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Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
73
Conceptual Overview of Rock
and Fluid Factors that Impact
Seismic Velocity and Impedance
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
74
Typical rock velocities, from Bourbié, Coussy, and
Zinszner, Acoustics of Porous Media, Gulf Publishing.
Type of formation P wave
velocity
(m/s)
S wave
velocity
(m/s)
Density
(g/cm3
)
Density of
constituent
crystal
(g/cm3
)
Scree, vegetal soil 300-700 100-300 1.7-2.4 -
Dry sands 400-1200 100-500 1.5-1.7 2.65 quartz
Wet sands 1500-2000 400-600 1.9-2.1 2.65 quartz
Saturated shales and clays 1100-2500 200-800 2.0-2.4 -
Marls 2000-3000 750-1500 2.1-2.6 -
Saturated shale and sand sections 1500-2200 500-750 2.1-2.4 -
Porous and saturated sandstones 2000-3500 800-1800 2.1-2.4 2.65 quartz
Limestones 3500-6000 2000-3300 2.4-2.7 2.71 calcite
Chalk 2300-2600 1100-1300 1.8-3.1 2.71 calcite
Salt 4500-5500 2500-3100 2.1-2.3 2.1 halite
Anhydrite 4000-5500 2200-3100 2.9-3.0 -
Dolomite 3500-6500 1900-3600 2.5-2.9 (Ca, Mg)
CO32.8-2.9
Granite 4500-6000 2500-3300 2.5-2.7 -
Basalt 5000-6000 2800-3400 2.7-3.1 -
Gneiss 4400-5200 2700-3200 2.5-2.7 -
Coal 2200-2700 1000-1400 1.3-1.8 -
Water 1450-1500 - 1.0 -
Ice 3400-3800 1700-1900 0.9 -
Oil 1200-1250 - 0.6-0.9 -
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
75
The Saturation and Pressure Dependence of
P- and S-wave Velocities.
F.1
3
4
5
6
7
0 100 200 300
Webatuck dolomite
Velocity(km/s)
Effective Pressure (bars)
S a t .
S a t .
Dry
Dry
V
P
V
S
1
2
3
4
5
6
0 100 200 300
Bedford Limestone
Velocity(km/s)
Effective Pressure (bars)
S a t .
Dry
Dry
S a t .
VP
VS
Crack shape
Number
of cracks
2
3
4
5
6
0 100 200
Solenhofen limestone
Velocity(km/s)
Effective Pressure (bars)
V
S
V
PSat. and Dry
Sat. and Dry
2
3
4
5
6
7
0 100 200 300
Westerly Granite
Velocity(km/s)
Effective Pressure (bars)
Dry
S a t .
V
P
V
S
Dry
S a t .Flat asymptoteWater-saturated
Saturated
Velocity(km/s)
Velocity(km/s)
Velocity(km/s)
Velocity(km/s)
Effective Pressure (bars)
Effective Pressure (bars)
Effective Pressure (bars)
Effective Pressure (bars)
Bedford Limestone Westerly Granite
Solenhofen Limestone
Webatuck Dolomite
Peffective = Pconfining − Ppore
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
76
Fundamental Observations of Rock Physics
• Velocities almost always increase with effective
pressure. For reservoir rocks they often tend toward
a flat, high pressure asymptote.
• To first order, only the difference between confining
pressure and pore pressure matters, not the absolute
levels of each -- ”effective pressure law.”
• The pressure dependence results from the closing of
cracks, flaws, and grain boundaries, which elastically
stiffens the rock mineral frame.
• The only way to know the pressure dependence of
velocities for a particular rock is to measure it.
• Make ultrasonic measurements on dry cores; fluid-
related dispersion will mask pressure effects.
• The amount of velocity change with pressure is a
measure of the number of cracks; the pressure range
needed to reach the high pressure asymptote is a
measure of crack shape (e.g. aspect ratio).
• Velocities tend to be sensitive to the pore fluid
content. Usually the P-wave velocity is most
sensitive and the S-wave velocity is less sensitive.
• Saturation dependence tends to be larger for soft
(low velocity) rocks.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
77
Pressure-Dependence of Velocities
It is customary to determine the pressure dependence of
velocities from core measurements. A convenient way to
quantify the dependence is to normalize the velocities for
each sample by the high pressure value as shown here.
This causes the curves to cluster at the high pressure point.
Then we fit an average trend through the cloud, as shown.
The velocity change between any two effective pressures
P1 and P2 can be conveniently written as:
Vp and Vs often have a different pressure behavior, so
determine separate functions for them.
Remember to recalibrate this equation to your own cores!
F29
Remember: Calibrate to Dry Cores!
Vp
Vp(40)
=1.0 −0.40 *exp(−Peff /11)
Vs
Vs(40)
=1.0 − 0.38* exp(−Peff /12)
V(P2)
V(P1)
=
1.0 − 0.38exp(−P2 /12)
1.0 − 0.38exp(−P1/12)
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
78
Replace Gas with Water Gas Water Difference
Increase Pp by 100 bars
4D Example: Deep, Stiff, Gas Sand
F32
Small
impedance
increase from
fluids
Modest
impedance
decrease
from pressure
Trajectories in the AVO plane
Increasing Pp Increasing Sw
Before After Difference
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
79
Replace Gas with Water Gas Water Difference
Increase Pp by 100 bars
4D Example: Deepwater, Soft, Gas Sand
F32
Before After Difference
Large
impedance
increase
Small
impedance
decrease
Trajectories in the AVO plane
Increasing Pp
Increasing Sw
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
80
Effects of Pore Fluid on P-wave Velocity (Low Frequency)
Calculations made from dry velocities, using Gassmann relation,
Kmin = 36 GPa, Kwater = 2.2, Koil = 1.
Density does not lead to ambiguity
when Impedance is measured. lmp = ρV = ρ × modulus
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
81
Beaver Sandstone
6% porosity
Effects of Pore Fluid on P-wave Velocity (Low Frequency)
Fontainebleau Sandstone
15% porosity
F.4
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
82
Velocities depend on fluid modulus and
density
• When going from a dry to water saturated rock,
sometimes the P-velocity increases; sometimes it
decreases.
• The rock elastic bulk modulus almost always
stiffens with a stiffer (less compressible) pore fluid.
• The stiffening effect of fluid on rock modulus is
largest for a soft (low velocity) rock.
• The bulk density also increases when going from a
dry to water-saturated rock.
• Because velocity depends on the ratio of elastic
modulus to density, the modulus and density
effects “fight” each other; sometimes the velocity
goes up; sometimes down.
• Measures of modulus ( ), impedance
( ), and don’t have
the density effect “ambiguity.”
• Be careful of ultrasonic data! At high frequencies,
the elastic-stiffening effect is exaggerated for both
bulk and shear moduli; so we don’t often see the
density effect in the lab and the velocities will be
contaminated by fluid-related dispersion.
M = ρV 2
lmp = ρV = ρ modulus VP /VS
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
83
Beaver Sandstone
6% porosity
Effect of Pore Pressure
Effect of pore pressure on velocity,
calculated assuming effective pressure law
is valid, and assuming a fixed confining
pressure of 40MPa (low frequency
calculations using Gassmann relation).
4.4
4.6
4.8
5
5.2
5.4
0 5 1 0 1 5 2 0 2 5 3 0 3 5 4 0
Velocity(km/s)
Pore Pressure (MPa)
dry
oil
water
F.6
Increasing pore
pressure
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
84
Ways that Pore Pressure
Impacts Velocities
• Increasing pore pressure softens the elastic
mineral frame by opening cracks and flaws,
tending to lower velocities.
• Increasing pore pressure tends to make the
pore fluid or gas less compressible, tending to
increase velocities.
• Changing pore pressure can change the
saturation as gas goes in and out of solution.
Velocities can be sensitive to saturation.
• High pore pressure persisting over long
periods of time can inhibit diagenesis and
preserve porosity, tending to keep velocities
low.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
85
Ultrasonic velocities and porosity in Fontainebleau sandstone
(Han, 1986). Note the large change in velocity with a very
small fractional change in porosity. This is another indicator
that pressure opens and closes very thin cracks and flaws.
Pressure Dependence of Velocities
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
86
Dry shaly sandstone data from Han (1986). Each vertical
“streak” plotted with the same symbol is a single rock at
different pressures. Note the large change in modulus with
little change in porosity -- another illustration that cracks and
flaws have a large change on velocity, even though they
contribute very little to porosity.
Only the values at high pressure and with Han's empirical
clay correction applied. F.8
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
87
The Information in a Rock's
Velocity-Pressure Curve
1. High pressure limiting velocity is a function of
porosity
2. The amount of velocity change with pressure
indicates the amount of soft, crack-like pore space
3. The range of the greatest pressure sensitivity
indicates the shape or aspect ratios of the crack-
like pore space
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
88
Soft, Crack-Like Porosity
1. Includes micro and macrofractures and
compliant grain boundaries.
2. Soft Porosity:
• Decreases both P and S-wave velocities
• Increases velocity dispersion and attenuation
• Creates pressure dependence of V and Q
• Creates stress-induced anisotropy of V and Q
• Enhances sensitivity to fluid changes
(sensitivity to hydrocarbon indicators)
3. High confining pressure (depth) and cementation,
tend to decrease the soft porosity, and therefore
decreases these effects.
4. High pore pressure tends to increase the soft
porosity and therefore increases these effects.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
89
Curves on the left show the typical increase of velocity with effective
pressure. For each sample the velocity change is associated with the
opening and closing of cracks and flaws. These are typical when rapid
changes in effective pressure occur, such as during production.
Curves on the right show the same data projected on the velocity- porosity
plane. Younger, high porosity sediments tend to fall on the lower right.
Diagenesis and cementation tend to move samples to the upper left
(lower porosity, higher velocity). One effect of over- pressure is to inhibit
diagenesis, preserving porosity and slowing progress from lower right to
upper left. This is called “loading” type overpressure. Rapid, late stage
development of overpressure can open cracks and grain boundaries,
resembling the curves on the left. This is sometimes called “transient” or
“unloading” overpressure. In both cases, high pressure leads to lower
velocities, but along different trends.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
90
Seismic Velocity and Overpressure
A typical approach to overpressure analysis is to look for
low velocity deviations from normal depth trends. Caution:
when overpressure is “late stage,” estimates of pressure
can be too low.
F31
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
91
Experiments that illustrate the effective pressure law. In the first part of
the experiment, effective pressure is increased by increasing confining
pressure from 0 to 80 MPa, while keeping pore pressure zero (solid dots).
Then, effective pressure is decreased by keeping confining pressure fixed
at 80 MPa, but pumping up the pore pressure from 0 to nearly 80 MPa
(open circles). (Jones,1983.)
The curves trace approximately (but not exactly) the same trend. There is
some hysteresis, probably associated with frictional adjustment of crack
faces and grain boundaries. For most purposes, the hysteresis is small
compared to more serious difficulties measuring velocities, so we assume
that the effective pressure law can be applied. This is a tremendous
convenience, since most laboratory measurements are made with pore
pressure equal 0.
F.9
2.5
3
3.5
4
4.5
5
0 20 40 60 80
St. Peter sandstone
Velocity(km/s)
Effective Pressure (MPa)
p
c
=80 MPa
p
c
=80 MPa
p
p
=0
p
p
=0
VP
VS
2.6
2.8
3
3.2
3.4
3.6
0 20 40 60 80
Sierra White granite
Velocity(km/s)
Effective Pressure (MPa)
p
p
=0
p
c
=80 MPa
VS
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
92
Pierre shale (ultrasonic), from Tosaya, 1982.
F.11
For shales, we also often see an increase of velocity with
effective pressure. The rapid increase of velocity at low
pressures is somewhat elastic, analogous to the closing of
cracks and grain boundaries that we expect in sandstones.
The high pressure asymptotic behavior shows a continued
increase in velocity rather than a flat limit. This is probably
due to permanent plastic deformation of the shale.
0.5
1
1.5
2
2.5
3
3.5
4
0 5 0 100 150 200
Velocity(km/s)
Confining Pressure (MPa)
p
p
=1MPa
p
p
=41 MPa
pp
=0
p
p
=0
pp
=1MPa
V P
V S
S a t .
S a t .
D r y
D r y
p
p
=41 MPa
Velocity(km/s)
Confining Pressure (MPa)
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
93
transducer
transducer
Rock
sample
Jacket
Confining
pressure
Pore
pressure
transducer
transducer
Concept of
Induced Pore Pressure
∆σ = 1bar
∆Pp ~ 0.2bar
∆Pp ~ 1bar
Stiff Pore
Soft Pore
We expect a small
induced pressure
in stiff pores
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
94
Chalk (ultrasonic), from Gregory, 1976, replotted from Bourbié,
Coussy, and Zinszner, 1987, Gulf Publishing Co.
F.12
For chalks, we also see an increase of velocity with
effective pressure. The rapid increase of velocity at
low pressures is somewhat elastic and reversible.
The high pressure asymptotic behavior shows a
continued increase in velocity rather than a flat limit.
This is probably due to permanent crushing of the
fragile pore space.
1.5
2
2.5
3
3.5
0 1 0 2 0 3 0 4 0 5 0
Chalk
Velocity(km/s)
Effective Pressure (MPa)
Sw
100
0
5
10
20
40
80
60
V P
V S
5
φ = 30.6%
Velocity(km/s)
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
95
Influence of temperature on oil saturated samples,
from Tosaya, et al. (1985).
F.16
We observe experimentally that velocities are most
sensitive to temperature when the rocks contain
liquid hydrocarbons (oil). We believe that this results
from an increase of the oil compressibility and a
decrease of the oil viscosity as the temperature goes
up.
In field situations other factors can occur. For
example, gas might come out of solution as the
temperature goes up.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
96
An Early, Successful 4D Field Study
Thermal Signature of Steam Flood
From DeBuyl, 1989
Traveltime increase in
steamed interval after a few
months of steam injection.
After a few more months,
the anomaly spreads.
F30
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
97
Velocity vs. viscosity in glycerol saturated samples,
from Nur (1980).
F.17
Temperature
Temperature
In this experiment the pore fluid is glycerol, whose viscosity
is extremely sensitive to temperature. The data show a
classical viscoelastic behavior with lower velocity at low
viscosity and higher velocity at higher viscosity. Viscosity is
one of several pore fluid properties that are sensitive to
temperature.
0.5
0.6
0.7
0.8
0.9
1
1.1
-4 -2 0 2 4 6 8 10
Barre granite
µ/µο
Log viscosity (poise)
Bedford limestone
0.7
0.8
0.9
1
-4 -2 0 2 4 6 8 10
Bedford limestone
Vp
Vs
V/Vo
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
98
Compressional velocities in the n-Alkanes vs. temperature.
A drastic decrease of velocity with temperature! The
numbers in the figure represent carbon numbers. From
Wang, 1988, Ph.D. dissertation, Stanford University.
F.18
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
99
Compressional velocities in the n-Alkanes vs. inverse of the
carbon numbers, at different temperatures. From Wang, 1988,
Ph.D. dissertation, Stanford University.
F.19
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
100
Batzle-Wang formulas for fluid density and bulk
modulus (Geophysics, Nov. 1992).
F30
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
101
F30
API =141.5
ρO
−131.5
1 l/l = 5.615 ft
3
/bbl
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
102
F30
BrineBulkModulus(Gpa)BrineDensity(kg/m3)
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
103
BubblePoint computed using Batzle, Wang Relations
Caution: Calibrate to lab
data when possible!
F30
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
104
Soft
Deepwater
Sands
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
105
Fluid Properties
• The density and bulk modulus of most reservoir
fluids increase as pore pressure increases.
• The density and bulk modulus of most reservoir
fluids decrease as temperature increases.
• The Batzle-Wang formulas describe the empirical
dependence of gas, oil, and brine properties on
temperature, pressure, and composition.
• The Batzle-Wang bulk moduli are the adiabatic
moduli, which we believe are appropriate for wave
propagation.
• In contrast, standard PVT data are isothermal.
Isothermal moduli can be ~20% too low for oil, and
a factor of 2 too low for gas. For brine, the two don’t
differ much.
Nice paper by Virginia Clark, July ‘92 Geophysics.
KS
−1
= KT
−1
−
α2
T
ρCP
α = thermal expansion; Cp = heat capacity
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
106
Stress-Induced Velocity Anisotropy -- the Historical
Basis for Seismic Fracture Detection
Stress-induced velocity anisotropy in Barre Granite (Nur, 1969). In this
classic experiment, Nur manipulated the crack alignment by applying
uniaxial stress. Initially the rock is isotropic, indicating an isotropic
distribution of cracks. Cracks normal to the stress (or nearly so) closed,
creating crack alignment and the associated anisotropy.
Measurement angle related to the
uniaxial stress direction
F.20
P and S waves
θ
Axial Stress
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
107
Stress-Induced Velocity Anisotropy
Due to Crack Opening Near Failure
Uniaxial stress-induced velocity anisotropy in Westerly
Granite (Lockner, et al. 1977).
P
P
Source
Source
Source
S
S S
SII
II
Fracture
IIAS
0.6
0.7
0.8
0.9
1
1.1
1.2
0 2 0 4 0 6 0 8 0 100
P
S⊥
SII
SIIA
V/Vo
Percent Failure Strength
T
T
F.21
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
108
Seismic Anisotropy Due to
Rock Fabric
Isotropic mixture
slight alignment
layered
10
20
30
40
50
60
70
80
90
0 0.2 0.4 0.6 0.8 1
ρVp2
fabric anisotropy
vertical (c33)
horizontal (c11)
Virtually any rock that has a visual layering or fabric at a scale finer
than the seismic wavelength will be elastically and seismically
anisotropic. Sources can include elongated and aligned grains and
pores, cracks, and fine scale layering. Velocities are usually faster
for propagation along the layering.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
109
Velocity Anisotropy Due to Fabric
Anisotropic velocities vs. pressure. (a) and (b) Jones
(1983), (c) Tosaya (1982).
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
110
Velocity Anisotropy in Shale
Cotton Valley shale (ultrasonic), from Tosaya, 1982.
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
111
Velocity Anisotropy Resulting From
Thinly Layered Kerogen
P-wave anisotropy in shales (from Vernik, 1990):
(1) Bakken black shales, (2) Bakken dolomitic siltstone,
(3) Bakken shaly dolomite, (4) Chicopee shale (Lo, et al,
1985).
Vernik found that kerogen-bearing shales can have very
large anisotropy, easily 50%.
F.23
Stanford Rock Physics Laboratory - Gary Mavko
Parameters That Influence Seismic Velocity
112
Velocities in kerogen-rich Bakken shales (Vernik, 1990)
and other low porosity argillaceous rocks (Lo et al.,
1985; Tosaya, 1982; Vernik et al., 1987). Compiled by
Vernik, 1990.
F.24

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Rock Physics: Seismic Velocity

  • 1. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 73 Conceptual Overview of Rock and Fluid Factors that Impact Seismic Velocity and Impedance
  • 2. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 74 Typical rock velocities, from Bourbié, Coussy, and Zinszner, Acoustics of Porous Media, Gulf Publishing. Type of formation P wave velocity (m/s) S wave velocity (m/s) Density (g/cm3 ) Density of constituent crystal (g/cm3 ) Scree, vegetal soil 300-700 100-300 1.7-2.4 - Dry sands 400-1200 100-500 1.5-1.7 2.65 quartz Wet sands 1500-2000 400-600 1.9-2.1 2.65 quartz Saturated shales and clays 1100-2500 200-800 2.0-2.4 - Marls 2000-3000 750-1500 2.1-2.6 - Saturated shale and sand sections 1500-2200 500-750 2.1-2.4 - Porous and saturated sandstones 2000-3500 800-1800 2.1-2.4 2.65 quartz Limestones 3500-6000 2000-3300 2.4-2.7 2.71 calcite Chalk 2300-2600 1100-1300 1.8-3.1 2.71 calcite Salt 4500-5500 2500-3100 2.1-2.3 2.1 halite Anhydrite 4000-5500 2200-3100 2.9-3.0 - Dolomite 3500-6500 1900-3600 2.5-2.9 (Ca, Mg) CO32.8-2.9 Granite 4500-6000 2500-3300 2.5-2.7 - Basalt 5000-6000 2800-3400 2.7-3.1 - Gneiss 4400-5200 2700-3200 2.5-2.7 - Coal 2200-2700 1000-1400 1.3-1.8 - Water 1450-1500 - 1.0 - Ice 3400-3800 1700-1900 0.9 - Oil 1200-1250 - 0.6-0.9 -
  • 3. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 75 The Saturation and Pressure Dependence of P- and S-wave Velocities. F.1 3 4 5 6 7 0 100 200 300 Webatuck dolomite Velocity(km/s) Effective Pressure (bars) S a t . S a t . Dry Dry V P V S 1 2 3 4 5 6 0 100 200 300 Bedford Limestone Velocity(km/s) Effective Pressure (bars) S a t . Dry Dry S a t . VP VS Crack shape Number of cracks 2 3 4 5 6 0 100 200 Solenhofen limestone Velocity(km/s) Effective Pressure (bars) V S V PSat. and Dry Sat. and Dry 2 3 4 5 6 7 0 100 200 300 Westerly Granite Velocity(km/s) Effective Pressure (bars) Dry S a t . V P V S Dry S a t .Flat asymptoteWater-saturated Saturated Velocity(km/s) Velocity(km/s) Velocity(km/s) Velocity(km/s) Effective Pressure (bars) Effective Pressure (bars) Effective Pressure (bars) Effective Pressure (bars) Bedford Limestone Westerly Granite Solenhofen Limestone Webatuck Dolomite Peffective = Pconfining − Ppore
  • 4. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 76 Fundamental Observations of Rock Physics • Velocities almost always increase with effective pressure. For reservoir rocks they often tend toward a flat, high pressure asymptote. • To first order, only the difference between confining pressure and pore pressure matters, not the absolute levels of each -- ”effective pressure law.” • The pressure dependence results from the closing of cracks, flaws, and grain boundaries, which elastically stiffens the rock mineral frame. • The only way to know the pressure dependence of velocities for a particular rock is to measure it. • Make ultrasonic measurements on dry cores; fluid- related dispersion will mask pressure effects. • The amount of velocity change with pressure is a measure of the number of cracks; the pressure range needed to reach the high pressure asymptote is a measure of crack shape (e.g. aspect ratio). • Velocities tend to be sensitive to the pore fluid content. Usually the P-wave velocity is most sensitive and the S-wave velocity is less sensitive. • Saturation dependence tends to be larger for soft (low velocity) rocks.
  • 5. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 77 Pressure-Dependence of Velocities It is customary to determine the pressure dependence of velocities from core measurements. A convenient way to quantify the dependence is to normalize the velocities for each sample by the high pressure value as shown here. This causes the curves to cluster at the high pressure point. Then we fit an average trend through the cloud, as shown. The velocity change between any two effective pressures P1 and P2 can be conveniently written as: Vp and Vs often have a different pressure behavior, so determine separate functions for them. Remember to recalibrate this equation to your own cores! F29 Remember: Calibrate to Dry Cores! Vp Vp(40) =1.0 −0.40 *exp(−Peff /11) Vs Vs(40) =1.0 − 0.38* exp(−Peff /12) V(P2) V(P1) = 1.0 − 0.38exp(−P2 /12) 1.0 − 0.38exp(−P1/12)
  • 6. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 78 Replace Gas with Water Gas Water Difference Increase Pp by 100 bars 4D Example: Deep, Stiff, Gas Sand F32 Small impedance increase from fluids Modest impedance decrease from pressure Trajectories in the AVO plane Increasing Pp Increasing Sw Before After Difference
  • 7. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 79 Replace Gas with Water Gas Water Difference Increase Pp by 100 bars 4D Example: Deepwater, Soft, Gas Sand F32 Before After Difference Large impedance increase Small impedance decrease Trajectories in the AVO plane Increasing Pp Increasing Sw
  • 8. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 80 Effects of Pore Fluid on P-wave Velocity (Low Frequency) Calculations made from dry velocities, using Gassmann relation, Kmin = 36 GPa, Kwater = 2.2, Koil = 1. Density does not lead to ambiguity when Impedance is measured. lmp = ρV = ρ × modulus
  • 9. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 81 Beaver Sandstone 6% porosity Effects of Pore Fluid on P-wave Velocity (Low Frequency) Fontainebleau Sandstone 15% porosity F.4
  • 10. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 82 Velocities depend on fluid modulus and density • When going from a dry to water saturated rock, sometimes the P-velocity increases; sometimes it decreases. • The rock elastic bulk modulus almost always stiffens with a stiffer (less compressible) pore fluid. • The stiffening effect of fluid on rock modulus is largest for a soft (low velocity) rock. • The bulk density also increases when going from a dry to water-saturated rock. • Because velocity depends on the ratio of elastic modulus to density, the modulus and density effects “fight” each other; sometimes the velocity goes up; sometimes down. • Measures of modulus ( ), impedance ( ), and don’t have the density effect “ambiguity.” • Be careful of ultrasonic data! At high frequencies, the elastic-stiffening effect is exaggerated for both bulk and shear moduli; so we don’t often see the density effect in the lab and the velocities will be contaminated by fluid-related dispersion. M = ρV 2 lmp = ρV = ρ modulus VP /VS
  • 11. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 83 Beaver Sandstone 6% porosity Effect of Pore Pressure Effect of pore pressure on velocity, calculated assuming effective pressure law is valid, and assuming a fixed confining pressure of 40MPa (low frequency calculations using Gassmann relation). 4.4 4.6 4.8 5 5.2 5.4 0 5 1 0 1 5 2 0 2 5 3 0 3 5 4 0 Velocity(km/s) Pore Pressure (MPa) dry oil water F.6 Increasing pore pressure
  • 12. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 84 Ways that Pore Pressure Impacts Velocities • Increasing pore pressure softens the elastic mineral frame by opening cracks and flaws, tending to lower velocities. • Increasing pore pressure tends to make the pore fluid or gas less compressible, tending to increase velocities. • Changing pore pressure can change the saturation as gas goes in and out of solution. Velocities can be sensitive to saturation. • High pore pressure persisting over long periods of time can inhibit diagenesis and preserve porosity, tending to keep velocities low.
  • 13. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 85 Ultrasonic velocities and porosity in Fontainebleau sandstone (Han, 1986). Note the large change in velocity with a very small fractional change in porosity. This is another indicator that pressure opens and closes very thin cracks and flaws. Pressure Dependence of Velocities
  • 14. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 86 Dry shaly sandstone data from Han (1986). Each vertical “streak” plotted with the same symbol is a single rock at different pressures. Note the large change in modulus with little change in porosity -- another illustration that cracks and flaws have a large change on velocity, even though they contribute very little to porosity. Only the values at high pressure and with Han's empirical clay correction applied. F.8
  • 15. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 87 The Information in a Rock's Velocity-Pressure Curve 1. High pressure limiting velocity is a function of porosity 2. The amount of velocity change with pressure indicates the amount of soft, crack-like pore space 3. The range of the greatest pressure sensitivity indicates the shape or aspect ratios of the crack- like pore space
  • 16. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 88 Soft, Crack-Like Porosity 1. Includes micro and macrofractures and compliant grain boundaries. 2. Soft Porosity: • Decreases both P and S-wave velocities • Increases velocity dispersion and attenuation • Creates pressure dependence of V and Q • Creates stress-induced anisotropy of V and Q • Enhances sensitivity to fluid changes (sensitivity to hydrocarbon indicators) 3. High confining pressure (depth) and cementation, tend to decrease the soft porosity, and therefore decreases these effects. 4. High pore pressure tends to increase the soft porosity and therefore increases these effects.
  • 17. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 89 Curves on the left show the typical increase of velocity with effective pressure. For each sample the velocity change is associated with the opening and closing of cracks and flaws. These are typical when rapid changes in effective pressure occur, such as during production. Curves on the right show the same data projected on the velocity- porosity plane. Younger, high porosity sediments tend to fall on the lower right. Diagenesis and cementation tend to move samples to the upper left (lower porosity, higher velocity). One effect of over- pressure is to inhibit diagenesis, preserving porosity and slowing progress from lower right to upper left. This is called “loading” type overpressure. Rapid, late stage development of overpressure can open cracks and grain boundaries, resembling the curves on the left. This is sometimes called “transient” or “unloading” overpressure. In both cases, high pressure leads to lower velocities, but along different trends.
  • 18. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 90 Seismic Velocity and Overpressure A typical approach to overpressure analysis is to look for low velocity deviations from normal depth trends. Caution: when overpressure is “late stage,” estimates of pressure can be too low. F31
  • 19. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 91 Experiments that illustrate the effective pressure law. In the first part of the experiment, effective pressure is increased by increasing confining pressure from 0 to 80 MPa, while keeping pore pressure zero (solid dots). Then, effective pressure is decreased by keeping confining pressure fixed at 80 MPa, but pumping up the pore pressure from 0 to nearly 80 MPa (open circles). (Jones,1983.) The curves trace approximately (but not exactly) the same trend. There is some hysteresis, probably associated with frictional adjustment of crack faces and grain boundaries. For most purposes, the hysteresis is small compared to more serious difficulties measuring velocities, so we assume that the effective pressure law can be applied. This is a tremendous convenience, since most laboratory measurements are made with pore pressure equal 0. F.9 2.5 3 3.5 4 4.5 5 0 20 40 60 80 St. Peter sandstone Velocity(km/s) Effective Pressure (MPa) p c =80 MPa p c =80 MPa p p =0 p p =0 VP VS 2.6 2.8 3 3.2 3.4 3.6 0 20 40 60 80 Sierra White granite Velocity(km/s) Effective Pressure (MPa) p p =0 p c =80 MPa VS
  • 20. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 92 Pierre shale (ultrasonic), from Tosaya, 1982. F.11 For shales, we also often see an increase of velocity with effective pressure. The rapid increase of velocity at low pressures is somewhat elastic, analogous to the closing of cracks and grain boundaries that we expect in sandstones. The high pressure asymptotic behavior shows a continued increase in velocity rather than a flat limit. This is probably due to permanent plastic deformation of the shale. 0.5 1 1.5 2 2.5 3 3.5 4 0 5 0 100 150 200 Velocity(km/s) Confining Pressure (MPa) p p =1MPa p p =41 MPa pp =0 p p =0 pp =1MPa V P V S S a t . S a t . D r y D r y p p =41 MPa Velocity(km/s) Confining Pressure (MPa)
  • 21. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 93 transducer transducer Rock sample Jacket Confining pressure Pore pressure transducer transducer Concept of Induced Pore Pressure ∆σ = 1bar ∆Pp ~ 0.2bar ∆Pp ~ 1bar Stiff Pore Soft Pore We expect a small induced pressure in stiff pores
  • 22. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 94 Chalk (ultrasonic), from Gregory, 1976, replotted from Bourbié, Coussy, and Zinszner, 1987, Gulf Publishing Co. F.12 For chalks, we also see an increase of velocity with effective pressure. The rapid increase of velocity at low pressures is somewhat elastic and reversible. The high pressure asymptotic behavior shows a continued increase in velocity rather than a flat limit. This is probably due to permanent crushing of the fragile pore space. 1.5 2 2.5 3 3.5 0 1 0 2 0 3 0 4 0 5 0 Chalk Velocity(km/s) Effective Pressure (MPa) Sw 100 0 5 10 20 40 80 60 V P V S 5 φ = 30.6% Velocity(km/s)
  • 23. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 95 Influence of temperature on oil saturated samples, from Tosaya, et al. (1985). F.16 We observe experimentally that velocities are most sensitive to temperature when the rocks contain liquid hydrocarbons (oil). We believe that this results from an increase of the oil compressibility and a decrease of the oil viscosity as the temperature goes up. In field situations other factors can occur. For example, gas might come out of solution as the temperature goes up.
  • 24. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 96 An Early, Successful 4D Field Study Thermal Signature of Steam Flood From DeBuyl, 1989 Traveltime increase in steamed interval after a few months of steam injection. After a few more months, the anomaly spreads. F30
  • 25. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 97 Velocity vs. viscosity in glycerol saturated samples, from Nur (1980). F.17 Temperature Temperature In this experiment the pore fluid is glycerol, whose viscosity is extremely sensitive to temperature. The data show a classical viscoelastic behavior with lower velocity at low viscosity and higher velocity at higher viscosity. Viscosity is one of several pore fluid properties that are sensitive to temperature. 0.5 0.6 0.7 0.8 0.9 1 1.1 -4 -2 0 2 4 6 8 10 Barre granite µ/µο Log viscosity (poise) Bedford limestone 0.7 0.8 0.9 1 -4 -2 0 2 4 6 8 10 Bedford limestone Vp Vs V/Vo
  • 26. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 98 Compressional velocities in the n-Alkanes vs. temperature. A drastic decrease of velocity with temperature! The numbers in the figure represent carbon numbers. From Wang, 1988, Ph.D. dissertation, Stanford University. F.18
  • 27. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 99 Compressional velocities in the n-Alkanes vs. inverse of the carbon numbers, at different temperatures. From Wang, 1988, Ph.D. dissertation, Stanford University. F.19
  • 28. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 100 Batzle-Wang formulas for fluid density and bulk modulus (Geophysics, Nov. 1992). F30
  • 29. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 101 F30 API =141.5 ρO −131.5 1 l/l = 5.615 ft 3 /bbl
  • 30. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 102 F30 BrineBulkModulus(Gpa)BrineDensity(kg/m3)
  • 31. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 103 BubblePoint computed using Batzle, Wang Relations Caution: Calibrate to lab data when possible! F30
  • 32. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 104 Soft Deepwater Sands
  • 33. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 105 Fluid Properties • The density and bulk modulus of most reservoir fluids increase as pore pressure increases. • The density and bulk modulus of most reservoir fluids decrease as temperature increases. • The Batzle-Wang formulas describe the empirical dependence of gas, oil, and brine properties on temperature, pressure, and composition. • The Batzle-Wang bulk moduli are the adiabatic moduli, which we believe are appropriate for wave propagation. • In contrast, standard PVT data are isothermal. Isothermal moduli can be ~20% too low for oil, and a factor of 2 too low for gas. For brine, the two don’t differ much. Nice paper by Virginia Clark, July ‘92 Geophysics. KS −1 = KT −1 − α2 T ρCP α = thermal expansion; Cp = heat capacity
  • 34. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 106 Stress-Induced Velocity Anisotropy -- the Historical Basis for Seismic Fracture Detection Stress-induced velocity anisotropy in Barre Granite (Nur, 1969). In this classic experiment, Nur manipulated the crack alignment by applying uniaxial stress. Initially the rock is isotropic, indicating an isotropic distribution of cracks. Cracks normal to the stress (or nearly so) closed, creating crack alignment and the associated anisotropy. Measurement angle related to the uniaxial stress direction F.20 P and S waves θ Axial Stress
  • 35. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 107 Stress-Induced Velocity Anisotropy Due to Crack Opening Near Failure Uniaxial stress-induced velocity anisotropy in Westerly Granite (Lockner, et al. 1977). P P Source Source Source S S S SII II Fracture IIAS 0.6 0.7 0.8 0.9 1 1.1 1.2 0 2 0 4 0 6 0 8 0 100 P S⊥ SII SIIA V/Vo Percent Failure Strength T T F.21
  • 36. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 108 Seismic Anisotropy Due to Rock Fabric Isotropic mixture slight alignment layered 10 20 30 40 50 60 70 80 90 0 0.2 0.4 0.6 0.8 1 ρVp2 fabric anisotropy vertical (c33) horizontal (c11) Virtually any rock that has a visual layering or fabric at a scale finer than the seismic wavelength will be elastically and seismically anisotropic. Sources can include elongated and aligned grains and pores, cracks, and fine scale layering. Velocities are usually faster for propagation along the layering.
  • 37. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 109 Velocity Anisotropy Due to Fabric Anisotropic velocities vs. pressure. (a) and (b) Jones (1983), (c) Tosaya (1982).
  • 38. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 110 Velocity Anisotropy in Shale Cotton Valley shale (ultrasonic), from Tosaya, 1982.
  • 39. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 111 Velocity Anisotropy Resulting From Thinly Layered Kerogen P-wave anisotropy in shales (from Vernik, 1990): (1) Bakken black shales, (2) Bakken dolomitic siltstone, (3) Bakken shaly dolomite, (4) Chicopee shale (Lo, et al, 1985). Vernik found that kerogen-bearing shales can have very large anisotropy, easily 50%. F.23
  • 40. Stanford Rock Physics Laboratory - Gary Mavko Parameters That Influence Seismic Velocity 112 Velocities in kerogen-rich Bakken shales (Vernik, 1990) and other low porosity argillaceous rocks (Lo et al., 1985; Tosaya, 1982; Vernik et al., 1987). Compiled by Vernik, 1990. F.24