
Wang, Xiaohai, M. Mauldon, W. Dunne. Estimating size and aspect ratio of rectangular fractures from traces on cylindrical rock exposures. (for submission to Rock Mechanics & Rock Engineering)
Mauldon, Matthew, X. Wang. Estimating fracture intensity from traces on cylindrical exposures. (for submission to International Journal of Rock Mechanics & Mining Sciences)
Wang, Xiaohai, M. Mauldon, and W. S. Dershowitz. Multi-dimensional intensity measures for Fisher-distributed fractures. (submitted to Mathematical Geology, May 2005)
Wang, Xiaohai, M. Mauldon, W. Dunne, C. Heiny. 2005. Extracting fracture characteristics from piercing-type intersections on borehole walls. In: Proceedings of the 40th U.S. Symposium on Rock Mechanics (USRMS) (2005), Anchorage, Alaska.
Wang, X., M. Mauldon, W. Dunne, C. Heiny. 2004. Using Borehole Data to Estimate Size and Aspect Ratio of Subsurface Fractures. In: Proceedings of the 6th North American Rock Mechanics Symposium (NARMS), Houston, Texas
Mauldon, M. and X. Wang. 2003. Measuring Fracture Intensity in Tunnels Using Cycloidal Scanlines. In: Proceedings of the 12th Pan-Am. Conf on Soil Mech & Geotech Eng. & 39th U.S. Rock Mech Symp. Soil & Rock America 2003, Culligan, Einstein & Whittle, eds., Boston: Vol. 1, 123-128
Jiang, Q., X. Wang, D. Feng, S. Feng. 2003. Three Dimensional Limit Equilibrium Analysis System Software 3D_SLOPE for Slope Stability and its Application. Chinese Journal of Rock Mechanics and Engineering. 22 (7): 1121-1125
Mauldon, M., X. Wang, D. Peacock. 2002. Fracture frequency predictions using double-corrected data. In: Proc. of the 5th North American Rock Mechanics Symp. And the 17th Tunnelling Association of Canada Conference: NARMS-TAC 2002, Hammah, R. et al. ed., Toronto, Canada: 27-34
Jiang, Q., M.R. Yeung, X. Wang, D. Feng. 2002. Development of the interactive visualization system for three dimensional slope stability analysis. In: Proc. of the 9th Congress of the International Association of Engineering Geology and the Environment, Durban, September 16-20, 244-252
Zhao, Y., X. Wang, K. Duan, D. Yang. 2002. Unsymmetry of scale transformation of rock mass anisotropy, Chinese Journal of Rock Mechanics and Engineering, Vol. 21. No. 11: 1594-1597
Zhang, Y., X. Wang, J. Chen, S. Bai. 2000. Application of 3D Volume Visualization in Geology, Journal of Rock Mechanics & Engineering (in Chinese), Vol. 20. No. 5.
Wang, X., S. Bai. 1999. 3D Topological Grid Data Structure for Modeling Subsurface In: Proc. of International Symposium on Spatial Data Quality (ISSDQ 1999), Hong Kong.
113
Wang, X., S. Bai, Z. Gu. 1998. The Problems in the Applications of GIS in Rock and Soil Projects. Research and Practice in Rock and Soil Mechanics. Zhengzhou.
Wang, X., S. Bai. 1998. An Easily Integrated Three-dimensional Data Structure in Strata Modeling. In: Proceedings of International Conference on Modeling Geographical and Environmental Systems with Geographic Information Systems. Hong Kong
Zhao, Yangsheng, X. Wang, K. Duan. 1997. The Scale-invariability of the Distribution of Rock Mass Fissures. Modern Mechanics and Technology Progressing. Beijing.
AWARDS / AFFILIATION
Graduate Research Development Project Grant, Virginia Polytechnic Institute & State University, 2003-2004
Outstanding poster presenter, 20th Annual Graduate Student Assembly Research Symposium & Exposition, Virginia Polytechnic Institute & State University, 2004
Best poster (tied), 6th North American Rock Mechanics Symposium (NARMS), June 6-10, Houston, TX, 2004
Member of American Rock Mechanics Association, 2004, 2005