USGS/SLU Moment Tensor Solution ENS 2017/06/20 16:03:35:0 62.76 -148.40 53.9 3.8 Alaska Stations used: AK.BWN AK.CUT AK.DHY AK.GHO AK.GLI AK.KNK AK.KTH AK.MCK AK.PWL AK.RC01 AK.RND AK.SAW AK.SCM AK.SCRK AK.TRF AT.PMR TA.N25K Filtering commands used: cut o DIST/3.5 -30 o DIST/3.5 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 7.24e+21 dyne-cm Mw = 3.84 Z = 64 km Plane Strike Dip Rake NP1 95 85 15 NP2 4 75 175 Principal Axes: Axis Value Plunge Azimuth T 7.24e+21 14 320 N 0.00e+00 74 113 P -7.24e+21 7 228 Moment Tensor: (dyne-cm) Component Value Mxx 8.87e+20 Mxy -6.89e+21 Mxz 1.89e+21 Myy -1.21e+21 Myz -4.47e+20 Mzz 3.26e+20 #########----- #############--------- # #############----------- ## T #############------------ #### ##############------------- ######################-------------- #######################--------------- ########################---------------- ########################---------------- #########################----------------- ----#####################----------------- -----------------########----------------- -------------------------################# -----------------------################# -----------------------################# ----------------------################ - ----------------################ P ----------------############### ----------------############# ---------------############# -----------########### ------######## Global CMT Convention Moment Tensor: R T P 3.26e+20 1.89e+21 4.47e+20 1.89e+21 8.87e+20 6.89e+21 4.47e+20 6.89e+21 -1.21e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170620160335/index.html |
STK = 95 DIP = 85 RAKE = 15 MW = 3.84 HS = 64.0
The NDK file is 20170620160335.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2017/06/20 16:03:35:0 62.76 -148.40 53.9 3.8 Alaska Stations used: AK.BWN AK.CUT AK.DHY AK.GHO AK.GLI AK.KNK AK.KTH AK.MCK AK.PWL AK.RC01 AK.RND AK.SAW AK.SCM AK.SCRK AK.TRF AT.PMR TA.N25K Filtering commands used: cut o DIST/3.5 -30 o DIST/3.5 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 7.24e+21 dyne-cm Mw = 3.84 Z = 64 km Plane Strike Dip Rake NP1 95 85 15 NP2 4 75 175 Principal Axes: Axis Value Plunge Azimuth T 7.24e+21 14 320 N 0.00e+00 74 113 P -7.24e+21 7 228 Moment Tensor: (dyne-cm) Component Value Mxx 8.87e+20 Mxy -6.89e+21 Mxz 1.89e+21 Myy -1.21e+21 Myz -4.47e+20 Mzz 3.26e+20 #########----- #############--------- # #############----------- ## T #############------------ #### ##############------------- ######################-------------- #######################--------------- ########################---------------- ########################---------------- #########################----------------- ----#####################----------------- -----------------########----------------- -------------------------################# -----------------------################# -----------------------################# ----------------------################ - ----------------################ P ----------------############### ----------------############# ---------------############# -----------########### ------######## Global CMT Convention Moment Tensor: R T P 3.26e+20 1.89e+21 4.47e+20 1.89e+21 8.87e+20 6.89e+21 4.47e+20 6.89e+21 -1.21e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170620160335/index.html |
Regional Moment Tensor (Mwr) Moment 7.568e+14 N-m Magnitude 3.9 Mwr Depth 60.0 km Percent DC 83 % Half Duration – Catalog US Data Source US2 Contributor US2 Nodal Planes Plane Strike Dip Rake NP1 1 75 -179 NP2 271 89 -15 Principal Axes Axis Value Plunge Azimuth T 7.877e+14 N-m 10 317 N -0.662e+14 N-m 75 87 P -7.215e+14 N-m 11 225 |
(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/3.5 -30 o DIST/3.5 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 2.0 125 45 -95 3.07 0.1983 WVFGRD96 4.0 180 70 20 3.06 0.2302 WVFGRD96 6.0 0 65 25 3.14 0.2683 WVFGRD96 8.0 0 60 25 3.23 0.3013 WVFGRD96 10.0 0 60 25 3.28 0.3234 WVFGRD96 12.0 0 65 20 3.32 0.3296 WVFGRD96 14.0 0 65 15 3.34 0.3256 WVFGRD96 16.0 265 65 25 3.38 0.3402 WVFGRD96 18.0 265 60 25 3.41 0.3594 WVFGRD96 20.0 265 65 25 3.44 0.3795 WVFGRD96 22.0 265 65 25 3.47 0.3976 WVFGRD96 24.0 265 65 25 3.49 0.4109 WVFGRD96 26.0 265 65 25 3.51 0.4185 WVFGRD96 28.0 85 80 -10 3.53 0.4312 WVFGRD96 30.0 90 75 15 3.55 0.4406 WVFGRD96 32.0 90 75 10 3.57 0.4575 WVFGRD96 34.0 90 75 10 3.59 0.4679 WVFGRD96 36.0 90 75 5 3.61 0.4734 WVFGRD96 38.0 95 75 10 3.65 0.4802 WVFGRD96 40.0 95 70 10 3.70 0.4899 WVFGRD96 42.0 95 75 15 3.72 0.4915 WVFGRD96 44.0 95 70 15 3.75 0.4971 WVFGRD96 46.0 95 75 15 3.76 0.5021 WVFGRD96 48.0 95 75 15 3.77 0.5066 WVFGRD96 50.0 95 80 15 3.78 0.5143 WVFGRD96 52.0 95 80 15 3.80 0.5217 WVFGRD96 54.0 95 80 15 3.80 0.5288 WVFGRD96 56.0 95 80 15 3.81 0.5328 WVFGRD96 58.0 95 85 15 3.82 0.5352 WVFGRD96 60.0 95 85 15 3.83 0.5387 WVFGRD96 62.0 275 90 -15 3.83 0.5373 WVFGRD96 64.0 95 85 15 3.84 0.5416 WVFGRD96 66.0 95 85 15 3.84 0.5403 WVFGRD96 68.0 90 90 15 3.83 0.5398 WVFGRD96 70.0 90 90 15 3.83 0.5406 WVFGRD96 72.0 90 90 15 3.84 0.5402 WVFGRD96 74.0 90 90 15 3.84 0.5392 WVFGRD96 76.0 270 90 -15 3.85 0.5397 WVFGRD96 78.0 90 90 15 3.85 0.5384 WVFGRD96 80.0 270 90 -15 3.86 0.5375 WVFGRD96 82.0 270 90 -15 3.86 0.5359 WVFGRD96 84.0 270 90 -10 3.86 0.5349 WVFGRD96 86.0 270 90 -10 3.87 0.5334 WVFGRD96 88.0 270 90 -10 3.87 0.5336 WVFGRD96 90.0 270 90 -10 3.87 0.5332 WVFGRD96 92.0 90 90 10 3.88 0.5323 WVFGRD96 94.0 90 90 10 3.88 0.5312 WVFGRD96 96.0 90 90 10 3.89 0.5301 WVFGRD96 98.0 90 90 10 3.89 0.5296
The best solution is
WVFGRD96 64.0 95 85 15 3.84 0.5416
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/3.5 -30 o DIST/3.5 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 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: