ausblenden:
Schlagwörter:
Earthquake source observations; Wave propagation; Subduction zone processes
Zusammenfassung:
The Maule earthquake (2010 February 27, Mw 8.8, Chile) broke the subduction megathrust
along a previously locked segment. Based on an international aftershock deployment,
catalogues of precisely located aftershocks have become available. Using 23 well-located
aftershocks, we calibrate the classic teleseismic backprojection procedure to map the highfrequency
seismic radiation emitted during the earthquake. The calibration corrects traveltimes
in a standard earth model both with a static term specific to each station, and a ‘dynamic’ term
specific to each combination of grid point and station. The second term has been interpolated
over the whole slipping area by kriging, and is about an order of magnitude smaller than the
static term. This procedure ensures that the teleseismic images of rupture development are
properly located with respect to aftershocks recorded with local networks and does not depend
on accurate hypocentre location of the main shock.
We track a bilateral rupture propagation lasting ∼160 s, with its dominant branch rupturing
northeastwards at about 3 kms−1. The area of maximum energy emission is offset from the
maximum coseismic slip but matches the zone where most plate interface aftershocks occur.
Along dip, energy is preferentially released from two disconnected interface belts, and a
distinct jump from the shallower belt to the deeper one is visible after about 20 s from the
onset. However, both belts keep on being active until the end of the rupture. These belts
approximately match the position of the interface aftershocks, which are split into two clusters
of events at different depths, thus suggesting the existence of a repeated transition from
stick-slip to creeping frictional regime.