1
Probabilistic source inversion of static displacement data using neural networks Paul Käufl, Andrew Valentine & Jeannot Trampert Dep. of Earth Sciences, Utrecht University, The Netherlands Contact: p.j.kaufl@uu.nl Introduction We present a neural network based method for point source inversion in a Bayesian framework. We demonstrate the method by inverting co- seismic displacement measurements provided by real-time GPS networks. The static offset is the remaining displacement after an earthquake has occurred. We aim to investigate to what extent this relatively novel observable can con- strain point source estimates. Our method has potential for earthquake early warning (EEW) systems, since it can rapidly pro- vide source parameter estimates together with uncertainty bounds. Once a trained network is available an inversion takes only a few millisec- onds on a desktop computer. Concept Figure 1: The solution to the inverse problem is the posterior probability distribution p(m|d = d obs ) (Tarantola, 2005) — the conditional distribution p(m|d) evaluated at the observa- tion d obs . In the general case, this distribution is unknown. Figure 2: However, we can find samples of the conditional distribution p(m|d) p(m)p(d|m) given a prior distribu- tion on the model parameters p(m), and a likelihood function p(d|m), that is a data noise model and a forward modelling code. Figure 3: A mixture density network (MDN) forms a smooth, parametric approximation of the conditional probability den- sity based on a set of training samples. Once an observation is available, we can evaluate this approximation and retrieve the posterior distribution. Training set & synthetic data The training set is formed by 80.000 deviatoric point sources drawn from a uniform prior distri- bution. Synthetic static displacements are cal- culated in a layered, isotropic, elastic medium using a propagator matrix method developed by O’Toole and Woodhouse (2011). An efficient point source parametrization Uncertainties translate to distances in param- eter space. A meaningful parametrization is thus of paramount importance for probabilistic inversions. We work in the geometric moment tensor domain introduced by Tape and Tape (2012) with parameters as follows: b isotropic component, 0 for deviatoric sources (fixed) γ non double-couple component, 0 for a pure double couple κ strike σ rake h cosine of dip M W moment magnitude Demonstration: The 2010 El Mayor-Cucapah Event After training and testing the networks, we present observations for a M W 7.2, 2010 event in Baja California, which yields 1-D posterior marginal distributions. -π/6 0 π/6 γ -π/6 0 π/6 True value 0 π 2π κ (strike) 0 π 2π -π/2 0 π/2 σ (rake) -π/2 0 π/2 0 0.5 1.0 h (cos(dip)) 0 0.5 1.0 6.5 7.25 8.0 M W 6.5 7.25 8.0 True value 2 12 22 depth [km] 2 12 22 31.2 31.95 32.7 lat [ ] 31.2 31.95 32.7 -117 -116 -115 lon [ ] -117 -116 -115 0.0 0.3 0.6 0.9 1.2 1.5 1.8 2.1 2.4 2.7 3.0 nats 0.0 0.8 γ 0 300 600 900 1200 0 1 κ 0 50 100 150 200 0 1 σ 0 80 160 240 0.0 0.6 h 0 150 300 450 0.0 1.5 M W 0 50 100 150 200 0.0 0.8 depth 0 300 600 900 1200 0 3 lat 0 40 80 120 160 0 3 lon 0 40 80 120 160 Figure 4: The network performance is assessed using another 4000 examples — the test set. Left: Predicted mode of the distribution vs the true value. Right: Histograms of the information gain — the distance between prior and posterior distribution (colour coded in the left plot). A small information gain indicates that the posterior closely resembles the prior. Not all parameters can be predicted well. -π/6 0 π/6 γ 0.0 0.5 1.0 1.5 2.0 GCMT USGS CMT USGS W phase Melgar et al (2011) O’Toole et al. (2013) Wei et al. (2011) 0 π 2π κ (strike) 0.00 0.06 0.12 0.18 0.24 -π/2 0 π/2 σ (rake) 0.0 0.4 0.8 1.2 1.6 0 0.5 1 h (cos[dip]) 0.0 0.8 1.6 2.4 3.2 6.5 7.25 8.0 M W 0 1 2 3 4 2 12 22 depth [km] 0.000 0.025 0.050 0.075 0.100 31.2 31.95 32.7 lat [ ] 0 2 4 6 8 -117 -116 -115 lon [ ] 0.0 2.5 5.0 7.5 10.0 -π/6 0 π/6 γ 0.0 0.5 1.0 1.5 2.0 0 5% 10% 20% 0 π 2π κ (strike) 0.00 0.08 0.16 0.24 0.32 0.40 -π/2 0 π/2 σ (rake) 0.0 0.4 0.8 1.2 1.6 0 0.5 1 h (cos[dip]) 0.0 0.6 1.2 1.8 2.4 6.5 7.25 8.0 M W 0 1 2 3 4 2 12 22 depth [km] 0.000 0.025 0.050 0.075 0.100 31.2 31.95 32.7 lat [ ] 0 2 4 6 8 -117 -116 -115 lon [ ] 0.0 2.5 5.0 7.5 10.0 Figure 5: Inversion results for the 2010 M w 7.2 El Mayor- Cucapah event. Vertical lines denote the position of other published moment-tensor point source solutions (Melgar et al., 2012; O’Toole et al., 2012; Wei et al., 2011). Prior distributions are shown in green. Our uncertainty estimates comprise most other solutions. Figure 6: Influence of different amounts of perturbations of the 1-D crustal Earth model on the posterior marginals. The sensitivity with respect to the Earth model seems minimal. Most parameters are unaffected up to unrealistically large variations of 20%. References Melgar, D., Y. Bock, and B. W. Crowell (2012, February). Real-time centroid moment tensor determination for large earthquakes from local and regional displacement records. Geophysical Journal International 188 (2), 703–718. O’Toole, T. B., A. P. Valentine, and J. H. Woodhouse (2012). Centroid-moment tensor inversions using high-rate GPS waveforms. Geophysical Journal International 191(1), 257–270. O’Toole, T. B. and J. H. Woodhouse (2011). Numerically stable computation of complete synthetic seismograms in- cluding the static displacement in plane layered media. Geophysical Journal International 187 (3), 1516–1536. Tape, W. and C. Tape (2012, July). A geometric set- ting for moment tensors. Geophysical Journal Interna- tional 190 (1), 476–498. Tarantola, A. (2005). Inverse Problem Theory. Number 4. SIAM. Wei, S., E. Fielding, S. Leprince, A. Sladen, J.-P. Avouac, D. Helmberger, E. Hauksson, R. Chu, M. Simons, K. Hud- nut, T. Herring, and R. Briggs (2011, July). Superficial sim- plicity of the 2010 El Mayor–Cucapah earthquake of Baja California in Mexico. Nature Geoscience 4(9), 615–618. Conclusions A probabilistic neural network inversion yields re- alistic uncertainty estimates and is able to deal with non-unique and multi-modal mappings. Computational demands are low, once a trained network is available, making the method suitable for EEW purposes. Static displacements provide robust information on location and magnitude and show little sensi- tivity to the crustal model. The flexible treatment of input data makes it possible to perform joint inversions of different data types, such as displacement waveforms and strong-motion accelerograms. A potential that still remains to be explored.

Probabilistic source inversion of static displacement data ...Probabilistic source inversion of static displacement data using neural networks Paul Käufl, Andrew Valentine & Jeannot

  • Upload
    others

  • View
    11

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Probabilistic source inversion of static displacement data ...Probabilistic source inversion of static displacement data using neural networks Paul Käufl, Andrew Valentine & Jeannot

Probabilistic source inversion of static displacement data using neural networksPaul Käufl, Andrew Valentine & Jeannot TrampertDep. of Earth Sciences, Utrecht University, The Netherlands

Contact: [email protected]

Introduction

We present a neural network based method forpoint source inversion in a Bayesian framework.

We demonstrate the method by inverting co-seismic displacement measurements providedby real-time GPS networks. The static offset is

the remaining displacement after an earthquakehas occurred. We aim to investigate to whatextent this relatively novel observable can con-strain point source estimates.

Our method has potential for earthquake early

warning (EEW) systems, since it can rapidly pro-vide source parameter estimates together withuncertainty bounds. Once a trained network isavailable an inversion takes only a few millisec-onds on a desktop computer.

Concept

Figure 1: The solution to the inverse problem is the posteriorprobability distribution p(m|d = dobs) (Tarantola, 2005) —the conditional distribution p(m|d) evaluated at the observa-tion dobs. In the general case, this distribution is unknown.

Figure 2: However, we can find samples of the conditionaldistribution p(m|d) ! p(m)p(d|m) given a prior distribu-tion on the model parameters p(m), and a likelihood functionp(d|m), that is a data noise model and a forward modellingcode.

Figure 3: A mixture density network (MDN) forms a smooth,parametric approximation of the conditional probability den-sity based on a set of training samples. Once an observationis available, we can evaluate this approximation and retrievethe posterior distribution.

Training set & synthetic data

The training set is formed by 80.000 deviatoricpoint sources drawn from a uniform prior distri-bution. Synthetic static displacements are cal-culated in a layered, isotropic, elastic mediumusing a propagator matrix method developed byO’Toole and Woodhouse (2011).

An efficient point source parametrization

Uncertainties translate to distances in param-eter space. A meaningful parametrization isthus of paramount importance for probabilisticinversions. We work in the geometric momenttensor domain introduced by Tape and Tape(2012) with parameters as follows:

b isotropic component, 0 for deviatoricsources (fixed)

! non double-couple component, 0 for apure double couple

" strike# rakeh cosine of dipMW moment magnitude

Demonstration: The 2010 El Mayor-Cucapah Event

After training and testing the networks, wepresent observations for a MW 7.2, 2010 event

in Baja California, which yields 1-D posteriormarginal distributions.

!!/6 0 !/6"

!!/6

0

!/6

True

valu

e

0 ! 2!

# (strike)

0

!

2!

!!/2 0 !/2$ (rake)

!!/2

0

!/2

0 0.5 1.0

h (cos(dip))

0

0.5

1.0

6.5 7.25 8.0MW

6.5

7.25

8.0

True

valu

e

2 12 22

depth [km]

2

12

22

31.2 31.95 32.7

lat ["]

31.2

31.95

32.7

!117 !116 !115

lon ["]

!117

!116

!115

0.0

0.3

0.6

0.9

1.2

1.5

1.8

2.1

2.4

2.7

3.0

nats 0.0 0.8

"

0

300

600

900

1200

0 1

#

0

50

100

150

200

0 1

$

0

80

160

240

0.0 0.6

h

0

150

300

450

0.0 1.5MW

0

50

100

150

200

0.0 0.8

depth

0

300

600

900

1200

0 3

lat

0

40

80

120

160

0 3

lon

0

40

80

120

160

Figure 4: The network performance is assessed using another 4000 examples — the test set. Left: Predicted mode ofthe distribution vs the true value. Right: Histograms of the information gain — the distance between prior and posteriordistribution (colour coded in the left plot). A small information gain indicates that the posterior closely resembles the prior.Not all parameters can be predicted well.

!!/6 0 !/6"

0.0

0.5

1.0

1.5

2.0

GCMT

USGS CMT

USGS W phase

Melgar et al (2011)

O’Toole et al. (2013)

Wei et al. (2011)

0 ! 2!# (strike)

0.00

0.06

0.12

0.18

0.24

!!/2 0 !/2$ (rake)

0.0

0.4

0.8

1.2

1.6

0 0.5 1

h (cos[dip])

0.0

0.8

1.6

2.4

3.2

6.5 7.25 8.0MW

0

1

2

3

4

2 12 22

depth [km]

0.000

0.025

0.050

0.075

0.100

31.2 31.95 32.7lat ["]

0

2

4

6

8

!117 !116 !115

lon ["]

0.0

2.5

5.0

7.5

10.0

!!/6 0 !/6

"

0.0

0.5

1.0

1.5

2.0

0 5% 10% 20%

0 ! 2!

# (strike)

0.00

0.08

0.16

0.24

0.32

0.40

!!/2 0 !/2

$ (rake)

0.0

0.4

0.8

1.2

1.6

0 0.5 1

h (cos[dip])

0.0

0.6

1.2

1.8

2.4

6.5 7.25 8.0MW

0

1

2

3

4

2 12 22

depth [km]

0.000

0.025

0.050

0.075

0.100

31.2 31.95 32.7

lat ["]

0

2

4

6

8

!117 !116 !115

lon ["]

0.0

2.5

5.0

7.5

10.0

Figure 5: Inversion results for the 2010 Mw 7.2 El Mayor-Cucapah event. Vertical lines denote the position of otherpublished moment-tensor point source solutions (Melgaret al., 2012; O’Toole et al., 2012; Wei et al., 2011). Priordistributions are shown in green. Our uncertainty estimatescomprise most other solutions.

Figure 6: Influence of different amounts of perturbations ofthe 1-D crustal Earth model on the posterior marginals. Thesensitivity with respect to the Earth model seems minimal.Most parameters are unaffected up to unrealistically largevariations of 20%.

References

Melgar, D., Y. Bock, and B. W. Crowell (2012, February).Real-time centroid moment tensor determination for largeearthquakes from local and regional displacement records.Geophysical Journal International 188(2), 703–718.

O’Toole, T. B., A. P. Valentine, and J. H. Woodhouse (2012).Centroid-moment tensor inversions using high-rate GPSwaveforms. Geophysical Journal International 191(1),257–270.

O’Toole, T. B. and J. H. Woodhouse (2011). Numericallystable computation of complete synthetic seismograms in-cluding the static displacement in plane layered media.Geophysical Journal International 187 (3), 1516–1536.

Tape, W. and C. Tape (2012, July). A geometric set-ting for moment tensors. Geophysical Journal Interna-tional 190(1), 476–498.

Tarantola, A. (2005). Inverse Problem Theory. Number 4.SIAM.

Wei, S., E. Fielding, S. Leprince, A. Sladen, J.-P. Avouac,D. Helmberger, E. Hauksson, R. Chu, M. Simons, K. Hud-nut, T. Herring, and R. Briggs (2011, July). Superficial sim-plicity of the 2010 El Mayor–Cucapah earthquake of BajaCalifornia in Mexico. Nature Geoscience 4(9), 615–618.

Conclusions

A probabilistic neural network inversion yields re-alistic uncertainty estimates and is able to dealwith non-unique and multi-modal mappings.Computational demands are low, once a trainednetwork is available, making the method suitablefor EEW purposes.Static displacements provide robust information

on location and magnitude and show little sensi-tivity to the crustal model.The flexible treatment of input data makes itpossible to perform joint inversions of differentdata types, such as displacement waveformsand strong-motion accelerograms. A potentialthat still remains to be explored.