adv advanced anced worksho shop p on n ea earthquake fa
play

Adv Advanced anced Worksho shop p on n Ea Earthquake Fa Fault - PowerPoint PPT Presentation

Adv Advanced anced Worksho shop p on n Ea Earthquake Fa Fault Mechanics: The Theory, , Simulation on and Observation ons ICTP, Trieste, Sept 2-14 2019 Lecture 8: dynamic source inversion Jean Paul Ampuero (IRD/UCA Geoazur) Dy


  1. Adv Advanced anced Worksho shop p on n Ea Earthquake Fa Fault Mechanics: The Theory, , Simulation on and Observation ons ICTP, Trieste, Sept 2-14 2019 Lecture 8: dynamic source inversion Jean Paul Ampuero (IRD/UCA Geoazur)

  2. Dy Dynamic so source i inversi sion • Definition • Early attempts • Trade-offs • Simplified parameterizations • State-of-the-art • Perspectives

  3. Kinematics and dynamics Ground motion observations : Seismograms of the Seismograms , geodesy Northridge earthquake Waveforms + static deformation n 1994 M6.7 Spectra n Radiated energy n HF envelopes n Kinematic models (how?) Kinematic model à description of the earthquake (Wald et al 1996) rupture history : Local final slip n Rise time n Rupture velocity n Dynamic models (why?) à Physical interpretation of earthquake rupture : Fault constitutive law : strength , weakening, • fracture energy, etc Dynamic model (Nielsen and Olsen 2000), • Initial conditions: stress , state, etc dashed contours = high initial stress

  4. Early attempts of dynamic source inversion ! " # Prior model ! " # Preferred model Final slip Peyrat et al (2001) Preferred 1992 Landers earthquake model Trial and error inversion. Fixed Dc

  5. Peyrat et al (2001) 1992 Landers earthquake

  6. Peyrat et al (2001) - 1992 Landers earthquake

  7. Peyrat and Olsen (2004) 2000 Mw 6.6 Tottori, Japan earthquake Non-linear inversion by Neighborhoood Algorithm

  8. Non-linear inversion required 60,000 computations of forward problem Peyrat and Olsen (2004) - 2000 Mw 6.6 Tottori, Japan earthquake

  9. Trade-off between dynamic rupture parameters Spudich & Guatteri: trade-off between ! " − ! $ and % & when the inversion is based on low frequency data Physical explanation: • Static elasticity à final slip %(() depends linearly on stress drop Δ! ( = ! , (() − ! $ (() • Fracture mechanics à First-order aspects of dynamic rupture depend on the non-dimensional number 1 2 31 4 5 6 - = . , /. & ∼ 7 1 8 31 4 9 :

  10. Di Carli et al (2010) - Tottori earthquake Dynamic source inversion based on elliptical patches

  11. Dynamic source inversion Forward problem is computationally expensive à optimized FD code, simple geometry Gallovic et al (JGR 2019) Uncertainty quantification à Bayesian sampling with Parallel Tempering Monte Carlo

  12. Dynamic source inversion Gallovic et al (JGR 2019) Synthetic test Input dynamic parameters of the target model (SIV Inv1 test problem)

  13. Dynamic source inversion Gallovic et al (JGR 2019) Synthetic test Verify the simplified FD code by comparison to a more complete but more expensive code, WaveQLab3D

  14. Dynamic source inversion Gallovic et al (JGR 2019) Properties of the inverted rupture model with the largest Model VR = 0.71 (its Data VR is 0.94)

  15. Dynamic source inversion Gallovic et al (JGR 2019) Properties of the inverted rupture model with the largest Data VR = 0.97

  16. Dynamic source inversion Gallovic et al (JGR 2019) Kinematic source properties

  17. Dynamic source inversion Gallovic et al (JGR 2019) Dynamic source parameters

  18. Dynamic source inversion Gallovic et al (JGR 2019) Mean strength τ s versus mean D c for all accepted model samples Trade-off is weak Histograms of model parameters at three selected points

  19. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019)

  20. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Best-fitting dynamic source model Frequency band 0.05–1.0 Hz (AMT and NRC) and 0.05–0.5 Hz (others) Variance reduction = 0.62

  21. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Kinematic parameters of the best-fitting model

  22. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Dynamic parameters of the best-fitting model

  23. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Ensemble properties: Histograms of rupture parameters

  24. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Ensemble properties: Mean and variance of rupture parameters

  25. Dynamic source inversion Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019) Ensemble properties: Mean and variance of rupture parameters

  26. Dynamic source inversion Gallovic et al (JGR 2019) Application to the 2016 Amatrice earthquake Verify the simplified FD code by comparison to a more complete but more expensive code, WaveQLab3D

  27. Dynamic source inversion Velocity waveforms for the best-fitting model, 0.05– 5.0 Hz Application to the 2016 Amatrice earthquake Gallovic et al (JGR 2019)

  28. Dynamic source inversion Continued development of dynamic source inversion enabled by advances in computational power and sampling algorithms Provides physics-based regularization of the inverse problem Challenges ahead: • Finer scale resolution of dynamic parameters • More realistic friction laws + off-fault dissipation • Include uncertainties in crustal structure (model covariance Cp)

Recommend


More recommend