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find direction of signals based on Array algorithms backtrace ray paths through the earth simplifications: flat earth, plane waves usually high or reasonable waveform similarity. Teleseismic Location. Epicentre Location using Arrays.
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find direction of signals based on Array algorithms backtrace ray paths through the earth simplifications: flat earth, plane waves usually high or reasonable waveform similarity Teleseismic Location
Epicentre Location using Arrays Problem: inaccuracy due to deviations from velocity model at the receiver Solution: array calibration (empirical corrections to direction)
Principle of Array Analysis for a given station geometry: t1, t2, t3 (observed) → plane wave (azimuth and slowness) → t1', t2', t3' (theo)
Validate result apply negative (t1',t2',t3')
for appropriate configuration t1, t2,..., tn (observed) → plane wave → t1', t2',..., tn' (theo) (t1, t2, ... , tn) ≈ (t1', t2', ... , tn' )
aperture too large / frequencies too high high veloc. low veloc. t1, t2,..., tn (observed) → plane wave → t1', t2',..., tn' (theo) (t1, t2, ... , tn) ≠ (t1', t2', ... , tn' )
Plane wave determination without picking FK Algorithm
Two ways of determining the plane wave a) measure t1,t2,t3 directly and invert for slowness,azimuth b) try many plane waves systematically, inversely apply (t1',t2',t3') delays and sum: compare summation amplitudes assume plane wave with slowness and azimuth, compute theoretical delays (t1',t2',t3') and apply, in most cases it looks like this: if you come close the true values of slowness and azimuth you will get aligen signals and constructive summation:
FK diagram destructive summation (wrong t1', t2', t3') 330° 30° azimuth slowness 12 300° 8 60° constructive summation (correct t1', t2', t3') 4 240° 120° 210° 150°
Example: FK analysis, GRF arrayEvent S. XinJiang, 25-Jul-2007, mb 4.6 330° 30° azimuth slowness 12 300° 8 60° 4 240° 120° 210° 150°
Tradeoff: location accuracy and coherency Array aperture no coherency no array features location possible, good array features low coherency low resolution Frequency
Arrays in Germany GERES: aperture ~4km frequencies: 1 - 50 Hz GRF: aperture ~100km frequencies: 0.1 – 5 Hz GRSN: aperture ~1000km frequencies: 0.01 – 0.5 Hz
Resolution of German Arrays Array aperture GRSN no coherency no array features location possible, GRF good array features low coherency GERES low resolution 0.05 1 Frequency (Hz) 50
Benefits of Array Data Processing • Improvement of signal/noise ratio • Determination of slowness and azimuth • Phase identification • Location of remote events • Rupture tracking
XinJiang event, time domainImprovement of signal/noise ratio