USGS/SLU Moment Tensor Solution ENS 2020/01/11 11:36:33:0 63.21 -151.46 10.9 4.1 Alaska Stations used: AK.BPAW AK.CCB AK.CUT AK.DHY AK.DIV AK.DOT AK.EYAK AK.GHO AK.GLB AK.GLI AK.HDA AK.HIN AK.I23K AK.J20K AK.K24K AK.KNK AK.KTH AK.L18K AK.L19K AK.M20K AK.MCK AK.N18K AK.N19K AK.O18K AK.PAX AK.PPLA AK.PWL AK.RC01 AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.SLK AK.SSN AK.SWD AK.TRF AK.WRH AT.PMR AV.ILSW IM.IL31 IU.COLA TA.G23K TA.H18K TA.M22K TA.M24K TA.P19K TA.POKR Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 6.76e+21 dyne-cm Mw = 3.82 Z = 14 km Plane Strike Dip Rake NP1 60 55 120 NP2 195 45 55 Principal Axes: Axis Value Plunge Azimuth T 6.76e+21 65 28 N 0.00e+00 24 221 P -6.76e+21 5 129 Moment Tensor: (dyne-cm) Component Value Mxx -1.74e+21 Mxy 3.76e+21 Mxz 2.65e+21 Myy -3.80e+21 Myz 7.10e+20 Mzz 5.54e+21 ----------#### ----------############ -----------################# ----------#################### ----------######################## ----------########################## ----------###########################- ----------########### #############--- ----------########### T ############---- ----------############ ###########------ ----------#########################------- ---------#########################-------- ---------#######################---------- --------#####################----------- --------##################-------------- --------##############---------------- -------##########--------------- - ######------------------------- P #####------------------------ #####----------------------- ###------------------- #------------- Global CMT Convention Moment Tensor: R T P 5.54e+21 2.65e+21 -7.10e+20 2.65e+21 -1.74e+21 -3.76e+21 -7.10e+20 -3.76e+21 -3.80e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20200111113633/index.html |
STK = 195 DIP = 45 RAKE = 55 MW = 3.82 HS = 14.0
The NDK file is 20200111113633.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2020/01/11 11:36:33:0 63.21 -151.46 10.9 4.1 Alaska Stations used: AK.BPAW AK.CCB AK.CUT AK.DHY AK.DIV AK.DOT AK.EYAK AK.GHO AK.GLB AK.GLI AK.HDA AK.HIN AK.I23K AK.J20K AK.K24K AK.KNK AK.KTH AK.L18K AK.L19K AK.M20K AK.MCK AK.N18K AK.N19K AK.O18K AK.PAX AK.PPLA AK.PWL AK.RC01 AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.SLK AK.SSN AK.SWD AK.TRF AK.WRH AT.PMR AV.ILSW IM.IL31 IU.COLA TA.G23K TA.H18K TA.M22K TA.M24K TA.P19K TA.POKR Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 6.76e+21 dyne-cm Mw = 3.82 Z = 14 km Plane Strike Dip Rake NP1 60 55 120 NP2 195 45 55 Principal Axes: Axis Value Plunge Azimuth T 6.76e+21 65 28 N 0.00e+00 24 221 P -6.76e+21 5 129 Moment Tensor: (dyne-cm) Component Value Mxx -1.74e+21 Mxy 3.76e+21 Mxz 2.65e+21 Myy -3.80e+21 Myz 7.10e+20 Mzz 5.54e+21 ----------#### ----------############ -----------################# ----------#################### ----------######################## ----------########################## ----------###########################- ----------########### #############--- ----------########### T ############---- ----------############ ###########------ ----------#########################------- ---------#########################-------- ---------#######################---------- --------#####################----------- --------##################-------------- --------##############---------------- -------##########--------------- - ######------------------------- P #####------------------------ #####----------------------- ###------------------- #------------- Global CMT Convention Moment Tensor: R T P 5.54e+21 2.65e+21 -7.10e+20 2.65e+21 -1.74e+21 -3.76e+21 -7.10e+20 -3.76e+21 -3.80e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20200111113633/index.html |
(a) ML computed using the IASPEI formula for Horizontal components; (b) 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.
(a) ML computed using the IASPEI formula for Vertical components (research); (b) 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.
The focal mechanism was determined using broadband seismic waveforms. The location of the event and the and stations used for 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 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:
cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 120 45 -90 3.37 0.3181 WVFGRD96 2.0 295 45 -90 3.55 0.4856 WVFGRD96 3.0 170 60 -25 3.56 0.4195 WVFGRD96 4.0 180 35 0 3.65 0.4493 WVFGRD96 5.0 185 30 10 3.69 0.5370 WVFGRD96 6.0 190 30 10 3.70 0.6025 WVFGRD96 7.0 195 35 25 3.71 0.6408 WVFGRD96 8.0 190 25 5 3.75 0.6532 WVFGRD96 9.0 200 35 45 3.79 0.6724 WVFGRD96 10.0 200 40 55 3.81 0.7018 WVFGRD96 11.0 200 40 60 3.81 0.7240 WVFGRD96 12.0 195 45 55 3.81 0.7381 WVFGRD96 13.0 195 45 55 3.82 0.7461 WVFGRD96 14.0 195 45 55 3.82 0.7491 WVFGRD96 15.0 195 45 55 3.83 0.7488 WVFGRD96 16.0 190 50 50 3.83 0.7467 WVFGRD96 17.0 190 50 50 3.84 0.7429 WVFGRD96 18.0 190 50 50 3.84 0.7372 WVFGRD96 19.0 190 50 50 3.85 0.7296 WVFGRD96 20.0 190 50 50 3.86 0.7204 WVFGRD96 21.0 190 50 50 3.87 0.7084 WVFGRD96 22.0 190 50 50 3.88 0.6961 WVFGRD96 23.0 190 50 50 3.89 0.6817 WVFGRD96 24.0 190 50 50 3.90 0.6654 WVFGRD96 25.0 190 50 50 3.90 0.6477 WVFGRD96 26.0 190 50 50 3.91 0.6290 WVFGRD96 27.0 190 50 50 3.91 0.6096 WVFGRD96 28.0 190 50 45 3.92 0.5899 WVFGRD96 29.0 190 50 45 3.92 0.5696
The best solution is
WVFGRD96 14.0 195 45 55 3.82 0.7491
The mechanism correspond 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 and because the velocity model used in the predictions may not be perfect. 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
cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2
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Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to thewavefroms. 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.
Thanks also to the many seismic network operators whose dedication make this effort possible: University of Nevada Reno, University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureau of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Oklahoma Geological Survey, TexNet, the Iris stations, the Transportable Array of EarthScope and other networks.
The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
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
Here we tabulate the reasons for not using certain digital data sets
The following stations did not have a valid response files: