The ANSS event ID is ak019i8au86 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak019i8au86/executive.
2019/01/11 02:33:38 61.471 -149.899 49.8 4.6 Alaska
USGS/SLU Moment Tensor Solution ENS 2019/01/11 02:33:38:0 61.47 -149.90 49.8 4.6 Alaska Stations used: AK.BRLK AK.CAST AK.CUT AK.FIRE AK.GHO AK.KNK AK.RC01 AK.SAW AK.SKN AK.SLK AT.PMR AV.STLK TA.M22K TA.O22K Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 7.85e+22 dyne-cm Mw = 4.53 Z = 58 km Plane Strike Dip Rake NP1 150 70 -70 NP2 283 28 -133 Principal Axes: Axis Value Plunge Azimuth T 7.85e+22 22 225 N 0.00e+00 19 323 P -7.85e+22 60 89 Moment Tensor: (dyne-cm) Component Value Mxx 3.37e+22 Mxy 3.32e+22 Mxz -2.03e+22 Myy 1.37e+22 Myz -5.35e+22 Mzz -4.74e+22 ############## -##################### ----######################## ---------------------######### ----###--------------------####### --######-----------------------##### -#########------------------------#### -##########-------------------------#### ############-------------------------### ##############------------- ---------### ###############------------ P ----------## ################----------- -----------# #################------------------------# #################----------------------- ##################---------------------- ##################-------------------- ##### ###########----------------- #### T #############-------------- ## ##############----------- #####################------- #####################- ############## Global CMT Convention Moment Tensor: R T P -4.74e+22 -2.03e+22 5.35e+22 -2.03e+22 3.37e+22 -3.32e+22 5.35e+22 -3.32e+22 1.37e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20190111023338/index.html |
STK = 150 DIP = 70 RAKE = -70 MW = 4.53 HS = 58.0
The NDK file is 20190111023338.ndk The waveform inversion is preferred.
The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
USGS/SLU Moment Tensor Solution ENS 2019/01/11 02:33:38:0 61.47 -149.90 49.8 4.6 Alaska Stations used: AK.BRLK AK.CAST AK.CUT AK.FIRE AK.GHO AK.KNK AK.RC01 AK.SAW AK.SKN AK.SLK AT.PMR AV.STLK TA.M22K TA.O22K Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 7.85e+22 dyne-cm Mw = 4.53 Z = 58 km Plane Strike Dip Rake NP1 150 70 -70 NP2 283 28 -133 Principal Axes: Axis Value Plunge Azimuth T 7.85e+22 22 225 N 0.00e+00 19 323 P -7.85e+22 60 89 Moment Tensor: (dyne-cm) Component Value Mxx 3.37e+22 Mxy 3.32e+22 Mxz -2.03e+22 Myy 1.37e+22 Myz -5.35e+22 Mzz -4.74e+22 ############## -##################### ----######################## ---------------------######### ----###--------------------####### --######-----------------------##### -#########------------------------#### -##########-------------------------#### ############-------------------------### ##############------------- ---------### ###############------------ P ----------## ################----------- -----------# #################------------------------# #################----------------------- ##################---------------------- ##################-------------------- ##### ###########----------------- #### T #############-------------- ## ##############----------- #####################------- #####################- ############## Global CMT Convention Moment Tensor: R T P -4.74e+22 -2.03e+22 5.35e+22 -2.03e+22 3.37e+22 -3.32e+22 5.35e+22 -3.32e+22 1.37e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20190111023338/index.html |
Regional Moment Tensor (Mwr) Moment 5.214e+15 N-m Magnitude 4.41 Mwr Depth 49.0 km Percent DC 95% Half Duration - Catalog US Data Source US 3 Contributor US 3 Nodal Planes Plane Strike Dip Rake NP1 304 16 -124 NP2 159 76 -81 Principal Axes Axis Value Plunge Azimuth T 5.284e+15 N-m 31 241 N -0.144e+15 N-m 9 337 P -5.140e+15 N-m 58 81° |
Given the availability of digital waveforms for determination of the moment tensor, this section documents the added processing leading to mLg, if appropriate to the region, and ML by application of the respective IASPEI formulae. As a research study, the linear distance term of the IASPEI formula for ML is adjusted to remove a linear distance trend in residuals to give a regionally defined ML. The defined ML uses horizontal component recordings, but the same procedure is applied to the vertical components since there may be some interest in vertical component ground motions. Residual plots versus distance may indicate interesting features of ground motion scaling in some distance ranges. A residual plot of the regionalized magnitude is given as a function of distance and azimuth, since data sets may transcend different wave propagation provinces.
Left: ML computed using the IASPEI formula for Horizontal components. Center: 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.
Right: Residuals from new relation as a function of distance and azimuth.
Left: ML computed using the IASPEI formula for Vertical components (research). Center: 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.
Right: Residuals from new relation as a function of distance and azimuth.
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The focal mechanism was determined using broadband seismic waveforms. The location of the event (star) and the stations used for (red) 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's 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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 45 85 -5 3.67 0.1947 WVFGRD96 2.0 310 40 90 3.80 0.2410 WVFGRD96 3.0 140 70 30 3.89 0.2640 WVFGRD96 4.0 135 80 20 3.93 0.2926 WVFGRD96 5.0 135 80 15 3.97 0.3138 WVFGRD96 6.0 315 85 -25 3.99 0.3310 WVFGRD96 7.0 315 85 -20 4.02 0.3579 WVFGRD96 8.0 315 85 -25 4.07 0.3855 WVFGRD96 9.0 315 85 -20 4.10 0.4027 WVFGRD96 10.0 315 85 -20 4.12 0.4162 WVFGRD96 11.0 315 85 -20 4.13 0.4236 WVFGRD96 12.0 315 85 -20 4.14 0.4271 WVFGRD96 13.0 315 80 -20 4.15 0.4290 WVFGRD96 14.0 315 80 -20 4.16 0.4296 WVFGRD96 15.0 135 90 20 4.17 0.4289 WVFGRD96 16.0 135 90 20 4.18 0.4295 WVFGRD96 17.0 135 90 20 4.19 0.4280 WVFGRD96 18.0 135 75 0 4.22 0.4302 WVFGRD96 19.0 135 75 5 4.23 0.4322 WVFGRD96 20.0 135 75 5 4.24 0.4340 WVFGRD96 21.0 135 70 0 4.24 0.4338 WVFGRD96 22.0 140 65 5 4.23 0.4349 WVFGRD96 23.0 140 65 5 4.24 0.4368 WVFGRD96 24.0 140 60 5 4.25 0.4381 WVFGRD96 25.0 140 60 5 4.26 0.4397 WVFGRD96 26.0 140 60 5 4.27 0.4411 WVFGRD96 27.0 40 60 -10 4.27 0.4410 WVFGRD96 28.0 40 60 -10 4.28 0.4421 WVFGRD96 29.0 40 30 10 4.26 0.4466 WVFGRD96 30.0 35 30 5 4.27 0.4518 WVFGRD96 31.0 30 25 -5 4.27 0.4581 WVFGRD96 32.0 30 30 -5 4.29 0.4644 WVFGRD96 33.0 25 25 -15 4.29 0.4713 WVFGRD96 34.0 25 25 -15 4.29 0.4767 WVFGRD96 35.0 150 80 -80 4.27 0.4830 WVFGRD96 36.0 150 80 -80 4.28 0.4958 WVFGRD96 37.0 150 75 -75 4.29 0.5088 WVFGRD96 38.0 150 75 -75 4.29 0.5235 WVFGRD96 39.0 150 75 -70 4.30 0.5348 WVFGRD96 40.0 150 75 -80 4.43 0.5349 WVFGRD96 41.0 150 75 -80 4.44 0.5404 WVFGRD96 42.0 150 75 -80 4.44 0.5444 WVFGRD96 43.0 150 75 -80 4.45 0.5510 WVFGRD96 44.0 150 75 -80 4.46 0.5555 WVFGRD96 45.0 150 75 -80 4.46 0.5610 WVFGRD96 46.0 150 75 -75 4.47 0.5658 WVFGRD96 47.0 150 75 -80 4.48 0.5697 WVFGRD96 48.0 150 75 -75 4.48 0.5744 WVFGRD96 49.0 150 75 -75 4.49 0.5786 WVFGRD96 50.0 150 70 -75 4.49 0.5810 WVFGRD96 51.0 150 70 -75 4.50 0.5849 WVFGRD96 52.0 150 70 -75 4.50 0.5894 WVFGRD96 53.0 150 70 -75 4.51 0.5907 WVFGRD96 54.0 150 70 -75 4.52 0.5937 WVFGRD96 55.0 150 70 -75 4.52 0.5952 WVFGRD96 56.0 150 70 -75 4.52 0.5957 WVFGRD96 57.0 150 70 -75 4.53 0.5962 WVFGRD96 58.0 150 70 -70 4.53 0.5964 WVFGRD96 59.0 150 70 -70 4.54 0.5962 WVFGRD96 60.0 150 70 -70 4.54 0.5934 WVFGRD96 61.0 150 70 -70 4.54 0.5938 WVFGRD96 62.0 150 70 -70 4.55 0.5917 WVFGRD96 63.0 150 70 -70 4.55 0.5894 WVFGRD96 64.0 150 70 -70 4.55 0.5864 WVFGRD96 65.0 130 65 -55 4.59 0.5862 WVFGRD96 66.0 130 65 -55 4.60 0.5846 WVFGRD96 67.0 130 65 -55 4.60 0.5824 WVFGRD96 68.0 130 65 -55 4.60 0.5802 WVFGRD96 69.0 130 65 -55 4.61 0.5780
The best solution is
WVFGRD96 58.0 150 70 -70 4.53 0.5964
The mechanism corresponding 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, the velocity model used in the predictions may not be perfect and the epicentral parameters may be be off. 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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3
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Figure 3. Waveform comparison for selected depth. Red: observed; Blue - predicted. The time shift with respect to the model prediction is indicated. The percent of fit is also indicated. The time scale is relative to the first trace sample. |
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Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to the waveforms. 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.
The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows (The format is in the model96 format of Computer Programs in Seismology).
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