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1 Cecil H. and Ida M. Green Institute
of Geophysics and Planetary Physics
Scripps Institution of Oceanography
University of California, San Diego
La Jolla, California 92093-0225
We examine aftershock detectability thresholds for events in the initial part
of the 31 October 2001, ML 5.1 sequence in southern
California. This sequence occurred directly below the broadband ANZA
seismic network, which recorded continuous waveform data at 13 azimuthally
well-distributed stations within the study region (seven had epicentral
distances < 20 km). Of the 608 aftershocks (0 < ML
<
2.8) in the initial 2 hr of this sequence, the first five aftershocks
recorded were only identifiable at stations within 30 km after applying a
high-pass filter. Using a cluster (radius
1.1 km) of 200 representative
aftershocks, we track the maximum seismogram amplitude versus earthquake
magnitude. This relationship helps us quantify the visibility of aftershocks
within the mainshock coda and assess our detection capabilities. We estimate
that detectable aftershocks within the mainshock coda include (1) those over
magnitude
3 that are within 15 km of the network centroid that occur 12 sec
or more into the sequence, and (2) those over magnitude
2 that are within
30 km of the centroid of the network that occur 60 sec or more into the
sequence. We find a lack of large aftershocks in this sequence. The largest
aftershock (ML
2.8) is substantially smaller than the
mainshock (ML 5.1). We suggest this relatively
large-magnitude differential is dictated by a combination of factors that
includes complexity of the San Jacinto fault system and the lack of large
earthquakes in the region in the past
20 years.
Online material: Quicktime movies juxtaposing a 3.2 aftershock in the coda of a 5.1 mainshock.
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