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Studying finiteness of the earthquake source using 3D global waveform
modeling
Earthquakes
that have a source dimension in time and space smaller than
the period and wavelength of the waves of interest can be viewed
as a point source to a good approximation. However, for a few
events the effect of the finite source on the waveforms is significant
even at long periods. In those cases we can use synthetic waveforms
computed for different source models to extract information
about the kinematics of the rupture. |
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earthquakes propagate unilaterally along long faults they
radiate waves that look very different depending on the direction
we look at them from. Waves propagating in the rupture direction
produce a very narrow but high pulse, but those propagating
in the anti rupture direction are low amplitude and spread
out. |
Application
to the 2001, Mw 7.9 Kunlun, China, earthquake
Vala
Hjorleifsdottir looked at the Mw 7.9, Nov 14, 2001,
Kunlun, China event, which propagated eastward over a 400 km
long section of the Kunlun fault. By quantifying the azimuthal
phase-shift between observed data and synthetics calculated
for different rupture speeds, we can put bounds on what values
of rupture speeds are consistent with the data.
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| 9/29/06rect.gif" width="450" height="280"> |
A
comparison between data and synthetics for Rayleigh-waves
computed for source models with two distinct rupture speeds,
2.5 km/s and 4.5 km/s respectively. Notice that the synthetics
arrive later than the data in the rupture direction (90 degrees)
for the slower rupture speed but later in the anti-rupture
direction (270 degrees) and vice versa for the faster rupture
speed. We estimated the rupture speed to be 3.4-3.8 km/s.
This value is very close to the shear wave velocity of the
material the fault broke, indicating that not much energy
is going into the fracture and friction on the fault.
Currently we are working on methods to quantify the variation
of rupture speed in time and space.
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Application to the 2002 Mw 7.9 Denali fault, Alaska, earthquake
Dr.
Chen Ji constructed the slip history of the 2002
Mw 7.9 Denali fault earthquake, which ruptured a fault plane
320 km long. He then used the SEM code to evaluate his result.
After taking several cutting-edge results, such as 3D mantle
tomography model S20RTS [Ritsema et al., 1999], CRUST2.0 crustal
model [Laske et al., http://mahi.ucsd.edu/Gabi/rem.html, 2001],
ETOPO5, and finite fault slip model of the earthquake [Ji et
al., 2004] into account, we were able to fit the broadband teleseismic
body waves (f<0.2 Hz), and long period surface waves (T>40
sec) fairly well.
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Fault
geometry of the November 3, 2002, Denali earthquake. Below:
The five red boxes labeled A--E that denotes the surface projections
of the five fault segments that were involved in the rupture.
Bottom: Slip distribution along the five fault segments A--E
shown.
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To the right of each station are shown the data in black and
the 3D SEM synthetic seismograms in red. Both data and synthetics
are bandpass filtered between periods of 5 and 150 seconds.
The epicenter is denoted by the black star. Top:
P waves on the vertical component. Bottom:
S waves on the transverse component. Note the strong amplification
in the direction of rupture, as stations in N-America record
much larger amplitudes than those in other parts of the world.
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