Earthquake dynamics and source inversion Jean-Paul Ampuero
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31.07.2018
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Earthquake
dynamics and source inversion
Jean-Paul Ampuero
ETH Zurich
Overview
The forward problem: challenges, open questions
Dynamic properties inferred from kinematic models
Direct inversion for dynamic properties: which parameters can be resolved ?
Perspectives
The “standard”
dynamic rupture problem
Fault geometry and velocity model ?
Initial conditions ?
Fault constitutive law (“friction law”) ?
Input:
Geological field observations
Geophysical
boreholes
Laboratory
Strong motion seismology
Candidate ingredients:
Dry
friction
Frictional heating
Melting
Fluid thermal pressurization
Off-fault damage
Compaction / porosity evolution
Fault constitutive law (“friction law”) ?
Input:
Geological field observations
Geophysical boreholes
Laboratory
Strong motion seismology
Fault constitutive law (“friction law”) ?
Inferring fault dynamic properties from seismograms
Inferring fault dynamic properties from seismograms
Fracture energy
Gc controls dynamic rupture
Inversion of dynamic friction parameters with frequency band-limited data suffers from strong
trade-off
Scale contraction issue
Scale contraction issue
The view from
classical fracture mechanics
Gc controls dynamic rupture: theory
Classical fracture mechanics +Griffith criterion
local energy balance at the rupture front:
Gc = G(vr, L, )
crack tip equation of motion relates rupture speed to Gc
Gc = f(vr) Gstatic(L,)
Gc = f(vr) K2(L,)/2
where: stress intensity factor =
K ≈ √L
and
f(vr)
is a universal decreasing function
Summary
So far:
The development of dynamic source inversion methodologies
is in its infancy
Parameterization issue
Resolution limited by:
Data band-pass filtering
Attenuation
Inaccurate Green’s functions, poor knowledge of the crust
Scarce
instrumentation
Coarse parameterization, computational cost
Ideal wish-list:
Reach higher frequencies
Understand the meaning of the inferred
macroscopic parameters
Faster, better forward solvers
2.5D dynamic inversion
Dynamic source inversion = from seismograms +GPS +InSAR to spatial distribution of initial stress and fracture energy along the fault
Computationally expensive
and low vertical resolution
Reduce the problem dimensionality:
solve rupture dynamics averaged over the seismogenic depth (3D wave equation 2D Klein-Gordon equation)
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