USGS/SLU Moment Tensor Solution ENS 2022/10/18 10:24:26:0 61.39 -149.86 14.0 3.5 Alaska Stations used: AK.FID AK.FIRE AK.GHO AK.GLI AK.KNK AK.L22K AK.PWL AK.RC01 AK.SAW AK.SSN AT.PMR AV.RED AV.SPCP 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 = 40 km Plane Strike Dip Rake NP1 200 75 -60 NP2 314 33 -152 Principal Axes: Axis Value Plunge Azimuth T 6.76e+21 24 267 N 0.00e+00 29 11 P -6.76e+21 51 144 Moment Tensor: (dyne-cm) Component Value Mxx -1.76e+21 Mxy 1.56e+21 Mxz 2.56e+21 Myy 4.68e+21 Myz -4.47e+21 Mzz -2.93e+21 -------------- ----------------###### --############----########## #################--########### ##################------########## ##################----------######## ##################------------######## ##################---------------####### ##################----------------###### ##################------------------###### #### ##########--------------------##### #### T ##########--------------------##### #### #########----------------------#### ###############----------------------### ##############---------- ----------### #############---------- P ----------## ###########----------- ---------## ##########-----------------------# ########---------------------- #######--------------------- ####------------------ -------------- Global CMT Convention Moment Tensor: R T P -2.93e+21 2.56e+21 4.47e+21 2.56e+21 -1.76e+21 -1.56e+21 4.47e+21 -1.56e+21 4.68e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20221018102426/index.html |
STK = 200 DIP = 75 RAKE = -60 MW = 3.82 HS = 40.0
The NDK file is 20221018102426.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2022/10/18 10:24:26:0 61.39 -149.86 14.0 3.5 Alaska Stations used: AK.FID AK.FIRE AK.GHO AK.GLI AK.KNK AK.L22K AK.PWL AK.RC01 AK.SAW AK.SSN AT.PMR AV.RED AV.SPCP 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 = 40 km Plane Strike Dip Rake NP1 200 75 -60 NP2 314 33 -152 Principal Axes: Axis Value Plunge Azimuth T 6.76e+21 24 267 N 0.00e+00 29 11 P -6.76e+21 51 144 Moment Tensor: (dyne-cm) Component Value Mxx -1.76e+21 Mxy 1.56e+21 Mxz 2.56e+21 Myy 4.68e+21 Myz -4.47e+21 Mzz -2.93e+21 -------------- ----------------###### --############----########## #################--########### ##################------########## ##################----------######## ##################------------######## ##################---------------####### ##################----------------###### ##################------------------###### #### ##########--------------------##### #### T ##########--------------------##### #### #########----------------------#### ###############----------------------### ##############---------- ----------### #############---------- P ----------## ###########----------- ---------## ##########-----------------------# ########---------------------- #######--------------------- ####------------------ -------------- Global CMT Convention Moment Tensor: R T P -2.93e+21 2.56e+21 4.47e+21 2.56e+21 -1.76e+21 -1.56e+21 4.47e+21 -1.56e+21 4.68e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20221018102426/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 are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 2.0 40 70 -20 3.19 0.3414 WVFGRD96 4.0 40 80 -15 3.30 0.4150 WVFGRD96 6.0 35 75 25 3.39 0.4447 WVFGRD96 8.0 45 60 35 3.46 0.4736 WVFGRD96 10.0 45 65 25 3.46 0.4928 WVFGRD96 12.0 45 70 25 3.48 0.5059 WVFGRD96 14.0 45 70 25 3.50 0.5157 WVFGRD96 16.0 45 70 25 3.52 0.5220 WVFGRD96 18.0 45 70 25 3.54 0.5284 WVFGRD96 20.0 40 85 40 3.56 0.5395 WVFGRD96 22.0 40 85 40 3.58 0.5532 WVFGRD96 24.0 40 85 40 3.60 0.5650 WVFGRD96 26.0 210 75 -45 3.62 0.5777 WVFGRD96 28.0 210 75 -45 3.64 0.5973 WVFGRD96 30.0 210 75 -50 3.65 0.6113 WVFGRD96 32.0 210 80 -50 3.67 0.6286 WVFGRD96 34.0 205 75 -50 3.68 0.6419 WVFGRD96 36.0 205 75 -50 3.70 0.6504 WVFGRD96 38.0 200 75 -50 3.72 0.6498 WVFGRD96 40.0 200 75 -60 3.82 0.6579 WVFGRD96 42.0 195 70 -60 3.83 0.6556 WVFGRD96 44.0 195 70 -60 3.84 0.6515 WVFGRD96 46.0 195 70 -60 3.85 0.6455 WVFGRD96 48.0 195 70 -60 3.86 0.6399 WVFGRD96 50.0 190 70 -60 3.88 0.6330 WVFGRD96 52.0 195 75 -55 3.89 0.6275 WVFGRD96 54.0 195 75 -55 3.89 0.6203 WVFGRD96 56.0 190 75 -55 3.92 0.6136 WVFGRD96 58.0 190 75 -55 3.92 0.6071 WVFGRD96 60.0 190 75 -55 3.93 0.5996 WVFGRD96 62.0 190 75 -55 3.93 0.5925 WVFGRD96 64.0 190 75 -55 3.94 0.5850 WVFGRD96 66.0 190 75 -55 3.94 0.5771 WVFGRD96 68.0 190 75 -55 3.95 0.5689 WVFGRD96 70.0 190 75 -55 3.95 0.5606 WVFGRD96 72.0 30 70 40 3.98 0.5474 WVFGRD96 74.0 30 70 40 3.99 0.5493 WVFGRD96 76.0 30 70 40 3.99 0.5511 WVFGRD96 78.0 30 70 40 4.00 0.5527 WVFGRD96 80.0 30 70 40 4.00 0.5530 WVFGRD96 82.0 30 70 40 4.01 0.5499 WVFGRD96 84.0 30 70 40 4.01 0.5452 WVFGRD96 86.0 30 70 40 4.01 0.5403 WVFGRD96 88.0 30 70 35 4.02 0.5375 WVFGRD96 90.0 30 70 35 4.03 0.5339 WVFGRD96 92.0 30 70 35 4.03 0.5267 WVFGRD96 94.0 25 75 30 4.04 0.5147 WVFGRD96 96.0 25 80 30 4.03 0.5036 WVFGRD96 98.0 30 75 25 4.03 0.4925
The best solution is
WVFGRD96 40.0 200 75 -60 3.82 0.6579
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: