The ANSS event ID is ak020cwv4p5l and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak020cwv4p5l/executive.
2020/10/07 08:59:30 61.643 -151.063 68.8 4.1 Alaska
USGS/SLU Moment Tensor Solution ENS 2020/10/07 08:59:30:0 61.64 -151.06 68.8 4.1 Alaska Stations used: AK.CAST AK.CUT AK.DHY AK.GHO AK.KNK AK.L19K AK.L20K AK.M20K AK.N19K AK.PPLA AK.RC01 AK.RND AK.SAW AK.SCM AK.SKN AK.TRF AT.PMR AV.RED AV.SPU AV.STLK TA.M22K TA.O22K Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 2.11e+22 dyne-cm Mw = 4.15 Z = 76 km Plane Strike Dip Rake NP1 190 80 -70 NP2 306 22 -153 Principal Axes: Axis Value Plunge Azimuth T 2.11e+22 32 263 N 0.00e+00 20 6 P -2.11e+22 51 123 Moment Tensor: (dyne-cm) Component Value Mxx -2.23e+21 Mxy 5.53e+21 Mxz 4.48e+21 Myy 9.02e+21 Myz -1.82e+22 Mzz -6.79e+21 ----------#### -------------######### ---############----######### ################--------###### #################-----------###### ##################-------------##### ##################----------------#### ###################-----------------#### ##################-------------------### ###################-------------------#### ##### ###########--------------------### ##### T ##########---------------------### ##### ##########---------- ---------## #################---------- P ---------# ################----------- --------## ###############----------------------# ##############---------------------- #############--------------------- ###########------------------- ##########------------------ #######--------------- ###----------- Global CMT Convention Moment Tensor: R T P -6.79e+21 4.48e+21 1.82e+22 4.48e+21 -2.23e+21 -5.53e+21 1.82e+22 -5.53e+21 9.02e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20201007085930/index.html |
STK = 190 DIP = 80 RAKE = -70 MW = 4.15 HS = 76.0
The NDK file is 20201007085930.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 +50 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 2.0 155 45 65 3.26 0.1210 WVFGRD96 4.0 295 55 -30 3.33 0.1353 WVFGRD96 6.0 300 60 -25 3.38 0.1621 WVFGRD96 8.0 300 55 -25 3.47 0.1785 WVFGRD96 10.0 120 60 -25 3.51 0.1883 WVFGRD96 12.0 120 65 -25 3.55 0.1945 WVFGRD96 14.0 120 65 -25 3.59 0.1951 WVFGRD96 16.0 225 65 40 3.61 0.1941 WVFGRD96 18.0 215 70 40 3.63 0.1996 WVFGRD96 20.0 210 80 35 3.66 0.2055 WVFGRD96 22.0 210 80 40 3.69 0.2114 WVFGRD96 24.0 210 80 40 3.71 0.2179 WVFGRD96 26.0 210 80 40 3.73 0.2234 WVFGRD96 28.0 210 80 40 3.75 0.2271 WVFGRD96 30.0 210 80 40 3.76 0.2266 WVFGRD96 32.0 210 75 -25 3.78 0.2284 WVFGRD96 34.0 205 70 -30 3.79 0.2382 WVFGRD96 36.0 205 70 -30 3.81 0.2453 WVFGRD96 38.0 205 70 -30 3.84 0.2537 WVFGRD96 40.0 205 80 -45 3.94 0.2663 WVFGRD96 42.0 30 90 50 3.98 0.2738 WVFGRD96 44.0 205 80 -50 3.99 0.2908 WVFGRD96 46.0 205 80 -50 4.01 0.3057 WVFGRD96 48.0 205 80 -50 4.03 0.3230 WVFGRD96 50.0 200 75 -55 4.04 0.3391 WVFGRD96 52.0 190 75 -65 4.06 0.3548 WVFGRD96 54.0 190 75 -65 4.07 0.3698 WVFGRD96 56.0 190 75 -65 4.09 0.3836 WVFGRD96 58.0 190 75 -65 4.10 0.3949 WVFGRD96 60.0 190 75 -65 4.10 0.4043 WVFGRD96 62.0 190 75 -65 4.11 0.4111 WVFGRD96 64.0 190 75 -70 4.12 0.4175 WVFGRD96 66.0 190 75 -70 4.13 0.4210 WVFGRD96 68.0 190 75 -70 4.13 0.4237 WVFGRD96 70.0 190 80 -70 4.14 0.4265 WVFGRD96 72.0 190 80 -70 4.14 0.4290 WVFGRD96 74.0 190 80 -70 4.15 0.4294 WVFGRD96 76.0 190 80 -70 4.15 0.4297 WVFGRD96 78.0 190 80 -70 4.16 0.4286 WVFGRD96 80.0 190 80 -70 4.16 0.4267 WVFGRD96 82.0 190 80 -70 4.16 0.4248 WVFGRD96 84.0 190 80 -70 4.17 0.4209 WVFGRD96 86.0 190 80 -70 4.17 0.4171 WVFGRD96 88.0 190 80 -70 4.17 0.4119 WVFGRD96 90.0 185 80 -75 4.18 0.4069 WVFGRD96 92.0 185 80 -70 4.18 0.4010 WVFGRD96 94.0 190 85 -70 4.18 0.3965 WVFGRD96 96.0 190 85 -70 4.18 0.3914 WVFGRD96 98.0 185 75 -70 4.17 0.3885
The best solution is
WVFGRD96 76.0 190 80 -70 4.15 0.4297
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 +50 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