Toward understanding tectonic control on the Mw 8.8 2010 Maule Chile earthquake
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Moreno, M.
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Toward understanding tectonic control on the Mw 8.8 2010 Maule Chile earthquake
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Abstract
The Maule earthquake of 27th February 2010 (Mw=8.8) affected ~500 km of the Nazca-South America plate
boundary in south-central Chile producing spectacular crustal deformation. Here, we present a detailed estimate
of static coseismic surface offsets as measured by survey and continuous GPS, both in near- and farfield
regions. Earthquake slip along the megathrust has been inferred from a joint inversion of our new
data together with published GPS, InSAR, and land-level changes data using Green's functions generated by
a spherical finite-element model with realistic subduction zone geometry. The combination of the data sets
provided a good resolution, indicating that most of the slip was well resolved. Coseismic slip was concentrated
north of the epicenter with up to 16 m of slip, whereas to the south it reached over 10m within two minor
patches. A comparison of coseismic slip with the slip deficit accumulated since the last great earthquake in
1835 suggests that the 2010 event closed a mature seismic gap. Slip deficit distribution shows an apparent
local overshoot that highlight cycle-to-cycle variability,which has to be taken into accountwhen anticipating future
events from interseismic observations. Rupture propagation was obviously not affected by bathymetric features
of the incoming plate. Instead, splay faults in the upper plate seem to have limited rupture propagation in
the updip and along-strike directions. Additionally, we found that along-strike gradients in slip are spatially
correlated with geometrical inflections of the megathrust. Our study suggests that persistent tectonic features
may control strain accumulation and release along subduction megathrusts.
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Artículo de publicación ISI
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MARISCOS project (LA 2970/1-1) granted by the German
Science Foundation (DFG
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URI: https://repositorio.uchile.cl/handle/2250/125651
DOI: doi:10.1016/j.epsl.2012.01.006
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Earth and Planetary Science Letters 321-322 (2012) 152–165
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