The ANSS event ID is ak01234mu8s7 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak01234mu8s7/executive.
2012/03/08 10:57:42 61.007 -150.914 10.0 4.0 Alaska
USGS/SLU Moment Tensor Solution ENS 2012/03/08 10:57:42:0 61.01 -150.91 10.0 4.0 Alaska Stations used: AK.BPAW AK.CAST AK.CCB AK.DHY AK.DIV AK.EYAK AK.GLI AK.KLU AK.KTH AK.MCK AK.MLY AK.PPLA AK.RIDG AK.RND AK.SAW AK.SCM AK.SKN AK.SSN AK.SWD AK.TRF IU.COLA Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.55e+22 dyne-cm Mw = 4.06 Z = 30 km Plane Strike Dip Rake NP1 43 78 118 NP2 155 30 25 Principal Axes: Axis Value Plunge Azimuth T 1.55e+22 50 343 N 0.00e+00 27 217 P -1.55e+22 28 111 Moment Tensor: (dyne-cm) Component Value Mxx 4.36e+21 Mxy 2.34e+21 Mxz 9.63e+21 Myy -1.00e+22 Myz -8.10e+21 Mzz 5.67e+21 ############## -##################### --########################## --###########################- ---########## ##############---- ----########## T #############------ ----########### ############-------- -----########################----------- -----#######################------------ ------######################-------------- ------####################---------------- ------##################------------------ ------#################----------- ----- ------##############------------- P ---- -------###########--------------- ---- -------########----------------------- -------#####------------------------ ---------------------------------- ---####----------------------- #########------------------- #########------------- ############## Global CMT Convention Moment Tensor: R T P 5.67e+21 9.63e+21 8.10e+21 9.63e+21 4.36e+21 -2.34e+21 8.10e+21 -2.34e+21 -1.00e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20120308105742/index.html |
STK = 155 DIP = 30 RAKE = 25 MW = 4.06 HS = 30.0
The NDK file is 20120308105742.ndk The waveform inversion is preferred.
The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
USGS/SLU Moment Tensor Solution ENS 2012/03/08 10:57:42:0 61.01 -150.91 10.0 4.0 Alaska Stations used: AK.BPAW AK.CAST AK.CCB AK.DHY AK.DIV AK.EYAK AK.GLI AK.KLU AK.KTH AK.MCK AK.MLY AK.PPLA AK.RIDG AK.RND AK.SAW AK.SCM AK.SKN AK.SSN AK.SWD AK.TRF IU.COLA Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.55e+22 dyne-cm Mw = 4.06 Z = 30 km Plane Strike Dip Rake NP1 43 78 118 NP2 155 30 25 Principal Axes: Axis Value Plunge Azimuth T 1.55e+22 50 343 N 0.00e+00 27 217 P -1.55e+22 28 111 Moment Tensor: (dyne-cm) Component Value Mxx 4.36e+21 Mxy 2.34e+21 Mxz 9.63e+21 Myy -1.00e+22 Myz -8.10e+21 Mzz 5.67e+21 ############## -##################### --########################## --###########################- ---########## ##############---- ----########## T #############------ ----########### ############-------- -----########################----------- -----#######################------------ ------######################-------------- ------####################---------------- ------##################------------------ ------#################----------- ----- ------##############------------- P ---- -------###########--------------- ---- -------########----------------------- -------#####------------------------ ---------------------------------- ---####----------------------- #########------------------- #########------------- ############## Global CMT Convention Moment Tensor: R T P 5.67e+21 9.63e+21 8.10e+21 9.63e+21 4.36e+21 -2.34e+21 8.10e+21 -2.34e+21 -1.00e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20120308105742/index.html |
USGS/SLU Regional Moment Solution 12/03/08 10:57:44.07 Epicenter: 60.996 -150.950 MW 4.1 USGS/SLU REGIONAL MOMENT TENSOR Depth 26 No. of sta: 67 Moment Tensor; Scale 10**15 Nm Mrr= 0.91 Mtt= 0.56 Mpp=-1.46 Mrt= 0.90 Mrp= 0.45 Mtp=-0.04 Principal axes: T Val= 1.68 Plg=51 Azm=350 N -0.11 36 196 P -1.57 13 96 Best Double Couple:Mo=1.6*10**15 NP1:Strike=149 Dip=45 Slip= 34 NP2: 34 67 130 |
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: ML computed using the IASPEI formula for Horizontal components. Center: ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
Right: Residuals from new relation as a function of distance and azimuth.
Left: ML computed using the IASPEI formula for Vertical components (research). Center: ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
Right: Residuals from new relation 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 0.02 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 265 45 -90 3.51 0.2878 WVFGRD96 1.0 85 45 -90 3.57 0.3107 WVFGRD96 2.0 265 45 -90 3.67 0.3879 WVFGRD96 3.0 265 45 -85 3.76 0.4134 WVFGRD96 4.0 115 60 -35 3.78 0.3851 WVFGRD96 5.0 120 75 -20 3.80 0.3547 WVFGRD96 6.0 125 90 -10 3.80 0.3297 WVFGRD96 7.0 130 50 0 3.78 0.3289 WVFGRD96 8.0 135 40 5 3.83 0.3428 WVFGRD96 9.0 140 35 15 3.84 0.3723 WVFGRD96 10.0 140 30 10 3.85 0.4033 WVFGRD96 11.0 145 30 15 3.85 0.4335 WVFGRD96 12.0 145 30 20 3.87 0.4615 WVFGRD96 13.0 150 30 25 3.88 0.4883 WVFGRD96 14.0 150 30 25 3.90 0.5133 WVFGRD96 15.0 150 30 25 3.91 0.5366 WVFGRD96 16.0 155 30 30 3.92 0.5582 WVFGRD96 17.0 155 30 30 3.93 0.5782 WVFGRD96 18.0 155 30 30 3.94 0.5964 WVFGRD96 19.0 155 30 30 3.95 0.6130 WVFGRD96 20.0 155 30 30 3.96 0.6283 WVFGRD96 21.0 160 30 30 3.97 0.6410 WVFGRD96 22.0 160 30 30 3.98 0.6540 WVFGRD96 23.0 160 30 30 3.99 0.6654 WVFGRD96 24.0 160 30 30 4.00 0.6753 WVFGRD96 25.0 160 30 30 4.01 0.6839 WVFGRD96 26.0 160 30 30 4.02 0.6908 WVFGRD96 27.0 160 30 30 4.03 0.6959 WVFGRD96 28.0 160 30 30 4.04 0.6996 WVFGRD96 29.0 155 30 25 4.05 0.7017 WVFGRD96 30.0 155 30 25 4.06 0.7021 WVFGRD96 31.0 155 30 25 4.07 0.7009 WVFGRD96 32.0 155 30 25 4.08 0.6979 WVFGRD96 33.0 155 30 25 4.08 0.6937 WVFGRD96 34.0 155 30 25 4.09 0.6882 WVFGRD96 35.0 155 30 25 4.09 0.6815 WVFGRD96 36.0 150 35 25 4.11 0.6750 WVFGRD96 37.0 150 35 25 4.12 0.6683 WVFGRD96 38.0 150 40 25 4.13 0.6619 WVFGRD96 39.0 150 40 25 4.13 0.6550 WVFGRD96 40.0 155 25 25 4.24 0.6418 WVFGRD96 41.0 155 25 25 4.24 0.6291 WVFGRD96 42.0 150 30 20 4.25 0.6156 WVFGRD96 43.0 150 30 20 4.25 0.6029 WVFGRD96 44.0 150 30 20 4.26 0.5896 WVFGRD96 45.0 150 30 20 4.26 0.5760 WVFGRD96 46.0 150 30 20 4.26 0.5622 WVFGRD96 47.0 150 30 20 4.26 0.5480 WVFGRD96 48.0 145 35 15 4.27 0.5348 WVFGRD96 49.0 145 35 15 4.27 0.5214
The best solution is
WVFGRD96 30.0 155 30 25 4.06 0.7021
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 0.02 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 WUS.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 Model after 8 iterations 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 1.9000 3.4065 2.0089 2.2150 0.302E-02 0.679E-02 0.00 0.00 1.00 1.00 6.1000 5.5445 3.2953 2.6089 0.349E-02 0.784E-02 0.00 0.00 1.00 1.00 13.0000 6.2708 3.7396 2.7812 0.212E-02 0.476E-02 0.00 0.00 1.00 1.00 19.0000 6.4075 3.7680 2.8223 0.111E-02 0.249E-02 0.00 0.00 1.00 1.00 0.0000 7.9000 4.6200 3.2760 0.164E-10 0.370E-10 0.00 0.00 1.00 1.00