USGS/SLU Moment Tensor Solution ENS 2017/05/21 19:33:38:0 59.76 -136.51 5.0 4.3 BC, Canada Stations used: AK.BAGL AK.BAL AK.BARN AK.BCP AK.BESE AK.CTG AK.GLB AK.JIS AK.KIAG AK.LOGN AK.MCAR AK.PAX AK.PIN AK.PNL AK.PTPK AK.SAMH AK.TABL AK.VRDI AT.CRAG AT.SIT AT.SKAG CN.DAWY CN.HYT CN.YUK2 CN.YUK3 CN.YUK4 CN.YUK5 CN.YUK6 CN.YUK7 CN.YUK8 NY.MAYO TA.K27K TA.K29M TA.L27K TA.L29M TA.M26K TA.M27K TA.M29M TA.M30M TA.M31M TA.N30M TA.N31M TA.N32M TA.O28M TA.O29M TA.O30N TA.P29M TA.P30M TA.P32M TA.P33M TA.Q32M TA.R32K TA.R33M TA.S31K TA.S32K TA.S34M TA.T33K TA.T35M TA.U33K TA.U35K TA.V35K US.WRAK Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 9.23e+21 dyne-cm Mw = 3.91 Z = 17 km Plane Strike Dip Rake NP1 26 78 144 NP2 125 55 15 Principal Axes: Axis Value Plunge Azimuth T 9.23e+21 34 340 N 0.00e+00 52 190 P -9.23e+21 15 80 Moment Tensor: (dyne-cm) Component Value Mxx 5.35e+21 Mxy -3.55e+21 Mxz 3.60e+21 Myy -7.60e+21 Myz -3.72e+21 Mzz 2.24e+21 ############## ####################-- #######################----- ######### ###########------- ########### T ###########--------- -########### ##########----------- --########################------------ ----######################-------------- -----#####################---------- - -------###################----------- P -- --------#################------------ -- ---------###############------------------ -----------############------------------- ------------#########------------------- --------------######-------------------- ----------------##-------------------- ----------------##------------------ --------------########------------ ----------#################### --------#################### ---################### ############## Global CMT Convention Moment Tensor: R T P 2.24e+21 3.60e+21 3.72e+21 3.60e+21 5.35e+21 3.55e+21 3.72e+21 3.55e+21 -7.60e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170521193338/index.html |
STK = 125 DIP = 55 RAKE = 15 MW = 3.91 HS = 17.0
The NDK file is 20170521193338.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2017/05/21 19:33:38:0 59.76 -136.51 5.0 4.3 BC, Canada Stations used: AK.BAGL AK.BAL AK.BARN AK.BCP AK.BESE AK.CTG AK.GLB AK.JIS AK.KIAG AK.LOGN AK.MCAR AK.PAX AK.PIN AK.PNL AK.PTPK AK.SAMH AK.TABL AK.VRDI AT.CRAG AT.SIT AT.SKAG CN.DAWY CN.HYT CN.YUK2 CN.YUK3 CN.YUK4 CN.YUK5 CN.YUK6 CN.YUK7 CN.YUK8 NY.MAYO TA.K27K TA.K29M TA.L27K TA.L29M TA.M26K TA.M27K TA.M29M TA.M30M TA.M31M TA.N30M TA.N31M TA.N32M TA.O28M TA.O29M TA.O30N TA.P29M TA.P30M TA.P32M TA.P33M TA.Q32M TA.R32K TA.R33M TA.S31K TA.S32K TA.S34M TA.T33K TA.T35M TA.U33K TA.U35K TA.V35K US.WRAK Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 9.23e+21 dyne-cm Mw = 3.91 Z = 17 km Plane Strike Dip Rake NP1 26 78 144 NP2 125 55 15 Principal Axes: Axis Value Plunge Azimuth T 9.23e+21 34 340 N 0.00e+00 52 190 P -9.23e+21 15 80 Moment Tensor: (dyne-cm) Component Value Mxx 5.35e+21 Mxy -3.55e+21 Mxz 3.60e+21 Myy -7.60e+21 Myz -3.72e+21 Mzz 2.24e+21 ############## ####################-- #######################----- ######### ###########------- ########### T ###########--------- -########### ##########----------- --########################------------ ----######################-------------- -----#####################---------- - -------###################----------- P -- --------#################------------ -- ---------###############------------------ -----------############------------------- ------------#########------------------- --------------######-------------------- ----------------##-------------------- ----------------##------------------ --------------########------------ ----------#################### --------#################### ---################### ############## Global CMT Convention Moment Tensor: R T P 2.24e+21 3.60e+21 3.72e+21 3.60e+21 5.35e+21 3.55e+21 3.72e+21 3.55e+21 -7.60e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170521193338/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 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 65 45 90 3.56 0.3336 WVFGRD96 2.0 70 45 95 3.66 0.3979 WVFGRD96 3.0 225 55 65 3.71 0.3667 WVFGRD96 4.0 25 90 -55 3.72 0.3850 WVFGRD96 5.0 30 90 -55 3.73 0.4279 WVFGRD96 6.0 30 90 -50 3.74 0.4613 WVFGRD96 7.0 25 85 -45 3.75 0.4849 WVFGRD96 8.0 30 90 -55 3.81 0.4990 WVFGRD96 9.0 25 85 -50 3.81 0.5158 WVFGRD96 10.0 125 45 15 3.83 0.5338 WVFGRD96 11.0 125 50 20 3.85 0.5564 WVFGRD96 12.0 125 50 20 3.86 0.5749 WVFGRD96 13.0 125 50 15 3.87 0.5884 WVFGRD96 14.0 125 50 15 3.88 0.5976 WVFGRD96 15.0 125 55 20 3.90 0.6033 WVFGRD96 16.0 125 55 20 3.91 0.6063 WVFGRD96 17.0 125 55 15 3.91 0.6068 WVFGRD96 18.0 125 55 15 3.92 0.6045 WVFGRD96 19.0 125 55 15 3.93 0.5999 WVFGRD96 20.0 125 55 15 3.94 0.5938 WVFGRD96 21.0 125 55 15 3.95 0.5850 WVFGRD96 22.0 125 55 15 3.96 0.5753 WVFGRD96 23.0 125 55 15 3.96 0.5648 WVFGRD96 24.0 125 50 10 3.96 0.5536 WVFGRD96 25.0 125 50 5 3.97 0.5431 WVFGRD96 26.0 120 50 -5 3.97 0.5322 WVFGRD96 27.0 120 50 -5 3.98 0.5219 WVFGRD96 28.0 115 50 -10 3.98 0.5121 WVFGRD96 29.0 115 50 -10 3.99 0.5027
The best solution is
WVFGRD96 17.0 125 55 15 3.91 0.6068
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 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3
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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 Bureas of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Iris stations and the Transportable Array of EarthScope.
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: