Left: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated. Right: residuals as a function of distance and azimuth.
The ANSS event ID is usp000jnrv and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000jnrv/executive.
2012/07/08 11:13:38 52.041 -60.863 11.0 3.8 Labrador, Canada
USGS/SLU Moment Tensor Solution
ENS 2012/07/08 11:13:38:0 52.04 -60.86 11.0 3.8 Labrador, Canada
Stations used:
CN.A11 CN.A21 CN.CHGQ CN.GGN CN.KAJQ CN.LMN CN.NATG CN.NMSQ
CN.SCHQ
Filtering commands used:
hp c 0.030 n 3
lp c 0.06 n 3
Best Fitting Double Couple
Mo = 6.53e+21 dyne-cm
Mw = 3.81
Z = 14 km
Plane Strike Dip Rake
NP1 35 65 80
NP2 238 27 110
Principal Axes:
Axis Value Plunge Azimuth
T 6.53e+21 68 285
N 0.00e+00 9 39
P -6.53e+21 19 132
Moment Tensor: (dyne-cm)
Component Value
Mxx -2.59e+21
Mxy 2.67e+21
Mxz 1.98e+21
Myy -2.34e+21
Myz -3.66e+21
Mzz 4.93e+21
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------------###########---##
--------###################--#
-------######################-----
------########################------
-----#########################--------
-----#########################----------
----##########################----------
----########## #############------------
---########### T ############-------------
---########### ###########--------------
---########################---------------
--#######################---------------
--#####################-----------------
-###################------------------
##################----------- ----
###############------------- P ---
##########---------------- -
######----------------------
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Global CMT Convention Moment Tensor:
R T P
4.93e+21 1.98e+21 3.66e+21
1.98e+21 -2.59e+21 -2.67e+21
3.66e+21 -2.67e+21 -2.34e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20120708111338/index.html
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STK = 35
DIP = 65
RAKE = 80
MW = 3.81
HS = 14.0
The NDK file is 20120708111338.ndk The waveform inversion is preferred.
Given the availability of digital waveforms for determination of the moment tensor, this section documents the added processing leading to mLg, if appropriate to the region, and ML by application of the respective IASPEI formulae. As a research study, the linear distance term of the IASPEI formula for ML is adjusted to remove a linear distance trend in residuals to give a regionally defined ML. The defined ML uses horizontal component recordings, but the same procedure is applied to the vertical components since there may be some interest in vertical component ground motions. Residual plots versus distance may indicate interesting features of ground motion scaling in some distance ranges. A residual plot of the regionalized magnitude is given as a function of distance and azimuth, since data sets may transcend different wave propagation provinces.
Left: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated.
Right: residuals as a function of distance and azimuth.
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The focal mechanism was determined using broadband seismic waveforms. The location of the event (star) and the stations used for (red) the waveform inversion are shown in the next figure.
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The program wvfgrd96 was used with good traces observed at short distance to determine the focal mechanism, depth and seismic moment. This technique requires a high quality signal and well determined velocity model for the Green's functions. To the extent that these are the quality data, this type of mechanism should be preferred over the radiation pattern technique which requires the separate step of defining the pressure and tension quadrants and the correct strike.
The observed and predicted traces are filtered using the following gsac commands:
hp c 0.030 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 0.5 195 30 -90 3.67 0.4886
WVFGRD96 1.0 200 30 -85 3.71 0.4914
WVFGRD96 2.0 15 60 -95 3.76 0.4673
WVFGRD96 3.0 195 90 -80 3.85 0.4570
WVFGRD96 4.0 10 90 75 3.79 0.4853
WVFGRD96 5.0 10 90 75 3.77 0.5079
WVFGRD96 6.0 10 90 70 3.75 0.5269
WVFGRD96 7.0 10 90 70 3.74 0.5403
WVFGRD96 8.0 190 85 -75 3.73 0.5504
WVFGRD96 9.0 10 90 70 3.72 0.5566
WVFGRD96 10.0 10 90 70 3.75 0.5605
WVFGRD96 11.0 190 90 -70 3.75 0.5629
WVFGRD96 12.0 35 65 80 3.82 0.5746
WVFGRD96 13.0 35 65 80 3.81 0.5802
WVFGRD96 14.0 35 65 80 3.81 0.5829
WVFGRD96 15.0 35 65 80 3.81 0.5828
WVFGRD96 16.0 35 65 80 3.81 0.5803
WVFGRD96 17.0 35 65 80 3.80 0.5755
WVFGRD96 18.0 230 60 90 3.79 0.5683
WVFGRD96 19.0 50 30 90 3.79 0.5680
WVFGRD96 20.0 50 30 90 3.82 0.5686
WVFGRD96 21.0 50 30 90 3.82 0.5660
WVFGRD96 22.0 55 30 95 3.82 0.5623
WVFGRD96 23.0 230 60 90 3.82 0.5568
WVFGRD96 24.0 55 30 95 3.82 0.5509
WVFGRD96 25.0 230 60 85 3.82 0.5441
WVFGRD96 26.0 230 60 85 3.82 0.5369
WVFGRD96 27.0 60 30 100 3.83 0.5299
WVFGRD96 28.0 230 60 85 3.83 0.5212
WVFGRD96 29.0 60 30 100 3.84 0.5137
The best solution is
WVFGRD96 14.0 35 65 80 3.81 0.5829
The mechanism corresponding to the best fit is
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The best fit as a function of depth is given in the following figure:
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The comparison of the observed and predicted waveforms is given in the next figure. The red traces are the observed and the blue are the predicted. Each observed-predicted component is plotted to the same scale and peak amplitudes are indicated by the numbers to the left of each trace. A pair of numbers is given in black at the right of each predicted traces. The upper number it the time shift required for maximum correlation between the observed and predicted traces. This time shift is required because the synthetics are not computed at exactly the same distance as the observed, the velocity model used in the predictions may not be perfect and the epicentral parameters may be be off. A positive time shift indicates that the prediction is too fast and should be delayed to match the observed trace (shift to the right in this figure). A negative value indicates that the prediction is too slow. The lower number gives the percentage of variance reduction to characterize the individual goodness of fit (100% indicates a perfect fit).
The bandpass filter used in the processing and for the display was
hp c 0.030 n 3 lp c 0.06 n 3
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| Figure 3. Waveform comparison for selected depth. Red: observed; Blue - predicted. The time shift with respect to the model prediction is indicated. The percent of fit is also indicated. The time scale is relative to the first trace sample. |
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| Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to the waveforms. Each solution is plotted as a vector at a given value of strike and dip with the angle of the vector representing the rake angle, measured, with respect to the upward vertical (N) in the figure. |
A check on the assumed source location is possible by looking at the time shifts between the observed and predicted traces. The time shifts for waveform matching arise for several reasons:
Time_shift = A + B cos Azimuth + C Sin Azimuth
The time shifts for this inversion lead to the next figure:
The derived shift in origin time and epicentral coordinates are given at the bottom of the figure.
The CUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows (The format is in the model96 format of Computer Programs in Seismology).
MODEL.01 CUS Model with Q from simple gamma values ISOTROPIC KGS FLAT EARTH 1-D CONSTANT VELOCITY LINE08 LINE09 LINE10 LINE11 H(KM) VP(KM/S) VS(KM/S) RHO(GM/CC) QP QS ETAP ETAS FREFP FREFS 1.0000 5.0000 2.8900 2.5000 0.172E-02 0.387E-02 0.00 0.00 1.00 1.00 9.0000 6.1000 3.5200 2.7300 0.160E-02 0.363E-02 0.00 0.00 1.00 1.00 10.0000 6.4000 3.7000 2.8200 0.149E-02 0.336E-02 0.00 0.00 1.00 1.00 20.0000 6.7000 3.8700 2.9020 0.000E-04 0.000E-04 0.00 0.00 1.00 1.00 0.0000 8.1500 4.7000 3.3640 0.194E-02 0.431E-02 0.00 0.00 1.00 1.00