1 – stress contributions 2 – probabilistic approach 3 – deformation transients small...
TRANSCRIPT
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1 – Stress contributions1 – Stress contributions
2 – Probabilistic approach2 – Probabilistic approach
3 – Deformation transients3 – Deformation transients
Small earthquakes contribute as much as large earthquakes do to stress changes
Extract the « influence » of small earthquakes directly from seismicity data
Evaluate how anomalous a given seismicity pattern can be
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Meier et al (JGR 2014)
1 – Stress contributions1 – Stress contributions
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Estimation of the contribution in static stress transfer from small (unresolved) sources
with -1 ≤ ≤ 1, C constant
r = hypocentral distances btw earthquakes
Mo = seismic moment
r
Source MSource Moo
ReceiverReceiver
3L+rCM=τ o
1 – Stress contributions1 – Stress contributions
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Holtsmark (1919), Chandrasekhar (1943)
Gravitational field at any given location, caused by a distribution of stars (with random masses)
V
g(r1,M
1)
RrπR
πr=rfr
3
2
3/4
4
R
} f g (g )=K g−5 /2
For one star :
1 – Stress contributions1 – Stress contributions
2)( GMrrgx
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X 1≡X 2≡X 3 ...
X= X 1+ X 2+ X 3+ ...+ X N≡ c X 1
c=N 1 /2For normal (Gaussian) distributions :
There exist other stable distributions, known as Lévy distributions, for which
They have power-law decays in
c=N 1 / α
f X (x ) = K x−1−α
Stability of random distributions for addition
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Holtsmark (1919), Chandrasekhar (1943)
Gravitational field at any given location, caused by a distribution of stars (with random masses)
V
g(r1,M
1)
R
For all stars :
V = g1 + g
2 + ... f V (V )=K ' V −5 /2
Stable for additionStable for addition
1 – Stress contributions1 – Stress contributions
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Holtsmark (1919), Chandrasekhar (1943)
Gravitational field at any given location, caused by a distribution of stars (with random masses)
V
g(r1,M
1)
R
}For all stars :
1 – Stress contributions1 – Stress contributions
2)( GMrrgx
RrπR
πr=rfr
3
2
3/4
4 f V (V )=K ' V −5 /2
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r = hypocentral distances btw earthquakes
Mo = seismic moment
r
Source MSource Moo
ReceiverReceiver
1 – Stress contributions1 – Stress contributions
Estimation of the contribution in static stress transfer from small (unresolved) sources
with -1 ≤ ≤ 1, C constant 3L+rCM=τ o
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r = hypocentral distances btw earthquakes
Mo = seismic moment
r
Source MSource Moo
ReceiverReceiver
3L+rCM=τ o
1Dr Kr=rf
} 3/1 Doτ τMK=τf
Stable for additionStable for addition
For one source:
Kagan (Nonl. Proc. Geophys., 1994)
1 – Stress contributions1 – Stress contributions
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r = hypocentral distances btw earthquakes
Mo = seismic moment
r
Source MSource Moo
ReceiverReceiver
} 3/1/3 Do
Dmτ, τMmNK=τf
Stable for additionStable for addition
For all N(m) sources of magnitude m:1 – Stress contributions1 – Stress contributions
3L+rCM=τ o
1Dr Kr=rf
N
Marsan (GJI 2004)
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}Stable for additionStable for addition
For all N(m) sources of magnitude m:
Gutenberg-Richter : N (m )=N 010−b m
Kanamori : M o=10
1.5m+ 9
NB : far field approximation
1 – Stress contributions1 – Stress contributions
3/1/3 Do
Dmτ, τMmNK=τf
3L+rCM=τ o
1Dr Kr=rf
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Compute stress on a regular grid
Largest earthquakes
dominate
3/1/3 Do
Dmτ, τMmNK=τf
D=3
10(1.5−b)m
1 – Stress contributions1 – Stress contributions
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1 – Stress contributions1 – Stress contributions
M
7
6
5
4
3
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M
7
6
5
4
3
1 – Stress contributions1 – Stress contributions
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M
7
6
5
4
3
1 – Stress contributions1 – Stress contributions
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M
7
6
5
4
3
1 – Stress contributions1 – Stress contributions
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1 – Stress contributions1 – Stress contributions
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Compute stress on hypocenters
All earthquakes contribute
101.5 (1−b )m
D=2
1 – Stress contributions1 – Stress contributions
3/1/3 Do
Dmτ, τMmNK=τf
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Meier et al (JGR 2014)
FM from Yang et al. (BSSA 2012)
Hypocenters from Hauksson et al. (BSSA 2012)
1 – Stress contributions1 – Stress contributions
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Meier et al (JGR 2014)
1 – Stress contributions1 – Stress contributions
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Stress change at the hypocenters of future earthquakes :
ALL magnitude bands contribute equally
Uncertainty on stress change grows as cut-off magnitude decreases
1 – Stress contributions1 – Stress contributions
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pi , j
probability that #i triggered #j
j<k
jk,
ji,ji, λ+λ
λ==p
0
Contribution from #i
Sum of all contributions
pi , j
i
j
Probabilistic approachProbabilistic approach
2 – Probabilistic approach2 – Probabilistic approach
1... ,1,2,1,0 jjjjj pppp
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lk,j,i λ=t,xλContribution from #i
Distance from #i to x
Time t-ti
Magnitude mi
Marsan and Lengliné (2008)
Inversion from data by Expectation – Maximization
2 – Probabilistic approach2 – Probabilistic approach
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Shearer et al. (2005) catalogue
N>70,000 earthquakes m ≥ 2
No decoupling between space and time
Correction for lack of detection following large shocks
Distances from fault to target hypocenter
target
mai
n fa
ult r
2 – Probabilistic approach2 – Probabilistic approach
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7M
76 <M
65 <M
54 <M
43 <M
32 <M
Mainshock magnitude
2 – Probabilistic approach2 – Probabilistic approach
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2 – Probabilistic approach2 – Probabilistic approach
B
C
A
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A
B
C
A B COROROROR
????????????
C is an indirect aftershock of A
2 – Probabilistic approach2 – Probabilistic approach
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0 – 5 km0 – 5 km
5 – 20 km5 – 20 km
> 20 km> 20 km
Probability of being a direct aftershock of a M>7 earthquake
1%1%
1 w
ee
k1
we
ek
3 m
on
ths
3 m
on
ths
60%60%
2 – Probabilistic approach2 – Probabilistic approach
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Probability of being a direct aftershock of a 3<M<4 earthquake
0 – 1 km0 – 1 km
1 – 5 km1 – 5 km
5 – 20 km5 – 20 km
2 – Probabilistic approach2 – Probabilistic approach
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Marsan and Lengliné (JGR 2010)
Our method: Direct ASDirect AS
Modified from Felzer & Brodsky (2006):
Background removedBackground removedL
ine
ar
de
nsi
ty (
1/k
m/d
ay)
Lin
ea
r d
en
sity
(1
/km
/da
y)
Distance (km)
0 < t < 15'
0.5 < t < 1 day
r -1.76 +- 0.35r -1.76 +- 0.35
3 ≤ mMS
< 4
mAS
≥ 2
2 – Probabilistic approach2 – Probabilistic approach
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M = 3 earthquake (L = 400 m, u = 1 cm)
1 km
2 km
km
km
CFF (bars)
Q: can static stress triggering explain this distribution?Q: can static stress triggering explain this distribution?
2 – Probabilistic approach2 – Probabilistic approach
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a
AσΔCFFatt
a t
t
Aσ
ΔCFF++tR,Rμ=n 1eeln //
21
Rate-and-state friction
Dieterich (JGR 1994)
= # of direct aftershocks in time and distance n [0, t ] [R1,R
2]
2 – Probabilistic approach2 – Probabilistic approach
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a
AσΔCFFatt
a t
t
Aσ
ΔCFF++tR,Rμ=n 1eeln //
21
Rate-and-state friction
Dieterich (JGR 1994)
= # of direct aftershocks in time and distance n [0, t ] [R1,R
2]
2 – Probabilistic approach2 – Probabilistic approach
Background rate – density at R1 < r < R2
∝ # of background earthquakes at these distances
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Background earthquakes
Mainshock 3 ≤ m < 4
No clustering
Clustering
Euclidean volume (km3)
~ r 1.65
2 – Probabilistic approach2 – Probabilistic approach
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r -2.4
r -2.2
t ~ 1 hourt ~ 1 hour
NO
T R
ES
OL
VE
DN
OT
RE
SO
LV
ED
2 – Probabilistic approach2 – Probabilistic approach
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Observations: ~ r -1.76 ± 0.35
Static stress model: ~ r -2.30 ± 0.27
Mainshock m = 3Aftershocks up to ~ 1 hour, at 1 < r < 30 km
Mainshock m = 3Aftershocks up to ~ 1 hour, at 1 < r < 30 km
Given the uncertainties, we cannot reject triggering by static stress
Given the uncertainties, we cannot reject triggering by static stress
2 – Probabilistic approach2 – Probabilistic approach
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3 – Deformation transient3 – Deformation transient
Marsan et al. (GRL 2014)
With precursory acceleration
Without precursory acceleration
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient
With precursory acceleration
Without precursory acceleration
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient
With precursory acceleration
Without precursory acceleration
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient
Extra aftershocks from extra foreshocks
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ETAS simulations
3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient!!! POSTER by Thomas Reverso
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient!!! POSTER by Thomas Reverso
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3 – Transient deformation3 – Transient deformation3 – Deformation transient3 – Deformation transient!!! POSTER by Thomas Reverso
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Small earthquakes contribute significantly to the stress budget
They add great spatial variability to stress changes caused by large sources
They cannot be accounted for deterministically (lack of information, number)
Probabilistic approach that can be parameterized given the observed seismicity
Observation of anomalous activity reveals slow deformation transients
Conclusions