application of earthquake simulations to seismicity …...application of earthquake simulations to...
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Application of earthquake simulations to seismicity induced by fluid injection
James H. Dieterich, Keith B. Richards-Dinger, and Kayla A. Kroll*University of California, Riverside
*Now at Lawrence Livermore National Laboratory
• Based on rate and state dependent friction
• Simulations avoid repeated solutions of a large system simultaneous
equations fast computation
• Event driven computations based on changes of fault sliding state. A fault
element may be at one of three sliding states
0 – Aging by log time of stationary contact
1 – Nucleating slip: Time- dependent accelerating slip to instability
Analytic solutions with rate-state friction
2 – Earthquake slip: quasi-dynamic – to a first approximatio. Slip speed set by
by shear impedance.
Earthquake simulator – RSQSim
t
s= m = m0 + aln
d
d*
æ
èç
ö
ø÷+ bln
qd*
Dc
æ
èç
ö
ø÷ dq = dt -
q
Dc
dd -aq
Bsds
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)All-California simulationAftershocks follow the Omori Lawfor aftershock decay with time
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)
• High resolution models of geometrically complex fault systems
➞Up to 106 fault elements
➞Range of earthquake magnitudes M=3.5 to M=8
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)
• High resolution models of geometrically complex fault systems
➞Up to 106 fault elements
➞Range of earthquake magnitudes M=xx to M=yy
Oak Ridge F.
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)
• High resolution models of geometrically complex fault systems
➞Up to 106 fault elements
➞Range of earthquake magnitudes M=xx to M=yy
• Long simulations of >106 earthquakes
➞Statistical characterizations are consistent with observations
➞Repeated simulations to explore parameter space
RSQSim
(Rate-State Quake Simulator)
• Comprehensive simulation of fault slip phenomena:
➞earthquakes, continuous creep, slow slip events, afterslip
• Implement rate- and state-dependent friction effects
➞Earthquake clustering effects (aftershocks and foreshocks)
• High resolution models of geometrically complex fault systems
➞Up to 106 fault elements
➞Range of earthquake magnitudes M=xx to M=yy
• Long simulations of >106 earthquakes
➞Good statistical characterizations
➞Repeated simulations to explore parameter space
Wells and Coppersmith (1994)
WGCEP 02 Appendix D
Hanks and Bakun (2007)
Rupture area km2
102 103
Magnitude
6.0
6
.5
7.0
7
.5
8
.0
Wells and Coppersmith
RSQSim
Simulation (random 200-yr period)
Tectonic stressing with fluid injection
Fault 1
Fault 2
Fault 1 Fault 2
Earth Surface
M=7.0 Multi-fault earthquake rupture simulation
Red shows areas that are actively slipping in the earthquake
Earthquake rate modelBased on rate-state nucleation solutions
Approach
The formulation is based on the premise that earthquake nucleation controls
the time and place of initiation of earthquakes. Hence, processes that alter
earthquake nucleation times control changes of seismicity rates. Assumes a
steady-state seismicity rate that is proportional to stressing rate.
Implemented with a simple planar fault models with 400-1600 fault elements
R =r
g ˙ t rdg =
1
Asdt - g dt +
t
s- a
æ è
ö ø ds
é
ë ê ù
û ú Earthquake rate ,
Coulomb stress
Earthquake rate ,
dS = dt - mds
R =r
g ˙ S rdg =
1
Asdt - g dS[ ]
(Dieterich, 1994), Dieterich and others, Nature, (2000), Dieterich and others, USGS Prof - 1676 (2003)
“Reservoir” Model
We use a simple analytic expression (Wang, 2000) for the diffusion of pore-fluid pressure, P, into a homogeneous full- or half-space from a point source, and only the effects of Pon the effective normal stress (vs. more complete poroelastic effects).
porosity compressibility
Zero Tectonic Stressing Rate Models
• If the initial shear stress τ0 is greater than τmax:
then events will nucleate even in the absence of pore-fluid pressure perturbations.
• If the initial shear stress τ0 is less than τmin:
where P is the maximum pore-fluid pressure perturbation, then no events will ever nucleate.
The semi-infinite reservoir model used in this initial study results in a long-term steady-state maximum fluid pressure that is inversely proportional to the distance from the point of injection. The maximum fluid pressure sets the minimum and maximum initial shear stress that will result in induced earthquakes
CM2
Pressure andEarthquake rate profiles
Simple fault model with 1600 fault elements (100m x 100m)
s0.5,
Change of fluid pressures along profile closest to injection point
Change of fluid pressures along profile closest to injection pointEarthquake rates (black)
Initial stress is 0.5 Mpa below that forstress for steady state seismicity
Diffusivity=0.01, Porosity=0.07, Initial Stress=-0.1MPa
Earthquake rate model
Example of simulation of induced seismicity using RSQSim
Space-time plot of earthquake ruptures and fluid pressures (along upper edge of fault)
Model: Single fault with initial shear stress ~5MPa below critical stress (for failure without injection), no tectonic stressing, injection rate = 0.01M3/s, injection point is 200m out of the plane of the fault
Startinjection
Endinjection
The average initial stress t on the fault surface strongly affects the characteristics of induced seismicity.
With increasing t in the range tmin to tmax :
• The delay between the start of injection and onset of seismicity decreases,
• the magnitude of the first induced event increases,
• the magnitude of the largest event in the sequence increases,
• the cumulative number of induced earthquakes increases,
• the distance from the injection point to the most distance earthquake increases, and
• the seismicity following shut-in increases and persists for longer times.
Initial shear stress and fluid pressures to induce earthquakes
0
2e13
4e13
Cu
mu
lati
ve
m
om
ent
Mag
nit
ud
e
0
20
-5 0 5 10 15 20 25
40
60
Cu
mu
lati
ve
nu
mber
o
f ev
ents
Time (years)
50 1 2 3 4
5
10
15
Easting (km)
TIm
e (y
ears
)
2
4
6
8 1
0
12
14 1
6
18
2
0
22
24
6
2 82 03 23
43
63
83
40
24
44
64 84
05
25
45
65
Initial Tau = 36 MPa
1.0
2.0
3.0
4.0
0
2e14
4e14
6e14
0
50
100
150
200
250
-5 0 5 10 15 20 25Time (years)
Initial Tau = 48 MPa
0 1 2 3 4 5
0
5
10
15
20
Easting (km)
Tim
e (y
ears
)
2
4
6 8
10
12 14
16
18
20
22
24 26
28
30 32
34 6
3 8
3 40
42 44
46
48 05
52 54
56 58
Cum
ula
tive
Num
ber
Cu
mu
lati
ve
Mo
men
tM
agnit
ud
e
1.0
2.0
3.0
4.0Initial Tau = 56 MPa
0 1 2 3 4 5
0
5
10
15
20
25
30
Easting (km)
Tim
e (y
ears
)C
um
ula
tiv
e
Mo
men
t
Cu
mu
lati
ve
Nu
mb
erM
agn
itu
de
2
4
6 8
10
12
14
16 18 20
22
24
26 28
30 32
34
36
38 40
42
44
46
48
05
52
54
6
5
0
2e15
4e15
6e15
8e15
0100
300
500
700
1
2
3
4
0 10 20 30 40
Time (years)
τ0 = 48 MPaτ0
= 36 MPa
τ0 = 56 MPa • At lower τ0: events confined to
area near injection point
• At higher τ0: – events can rupture into areas of
lower pore-fluid pressure
– Post shut-in seismicity is enriched and continues for a longer time
Effect of Initial Shear Stress
Effect of Initial Shear Stress
Effect of injection pulses
The volume of the crust that contains an earthquake rupture scales by 10M1.5
Dieterich, Richards-Dinger, Kroll (2015, SRL)
For isolated fracture permeabilty: M ~1.0log10(V)
The maximum possible earthquake magnitude is set by the fault dimensions. However, for faults with sub-critical initial stresses, , induced earthquake ruptures affect only a sufficiently pressured portion of the fault, and the maximum magnitude of the induced events increases with injected volume, in general agreement with observations.
Figure. The volume of injected fluid needed to pressurize (by some fixed amount) the volume of crust that embeds an induced earthquake rupture, scales by 101.5M , which has a slope of 2/3 on this plot (dashed line). Results from simulations are indicated by data points in color (see legend). All models have a normal stress of 100MPa. Additional parameters that affect maximum magnitude include reservoir storage capacity, and normal stress s which controls earthquake stress drop.
t 0 < tmax
Maximum magnitude and injected volume
Dieterich, Richards-Dinger, Kroll (2015, SRL)
Effect of as on decay following shut-in
R =r
g ˙ S rdg =
1
asdt -gdS[ ]
Effect of diffusivity k on decay followingShut-in
Many factors affect the rate of earthquake decay following shut-in
Diffusivity and as
Duration of seismicity following shut-in
Continuing earthquakes following shut-in
Two effects may cause delayed earthquakes following shut-in:
1) Continuing increase of pressure until the shut-in pulse reaches progressively distant points from the injection well.
2) Delayed nucleation in the form of aftershocks to earlier induced events and the stress perturbation from injection.
Prevention by shut-in: Test of traffic light procedures
We first ran this simulation with injection for 20 years to establish base-line induced seismicity
Then we re-ran the simulation with different shut-in times to determine the latest shut-in times that prevented events A, B and C.
Maximum magnitude following shut-in Extent of rupture
Effect of shut-in times on maximum magnitude
1.0
2.0
3.0
4.0
Mag
nit
ude
Event A:
M3.8; 2.92 yrs
Event A:
M3.8; 2.92 yrs
Event B:
M3.2; 9.4 yrs
Event C:
M4.1; 15.5 yrs
1050 15 20 25 30
Time (years)
1.0
2.0
3.0
4.0
Mag
nit
ud
e
1050 15 20 25 30
Time (years)
Shut-In at
2.82 years;
36.5 days
before Event A
Shut-In at
2.82 years
●
●
● ● ●●
● ● ●
●
● ● ●●
● ● ●
●
● ● ●●
● ●
2.80 2.85 2.90 2.95
1.5
2.5
3.5
Shut●In Tim e (years)
Mag
nit
ud
e
●
●
● ● ●●
● ●
Shut-in following the first M>3.1 event would have prevented subsequent M>3earthquakes,
Rake Angles From Region Stressing Rate Field
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Tectonic stressing with fluid injection
Easting (km)●2 ●1 0 1 2
●6.0
●5.5
●5.0
●4.5
●4.0
●3.5
●3.0
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6085
6090
6095
6100
Tim
e (y
ears
)Easting (km)
●2 ●1 0 1 2●6.0
●5.5
●5.0
●4.5
●4.0
●3.5
●3.0
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6085
6090
6095
6100
Tim
e (y
ears
)
Without injection
With injection
Tectonic stressing with fluid injection
Fault zone consists of 6 anastomosing faults with fractal roughness
Induced seismicity from injection into a fault zone
Induced seismicity from injection into a fault zoneAverage initial shear stress 54MPa
Kayla Kroll PhD thesis)
Injection point
Conclusions
1) Modeling• We have computational tools for quantitative virtual experiments• This includes models with highly complex fault systems – needed
for case studies
2) Rate-state friction – Earthquake clustering can result in continuing seismicity long after Pfluid effects have dissipated.
3) Initial stresses strongly affect characteristics of induced seismicity
4) With qualifications, maximum earthquake magnitude should scale by injected volume. Slope depends on bulk vs (fault) fracture diffusion
5) Traffic light procedures – real-time hazard assessment and risk mitigation may be problematic because of the increasing time lag for pressure signals to more distant points.