USGS/SLU Moment Tensor Solution ENS 2020/01/03 13:16:18:0 69.61 -144.71 7.9 4.0 Alaska Stations used: AK.COLD AK.FYU AK.H21K AK.I21K AK.I27K IM.IL31 TA.C26K TA.D23K TA.D27M TA.E19K TA.E22K TA.E23K TA.E24K TA.E25K TA.E28M TA.F21K TA.F28M TA.G23K TA.G24K TA.G26K TA.G31M TA.H27K TA.I28M TA.POKR TA.TOLK Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 7.50e+21 dyne-cm Mw = 3.85 Z = 10 km Plane Strike Dip Rake NP1 90 65 70 NP2 311 32 126 Principal Axes: Axis Value Plunge Azimuth T 7.50e+21 64 326 N 0.00e+00 18 99 P -7.50e+21 18 195 Moment Tensor: (dyne-cm) Component Value Mxx -5.40e+21 Mxy -2.32e+21 Mxz 4.53e+21 Myy -2.03e+14 Myz -1.08e+21 Mzz 5.40e+21 -------------- ---------------------- ---###########-------------- ####################---------- #########################--------- ############################-------- ###############################------- ############### ###############------- ############### T ################------ ################ #################------ #####################################----- -#####################################---# ----###################################### --------########################-----### -------------------------------------### ------------------------------------## -----------------------------------# ---------------------------------# ------------------------------ -------- ----------------- ----- P -------------- - ---------- Global CMT Convention Moment Tensor: R T P 5.40e+21 4.53e+21 1.08e+21 4.53e+21 -5.40e+21 2.32e+21 1.08e+21 2.32e+21 -2.03e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20200103131618/index.html |
STK = 90 DIP = 65 RAKE = 70 MW = 3.85 HS = 10.0
The NDK file is 20200103131618.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2020/01/03 13:16:18:0 69.61 -144.71 7.9 4.0 Alaska Stations used: AK.COLD AK.FYU AK.H21K AK.I21K AK.I27K IM.IL31 TA.C26K TA.D23K TA.D27M TA.E19K TA.E22K TA.E23K TA.E24K TA.E25K TA.E28M TA.F21K TA.F28M TA.G23K TA.G24K TA.G26K TA.G31M TA.H27K TA.I28M TA.POKR TA.TOLK Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 7.50e+21 dyne-cm Mw = 3.85 Z = 10 km Plane Strike Dip Rake NP1 90 65 70 NP2 311 32 126 Principal Axes: Axis Value Plunge Azimuth T 7.50e+21 64 326 N 0.00e+00 18 99 P -7.50e+21 18 195 Moment Tensor: (dyne-cm) Component Value Mxx -5.40e+21 Mxy -2.32e+21 Mxz 4.53e+21 Myy -2.03e+14 Myz -1.08e+21 Mzz 5.40e+21 -------------- ---------------------- ---###########-------------- ####################---------- #########################--------- ############################-------- ###############################------- ############### ###############------- ############### T ################------ ################ #################------ #####################################----- -#####################################---# ----###################################### --------########################-----### -------------------------------------### ------------------------------------## -----------------------------------# ---------------------------------# ------------------------------ -------- ----------------- ----- P -------------- - ---------- Global CMT Convention Moment Tensor: R T P 5.40e+21 4.53e+21 1.08e+21 4.53e+21 -5.40e+21 2.32e+21 1.08e+21 2.32e+21 -2.03e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20200103131618/index.html |
(a) mLg computed using the IASPEI formula; (b) mLg residuals ; the values used for the trimmed mean are indicated.
(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 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 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 95 40 75 3.52 0.2938 WVFGRD96 2.0 105 45 85 3.64 0.3539 WVFGRD96 3.0 265 80 70 3.73 0.3967 WVFGRD96 4.0 70 85 60 3.72 0.4724 WVFGRD96 5.0 75 80 60 3.73 0.5330 WVFGRD96 6.0 75 80 60 3.74 0.5752 WVFGRD96 7.0 80 75 60 3.75 0.6031 WVFGRD96 8.0 80 75 65 3.82 0.6297 WVFGRD96 9.0 90 65 75 3.84 0.6481 WVFGRD96 10.0 90 65 70 3.85 0.6575 WVFGRD96 11.0 90 65 70 3.85 0.6572 WVFGRD96 12.0 90 65 70 3.85 0.6507 WVFGRD96 13.0 90 65 70 3.86 0.6405 WVFGRD96 14.0 185 35 30 3.85 0.6346 WVFGRD96 15.0 185 35 30 3.86 0.6276 WVFGRD96 16.0 180 35 25 3.86 0.6200 WVFGRD96 17.0 180 35 25 3.87 0.6133 WVFGRD96 18.0 180 35 25 3.88 0.6070 WVFGRD96 19.0 180 35 25 3.89 0.5999 WVFGRD96 20.0 175 35 20 3.90 0.5923 WVFGRD96 21.0 175 35 20 3.91 0.5852 WVFGRD96 22.0 175 35 20 3.92 0.5775 WVFGRD96 23.0 170 35 15 3.93 0.5688 WVFGRD96 24.0 170 35 15 3.94 0.5597 WVFGRD96 25.0 170 35 10 3.94 0.5491 WVFGRD96 26.0 165 35 5 3.95 0.5396 WVFGRD96 27.0 165 35 5 3.96 0.5292 WVFGRD96 28.0 165 35 5 3.96 0.5190 WVFGRD96 29.0 160 35 -5 3.96 0.5104
The best solution is
WVFGRD96 10.0 90 65 70 3.85 0.6575
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 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 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: