The ANSS event ID is ak018fhjd3wg and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak018fhjd3wg/executive.
2018/12/03 12:18:58 61.246 -149.972 44.5 2.9 Alaska
USGS/SLU Moment Tensor Solution ENS 2018/12/03 12:18:58:0 61.25 -149.97 44.5 2.9 Alaska Stations used: AK.GHO AK.KNK AK.RC01 AK.SAW AK.SKN AK.SSN TA.M20K TA.M22K Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.10e+22 dyne-cm Mw = 3.96 Z = 50 km Plane Strike Dip Rake NP1 175 50 -85 NP2 347 40 -96 Principal Axes: Axis Value Plunge Azimuth T 1.10e+22 5 261 N 0.00e+00 4 352 P -1.10e+22 84 120 Moment Tensor: (dyne-cm) Component Value Mxx 2.09e+20 Mxy 1.65e+21 Mxz 4.47e+20 Myy 1.05e+22 Myz -1.94e+21 Mzz -1.08e+22 ####-######### ######-------######### ########-----------######### ########-------------######### #########----------------######### #########------------------######### ##########-------------------######### ##########---------------------######### ##########----------------------######## ###########----------------------######### ###########---------- ---------######### ########---------- P ----------######## T ########---------- ----------######## #########----------------------####### ###########---------------------######## ###########--------------------####### ##########--------------------###### ##########------------------###### #########----------------##### ##########-------------##### ########-----------### #######------# Global CMT Convention Moment Tensor: R T P -1.08e+22 4.47e+20 1.94e+21 4.47e+20 2.09e+20 -1.65e+21 1.94e+21 -1.65e+21 1.05e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20181203121858/index.html |
STK = 175 DIP = 50 RAKE = -85 MW = 3.96 HS = 50.0
The NDK file is 20181203121858.ndk The waveform inversion is preferred.
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 -40 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 185 45 95 3.10 0.1741 WVFGRD96 2.0 10 45 90 3.27 0.2306 WVFGRD96 3.0 340 25 65 3.33 0.2025 WVFGRD96 4.0 5 85 65 3.37 0.2583 WVFGRD96 5.0 15 80 75 3.37 0.3020 WVFGRD96 6.0 160 15 50 3.37 0.3348 WVFGRD96 7.0 145 20 35 3.38 0.3589 WVFGRD96 8.0 170 15 60 3.47 0.3762 WVFGRD96 9.0 155 20 45 3.48 0.3909 WVFGRD96 10.0 165 20 55 3.49 0.4001 WVFGRD96 11.0 165 25 55 3.50 0.4067 WVFGRD96 12.0 175 25 65 3.52 0.4122 WVFGRD96 13.0 175 25 65 3.53 0.4144 WVFGRD96 14.0 170 25 60 3.54 0.4139 WVFGRD96 15.0 170 25 60 3.55 0.4110 WVFGRD96 16.0 170 25 60 3.56 0.4063 WVFGRD96 17.0 170 25 60 3.57 0.4002 WVFGRD96 18.0 170 20 60 3.57 0.3934 WVFGRD96 19.0 170 20 60 3.58 0.3861 WVFGRD96 20.0 165 20 55 3.59 0.3772 WVFGRD96 21.0 10 80 45 3.68 0.3718 WVFGRD96 22.0 10 80 45 3.69 0.3670 WVFGRD96 23.0 25 85 65 3.65 0.3615 WVFGRD96 24.0 200 90 -65 3.65 0.3575 WVFGRD96 25.0 25 85 65 3.67 0.3564 WVFGRD96 26.0 200 90 -65 3.68 0.3534 WVFGRD96 27.0 25 85 60 3.69 0.3521 WVFGRD96 28.0 200 75 -65 3.69 0.3560 WVFGRD96 29.0 205 75 -65 3.69 0.3625 WVFGRD96 30.0 200 75 -65 3.71 0.3685 WVFGRD96 31.0 200 70 -65 3.72 0.3788 WVFGRD96 32.0 5 30 -85 3.74 0.3927 WVFGRD96 33.0 180 60 -95 3.75 0.4129 WVFGRD96 34.0 5 30 -85 3.76 0.4329 WVFGRD96 35.0 5 30 -85 3.76 0.4473 WVFGRD96 36.0 185 50 -80 3.77 0.4671 WVFGRD96 37.0 185 50 -80 3.77 0.4831 WVFGRD96 38.0 185 50 -80 3.78 0.4987 WVFGRD96 39.0 185 50 -80 3.80 0.5109 WVFGRD96 40.0 180 50 -80 3.88 0.5142 WVFGRD96 41.0 180 50 -80 3.90 0.5225 WVFGRD96 42.0 180 50 -80 3.91 0.5303 WVFGRD96 43.0 180 50 -80 3.92 0.5387 WVFGRD96 44.0 180 50 -80 3.93 0.5455 WVFGRD96 45.0 180 50 -80 3.93 0.5528 WVFGRD96 46.0 180 50 -80 3.94 0.5563 WVFGRD96 47.0 180 50 -80 3.94 0.5612 WVFGRD96 48.0 175 50 -80 3.96 0.5632 WVFGRD96 49.0 175 50 -85 3.96 0.5657 WVFGRD96 50.0 175 50 -85 3.96 0.5665 WVFGRD96 51.0 175 50 -85 3.96 0.5657 WVFGRD96 52.0 345 40 -100 3.97 0.5663 WVFGRD96 53.0 175 50 -85 3.97 0.5645 WVFGRD96 54.0 175 50 -85 3.97 0.5658 WVFGRD96 55.0 350 40 -95 3.97 0.5646 WVFGRD96 56.0 170 50 -95 3.98 0.5642 WVFGRD96 57.0 0 40 -80 3.99 0.5639 WVFGRD96 58.0 0 40 -80 3.99 0.5627 WVFGRD96 59.0 5 40 -75 4.00 0.5634
The best solution is
WVFGRD96 50.0 175 50 -85 3.96 0.5665
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 -40 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 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