Conclusions We perform extensive numerical simulations of 3D rupture propagation governed by the...
-
Upload
celine-hazard -
Category
Documents
-
view
217 -
download
0
Transcript of Conclusions We perform extensive numerical simulations of 3D rupture propagation governed by the...
Conclusions We perform extensive numerical simulations of 3D rupture propagation governed by the linear slip-weakening in order to define the optimal parameters that ensure spontaneous rupture propagation.
We consider square, elliptical and circular shapes of the initiation zone and find that the area of the initiation zone, for a given value of S, determines whether the rupture will spontaneously propagate or not regardless the particular shape of initiation zone. The transition between propagating and non-propagating ruptures is inconsistent with published theoretical estimates of the critical half-length in 2D and 3D cases.
We find that results obtained by FEM and ADER-DG methods converge. This indicates that the results of this study are method independent.
Additionally, we observe that adjusted over-shoot value is a good way to minimize the size of initiation zone without introducing numerical artifacts. This might be useful in simulations with heterogeneous faults.
For numerical simulations we used parameters in the table (right).
To obtain different values of the strength parameter, S, we used different values of initial traction and fixed values of static and dynamic coefficients of friction.
Abstract
Numerical simulations of earthquake ruptures require artificial procedures to initiate spontaneous dynamic propagation under linear slip-weakening friction. A frequently applied technique uses a stress asperity for which effects of the forced initiation depend on size and geometry of the asperity, the spatial distribution of stress in and around the asperity, and the maximum stress-overshoot value. To properly study the physics of earthquake rupture processes, it is mandatory to understand, and then minimize, the effects of the artificial initiation on the subsequent spontaneous rupture propagation. The model space of possible parameterizations for rupture initiation is large, but a detailed parametric study of their effects on the resulting dynamic crack propagation has not yet been conducted. We therefore extend our
previous work to define the optimal initiation parameterization that ensures spontaneous rupture propagation. We consider different sizes and shapes of the initiation region as well as different stress-overshoot values and different spatial sampling to investigate the conditions for spontaneous rupture propagation. This study does not examine in detail the stress distribution within the initiation patch as the required additional parameters greatly expand the model space; this is left for future work.
We perform extensive numerical simulations of 3D rupture propagation governed by linear slip-weakening friction. We find that the boundary delimiting regions of the spontaneous rupture propagation and premature rupture arrest appears to be determined by the area of the initiation patch and over-shoot value. Our results indicate that using over-shoot values appropriately scaled to the size of the initiation zone generate correct results without
numerical artifacts.
Additionally, we compare our numerical results with 2D and 3D analytical estimates (Andrews, 1976 a,b; Day, 1982; Campillo & Ionescu, 1997; Favreau et al., 1999; Uenishi & Rice, 2003, 2004), and find that in 3D numerical simulations the transition between propagating and non-propagating ruptures is incompatible with theoretical estimates of the critical half-lengths. We conjecture that these discrepancies are due to 3D effects and less idealized boundary/initial conditions in the numerical simulations.
Our study thus guides the appropriate choice of the rupture initiation zone, to reduce unsuccessful but costly dynamic rupture simulations, and to minimize the effects of forced initiation on the subsequent spontaneous rupture propagation.
Initiating spontaneous rupture propagation in dynamic models with linear slip-weakening friction
– a parametric study
REFERENCES
Andrews 1976a JGR Andrews 1976b JGRCampillo & Ionescu 1997 JGRDay 1982 BSSADay et al. 2005 JGRDunham 2007 JGRFavreau et al. 1999 BSSAGalis et al. 2010 GJI Pelties et al. 2012 JGRUenishi & Rice 2003 JGRUenishi & Rice 2004 EOS (AGU FM)
ACKONWLEDGEMENTS
We gratefully acknowledge the funding by the European Union through the Initial Training Network QUEST (grant agreement 238007), a Marie Curie Action within the ‘People’ Programme. C. Pelties is funded by VolkswagenStiftung (ASCETE project). ADER-DG results have been computed on the BlueGene/P Shaheen of the King Abdullah University of Science and Technology, Saudi Arabia.
cy a b x
Comparison of theoretical estimates with numerical results
IIAL
IIIAL
IIICL
IICL
2IIIUR DL2
IIUR DL
DL
3IIIUR DL3
IIUR DL
Theoretical estimates ofthe half-length size
Theoretical estimates ofthe area calculated from
the half-length size
AL
CL
2UR DL
DL
3UR DL
line color line style
square
circle
ellipse
Numerical results
ellipse
circle
square
Martin GALIS 1, Christian PELTIES 2, Jozef KRISTEK 3,4 , Peter MOCZO 3,4 and P. Martin MAI 1 1) KAUST – King Abdullah University of Science and Technology, Thuwal, Saudi Arabia
2) Ludwig-Maximilians-University Munich, Munich, Germany3) Comenius University Bratislava, Slovakia
4) Slovak Academy of Sciences, Bratislava, Slovakia
ECGS Workshop 2012 - Earthquake source physics on various scalesLuxembourg, October 3-5, 2012
1. SHAPE of the initiation zone
Material parameters
VP VS density QP, QS
6 000 m/s 3 464 m/s 2 670 kg/m3 Infinity
Friction law parameters ( fault dimensions 30km x 15km )
static coeff. of friction
dynamic coeff.of friction
normal component of initial traction
characteristic distance
0.67777778 0.525 120 MPa 0.4 m
We present results using these non-dimensional quantities:
strength parameternon-dimensional length/area
of initiation zone
(as used by Dunham, 2007)
Model parameters
2. SIZE of the initiation zone
3. OVERSHOOT in the initiation zone
Here we search for the minimal size of the initiation zone that generates spontaneous rupture propagation. We consider different shapes of initialization zone - square, circle and ellipse. For simulations we use finite-element method (FEM) with two element sizes – h =100m and h = 50m.Each gray point represents one simulation. The
black point represents simulation with the largest considered initiation zone for which rupture did not propagated spontaneously over the whole fault plane, the green point represents simulation with the smallest considered initiation zone for which we observed spontaneous rupture propagation. The red lines mark the transition
between propagating and non-propagating ruptures. To parameterize this boundary we use power functions
and
Square Circle Ellipse
h =
100 m
h =
50 m
h =
100 m
h =
50 m
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
3.0
2.5
2.0
1.5
1.0
0.5
0.0
0 0.5 1 1.5 20.25 0.75 1.25 1.75
non-d
imensi
onal h
alf
-len
gth
of
init
iati
on z
one
non-d
imensi
onal h
alf
-len
gth
of
init
iati
on z
one
strength parameter strength parameter strength parameter strength parameter
ellipsecirclesquare
ellipsecirclesquare
ellipsecirclesquare
ellipsecirclesquare
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
non-d
imensi
onal are
aof
init
iati
on z
one
non-d
imensi
onal are
aof
init
iati
on z
one
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
0 0.5 1 1.5 20.25 0.75 1.25 1.75
20
18
16
14
12
10
2
8
4
6
strength parameter
FEM h = 100m
FEM h = 50m
ADER-DG h=200m, O4
To check if the results are method dependent we consider only square shaped initiation zone and we use two different numerical methods: FEM (a finite element method, Galis et al., 2010) and ADER-DG (an arbitrarily high order – discontinuous Galerkin method, Pelties et al., 2012). For each method we consider also different spatial discretizations.
FEM ADER-DG
mesh uniform hexahedral unstructured tetrahedral
smallest change of initiation zone size
h/2 (h = element size)
50m (fixed for all discretizations)
discreti-zations
h=200, 150, 100, 75, 50, 37.5, 25mfor S=2.0 also 18.75m
h=200m: O: 2, 3, 4, 5, 6h=300m: O: 3, 4, 5
degrees of freedom(dof)
8(N+1)(N+2)(N+3)/6 N is polynomial degree (N = O + 1)
rupture dynamics
TSN (traction-at-split-node method)
inverse Riemann problemstrength parameter
10 100
19
18
17
16
15
14
9
13
11
12
10
10 100
10
9
8
7
6
5
0
4
2
3
1
non-d
imensi
onal are
aof
init
iati
on z
one
S = 0.1 S = 2.0
FEMADER-DG
Inside the stress asperity the stress is chosen larger than the yield stress. The stress overshoot is the difference between the prescribed stress and the yield stress.
In this part of the study we search for the minimal overshoot that ensures spontaneous rupture propagation for prescribed initiation zone. We also compare the effects of larger overshoot on the rupture propagation.
We express overshoot as percentage of dynamic stress drop, because if overshoot is expressed as a percentage of yield stress, proper scaling of over-shoot with stress-drop and strength excess is not guaranteed. For example, configurations with equal stress drops and strength excesses should provide the same results. But if overshoot depends on yield stress that will not always be true. 25
overs
hoot
[%
of
dynam
ic s
tress
dro
p]
20
15
10
5
00 0.2 0.4 0.6 0.8 1
S = 0.1
250
200
150
100
50
overs
hoot
[%
of
dynam
ic s
tress
dro
p]
0 0.2 0.4 0.6 0.8 10
S = 2.0
different over-shoot values with fixed initiation zone size
adjusted over-shoot values to the size of initiation zone
(green points from the left-most figure)
S = 0.1
receiver in the middle of initiation zone
in-plane receiver (15Lfric from hypocenter)
receiver in the middle of initiation zone
in-plane receiver (15Lfric from hypocenter)
non-d
imensi
onal h
alf
-len
gth
of
init
iati
on z
one
strength parameter
non-d
imensi
onal are
aof
init
iati
on z
one
strength parameter
email: [email protected]: ces.kaust.edu.sa www.nuquake.eu
Note: time 0 s means slip-rate reached value 1 m/s. Note: time 0 s means slip-rate reached value 0.5 m/s.
0.00270.00450.45454.5455
11.363627.727345.4545
over-shoot
0.00270.00450.45454.5455
11.363627.727345.4545
over-shoot
0.00270.03330.33333.3333
13.333320.000033.3333
over-shoot
0.00270.03330.33333.3333
13.333320.000033.3333
over-shoot
12.95 0.19
8.860.25
6.360.32
4.090.39
2.550.47
1.560.56
0.910.66
0.360.77
0.090.88
0.051.00
over-shoot
12.95 0.19
8.860.25
6.360.32
4.090.39
2.550.47
1.560.56
0.910.66
0.360.77
0.090.88
0.051.00
over-shoot
over-shoot
250.000.22
196.670.25
163.330.29
136.670.32
116.670.36
81.000.46
63.330.51
50.000.56
43.330.62
33.330.67
23.330.73
16.670.80
13.330.86
3.330.93
0.331.00
over-shoot
250.000.22
196.670.25
163.330.29
136.670.32
116.670.36
81.000.46
63.330.51
50.000.56
43.330.62
33.330.67
23.330.73
16.670.80
13.330.86
3.330.93
0.331.00
different over-shoot values with fixed initiation zone size
adjusted over-shoot values to the size of initiation zone
(green points from the left-most figure)
S = 2.0
non-d
imensi
onal are
aof
init
iati
on z
one
20
18
16
14
12
10
2
8
4
6
20
18
16
14
12
10
2
8
4
6
non-d
imensi
onal are
aof
init
iati
on z
one
non-d
imensi
onal are
aof
init
iati
on z
one
FEM + ADER-DG
non-d
imensi
onal are
aof
init
iati
on z
one
To explain observed differences between FEM and ADER-DG we perform a detailed study of the dependency of the minimal initiation zone size on the spatial discretization. We focus only on two limit cases – S = 0.1 (where differences between methods are smaller) and S = 2.0 (where differences between methods are larger). To compare FEM and ADER-DG results we used quantity h/∛dof. This quantity was then scaled using the non-dimensional estimate of breakdown zone width at the time of rupture initiation (Day et al., 2005).
The different behavior of FEM and ADER-DG with respect to the size of initiation zone and resolution is consequence of the differences between the methods. Probably the most important is the implementation of dynamic rupture - TSN method is used in FEM while inverse Riemann problem is used in ADER-DG. Some other differences between methods are summarized in the table below.
non-d
imensi
onal are
aof
init
iati
on z
one
10 100
10
9
8
7
6
5
0
4
2
3
1
10 100
non-d
imensi
onal are
aof
init
iati
on z
one
10 100
19
18
17
16
15
14
9
13
11
12
10
10 100
Note: Gray squares indicate possible initiation zone sizes for each
resolution.
Note: Gray squares indicate possible initiation zone sizes for each
resolution.
FEM ADER-DG FEM ADER-DG
FEM + ADER-DG FEM + ADER-DG