The ANSS event ID is ak02326457m5 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak02326457m5/executive.
2023/02/16 23:32:34 61.527 -150.544 65.1 4 Alaska
USGS/SLU Moment Tensor Solution ENS 2023/02/16 23:32:34:0 61.53 -150.54 65.1 4.0 Alaska Stations used: AK.CAPN AK.CUT AK.FIRE AK.GHO AK.GLI AK.KNK AK.L22K AK.PWL AK.RC01 AK.SCM AK.SKN AK.SLK AT.PMR AV.STLK 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 0.06 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 3.43e+22 dyne-cm Mw = 4.29 Z = 82 km Plane Strike Dip Rake NP1 222 78 -118 NP2 110 30 -25 Principal Axes: Axis Value Plunge Azimuth T 3.43e+22 28 334 N 0.00e+00 27 228 P -3.43e+22 50 102 Moment Tensor: (dyne-cm) Component Value Mxx 2.11e+22 Mxy -7.87e+21 Mxz 1.60e+22 Myy -8.52e+21 Myz -2.28e+22 Mzz -1.25e+22 ############## ###################### ###### ################### ####### T ################---- ######### #############--------- ########################------------ #######################--------------- ######################------------------ ####################-------------------- --#################----------------------- --################------------------------ ---#############------------- ---------- ---############-------------- P ---------- ---#########---------------- --------- -----######----------------------------- -----####----------------------------- ------#----------------------------# -----###-----------------------### --########---------------##### ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -1.25e+22 1.60e+22 2.28e+22 1.60e+22 2.11e+22 7.87e+21 2.28e+22 7.87e+21 -8.52e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230216233234/index.html |
STK = 110 DIP = 30 RAKE = -25 MW = 4.29 HS = 82.0
The NDK file is 20230216233234.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 0.06 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 2.0 95 50 -45 3.60 0.2991 WVFGRD96 4.0 95 70 -60 3.72 0.3303 WVFGRD96 6.0 125 55 40 3.72 0.3611 WVFGRD96 8.0 85 50 -65 3.81 0.3836 WVFGRD96 10.0 130 55 45 3.78 0.4059 WVFGRD96 12.0 125 60 40 3.78 0.4122 WVFGRD96 14.0 120 65 35 3.77 0.4164 WVFGRD96 16.0 120 60 30 3.78 0.4202 WVFGRD96 18.0 120 60 30 3.79 0.4235 WVFGRD96 20.0 120 60 25 3.80 0.4258 WVFGRD96 22.0 105 65 -30 3.83 0.4390 WVFGRD96 24.0 105 65 -30 3.84 0.4464 WVFGRD96 26.0 105 65 -30 3.86 0.4517 WVFGRD96 28.0 105 60 -30 3.87 0.4544 WVFGRD96 30.0 105 60 -30 3.89 0.4560 WVFGRD96 32.0 105 60 -25 3.90 0.4555 WVFGRD96 34.0 105 60 -25 3.92 0.4524 WVFGRD96 36.0 105 60 -25 3.94 0.4457 WVFGRD96 38.0 120 55 5 3.93 0.4396 WVFGRD96 40.0 100 50 -35 4.05 0.4526 WVFGRD96 42.0 115 40 -15 4.05 0.4586 WVFGRD96 44.0 110 35 -25 4.08 0.4687 WVFGRD96 46.0 105 35 -30 4.10 0.4823 WVFGRD96 48.0 105 35 -30 4.12 0.4977 WVFGRD96 50.0 100 35 -40 4.14 0.5145 WVFGRD96 52.0 100 35 -40 4.16 0.5314 WVFGRD96 54.0 100 35 -40 4.17 0.5467 WVFGRD96 56.0 100 35 -35 4.18 0.5610 WVFGRD96 58.0 100 35 -35 4.19 0.5745 WVFGRD96 60.0 105 35 -30 4.20 0.5860 WVFGRD96 62.0 105 35 -30 4.21 0.5970 WVFGRD96 64.0 105 35 -30 4.22 0.6055 WVFGRD96 66.0 105 35 -30 4.23 0.6141 WVFGRD96 68.0 105 35 -30 4.24 0.6203 WVFGRD96 70.0 105 35 -25 4.24 0.6254 WVFGRD96 72.0 110 35 -25 4.25 0.6305 WVFGRD96 74.0 110 35 -25 4.26 0.6343 WVFGRD96 76.0 110 35 -25 4.27 0.6363 WVFGRD96 78.0 110 30 -25 4.27 0.6382 WVFGRD96 80.0 110 30 -25 4.28 0.6394 WVFGRD96 82.0 110 30 -25 4.29 0.6395 WVFGRD96 84.0 110 30 -25 4.29 0.6381 WVFGRD96 86.0 115 30 -20 4.30 0.6362 WVFGRD96 88.0 115 30 -20 4.30 0.6328 WVFGRD96 90.0 115 30 -20 4.31 0.6284 WVFGRD96 92.0 115 35 -20 4.31 0.6231 WVFGRD96 94.0 115 35 -20 4.31 0.6174 WVFGRD96 96.0 115 35 -20 4.31 0.6112 WVFGRD96 98.0 115 35 -20 4.31 0.6048
The best solution is
WVFGRD96 82.0 110 30 -25 4.29 0.6395
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 0.06 n 3 br c 0.12 0.25 n 4 p 2
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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