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Matthew W. Herman1, Kevin P. Furlong1, Rob Govers2
1The Pennsylvania State University, 2Utrecht University
Constraining interseismic deformation processes in subduction zones through simple mechanical models
1 8 5 5
PENNSTATE GEODYNAMICS
IntroductionIn between earthquakes (the interseismic period), plates are frictionally locked at asperities. One way to model deformation around asperities is with dislocations embedded in an elastic half-space (e.g. Okada, 1992). In this framework, deformation generated by a slip deficit patch is represented with back-slip (opposite the direction of plate motion; Savage, 1983), and the rest of the system deforms as an unbroken elastic medium. This approach has led to misconceptions, such as:
Locked regions accumulate full slip deficit, while unlocked regions accumulate zero slip deficit.
Unlocked
Locked – Abrupt TransitionHigh shear stress
Lock
edLo
cked
Locked – Gradual Transition
Lock
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Consider a schematic plate moving in the direction of the arrows. In a totally unlocked system, the plate moves uniformly without deforming.
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If slip goes from zero inside the locked patch to the plate rate immediately outside, large stresses accumulate at the edge. However, the interface can slide in response to these stresses.
At a locked segment, the plate is restricted from moving. Outside the locked zone, the material deforms in response to the locking, so there is a transition zone over which slip goes from zero to plate rate.
Metois et al. (2016)
1000 km400 km
100 km
25º
WidthLength
Trench
+x +y
+z
Fixed
Model SetupWe use a 3-D finite element model of a subduction zone to explore how elastic strain accumulates around a locked asperity. Deformation is driven by relative motion: down-dip displacement is applied to both ends of the subducting plate and the back of the upper plate is held fixed. At rectangular asperities, the plates are locked together, while the rest of the plate interface is allowed to slide freely. The finite element approach allows us to apply these boundary conditions that are representative of the first-order frictional state of the megathrust. 0
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0.0 0.1 0.2 0.3 0.4 0.5Slip (m)
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0 20 40 60 80 100 120 140 160 180Depth (km) 0.5 meters
Surface Displacement Megathrust Slip
Arrows show upper plate slip
Surface Interface
0.0 0.1 0.2 0.3 0.4
Effective Stress (MPa)0 400-100 100 200 300
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Single Fault ResultsWe take transects along the megathrust (dashed lines) and plot the fault slip along these paths. The frictionally locked zone (green) has zero slip by definition. The region outside the asperity is able to slide freely (orange), and as a result of the locking, slip is reduced near the asperity. With increasing distance from the asperity, fault slip recovers to the full plate motion rate. This appears as a “halo” of reduced slip surrounding the asperity.
Stresses - What controls the observed deformation?Resistance to plate motion at the asperity causes shear stress to increase around the locked patch. This drives slip on the adjacent freely sliding region, which we model as a plane of zero shear stress resolved on it.
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Depth (km)
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Along−Dip (km)0 400300200100
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Along−Strike (km)0 1000900800700600500400300200100
Frictionally lockedFree to slide
If we model only the effects of the asperity, the predicted deformation is incomplete (green). The halo of reduced slip also contributes to surface displacements (orange). An inversion of the full signal sees the halo as a zone of partial coupling. This coupling is due to proximity to the asperity, rather than being indicative of frictional characteristics at that point.
Surface Displacements
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isp
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Asperity + Halo
Asperity only
Faul
t Slip
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io
A consequence of this increased area of slip deficit is that the eventual earthquake rupture can be larger than expected based on the area of the asperity alone (perhaps like Tohoku?). The total moment deficit is 2-3x greater than the deficit within the locked zone. This is critical up-dip of the locked patch; although this area may not be frictionally locked, slip deficit near the trench may approach full plate motion if adjacent to a shallow asperity.
Trench
Trench
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0.10 0.05 0.00 0.05 0.10
Shear Stress (MPa)
Shear stress from back-slip on a locked fault in a half-space, computed using Okada (1992) equations
Drives slip on interface
Modeled shear stress after freely sliding interface has slipped to resolve zero shear stress
Interface has slipped
Effective stress is a measure of the amplitude of the stress tensor
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Ozawa et al. (2012)Yue and Lay (2011)
0 10009008007006005004003002001000.0
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Offset: 20 km (0.5 fault length)
0 10009008007006005004003002001000.0
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Offset: 40 km (1 fault length)
Along−Strike (km)0 1000900800700600500400300200100
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Offset: 120 km (3 fault lengths)
0.0 0.1 0.2 0.3 0.4 0.5Slip (m)
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Multiple Asperity InteractionsCurrent models of the subduction interface have numerous asperities within the seismogenic zone (depths of 10-50 km). This interpretation is based on the distribution of seismicity on the plate boundary and seismological analyses of large megathrust earthquakes. If these asperities are close enough, their slip reduction halos will overlap.
First, we consider two equal-size asperities at the same depth on the megathrust, separated along strike (the y-direction).
Asperities
Lay et al. (2012)
Faul
t Slip
Rat
io
80% apparentcoupling
70% apparentcoupling
40% apparentcoupling
Single asperityslip deficit
0 10009008007006005004003002001000.0
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Along−Strike (km)
If an earthquake ruptures one asperity only the excess slip deficit can contribute to the event, while the rest of the boundary is held in place by the other locked area.
Area that slipsif one asperityand rest ofinterface areunlocked
SummaryInterpretations of interseismic coupling should consider how locked asperities affect the slip in the adjacent frictionally weak regions. The common interpretation of full slip deficit within asperities and zero slip deficit outside is physically unreasonable. Instead, a halo of apparent partial coupling should surround asperities. To first order, this halo effect around smaller asperities can explain much of the observed coupling patterns (e.g. in the subduction zone offshore Chile).
ReferencesLay et al. (2012). Depth-varying rupture properties of subduction zone megathrust faults. Journal of Geophysical Research 117.Metois et al. (2016). Interseismic coupling, megathrust earthquakes and seismic swarms along the Chilean Subduction Zone (38º-18ºS). Pure and Applied Geophysics 173.Okada (1992). Internal deformation due to shear and tensile faults in a half-space. Bulletin of the Seismological Society of America 82.Ozawa et al. (2011). Coseismic and postseismic slip of the 2011 magnitude-9 Tohoku-Oki earthquake. Nature 475.Savage (1983). A dislocation model of strain accumulation and release at a subduction zone. Journal of Geophysical Research 88.Yue and Lay (2011). Inversion of high-rate (1 sps) GPS data for rupture process of the 11 March 2011 Tohoku earthquake (Mw 9.1). Geophysical Research Letters 38.
−72˚− 68˚
−32˚
−28˚
−24˚
−20˚
60 k
m
−72˚− 68˚
−32˚
−28˚
−24˚
−20˚
Observed GPS Inverted Coupling Modeled SlipModeled
Displacements
Area that slips ifonly asperity is
unlocked
Surface Interface
Metois et al. (2016) Shear stress 20 km above fault plane0.10 0.05 0.00 0.05 0.10
Shear Stress (MPa)