The ANSS event ID is ak023be9qxdf and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak023be9qxdf/executive.
2023/09/05 07:50:50 60.680 -146.876 29.3 3.6 Alaska
USGS/SLU Moment Tensor Solution ENS 2023/09/05 07:50:50:0 60.68 -146.88 29.3 3.6 Alaska Stations used: AK.BMR AK.DIV AK.EYAK AK.FID AK.GHO AK.GLI AK.HIN AK.KLU AK.KNK AK.PWL AK.Q23K AK.SAW AK.SCM AK.SLK AK.SWD AK.WAT6 AT.PMR 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 0.06 n 3 Best Fitting Double Couple Mo = 6.31e+21 dyne-cm Mw = 3.80 Z = 47 km Plane Strike Dip Rake NP1 70 80 -15 NP2 163 75 -170 Principal Axes: Axis Value Plunge Azimuth T 6.31e+21 3 117 N 0.00e+00 72 217 P -6.31e+21 18 26 Moment Tensor: (dyne-cm) Component Value Mxx -3.36e+21 Mxy -4.78e+21 Mxz -1.80e+21 Myy 3.92e+21 Myz -4.70e+20 Mzz -5.59e+20 #------------- #####------------ -- #######------------- P ----- #########------------ ------ ###########----------------------- ############------------------------ #############------------------------- ##############-------------------------# ###############---------------------#### ################------------------######## #################-------------############ #################---------################ ##################---##################### ##############----###################### ######------------################### ------------------################## T ------------------################# ------------------################ -----------------############# -----------------########### ---------------####### -------------# Global CMT Convention Moment Tensor: R T P -5.59e+20 -1.80e+21 4.70e+20 -1.80e+21 -3.36e+21 4.78e+21 4.70e+20 4.78e+21 3.92e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230905075050/index.html |
STK = 70 DIP = 80 RAKE = -15 MW = 3.80 HS = 47.0
The NDK file is 20230905075050.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 -30 o DIST/3.3 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 40 50 -60 3.06 0.2303 WVFGRD96 2.0 40 50 -60 3.20 0.3220 WVFGRD96 3.0 45 45 -50 3.25 0.3474 WVFGRD96 4.0 65 55 -20 3.22 0.3622 WVFGRD96 5.0 70 60 -5 3.24 0.3790 WVFGRD96 6.0 255 60 30 3.29 0.4060 WVFGRD96 7.0 255 60 30 3.31 0.4329 WVFGRD96 8.0 260 55 40 3.38 0.4550 WVFGRD96 9.0 260 55 40 3.40 0.4738 WVFGRD96 10.0 250 70 25 3.37 0.4892 WVFGRD96 11.0 250 65 20 3.39 0.5044 WVFGRD96 12.0 250 65 20 3.41 0.5202 WVFGRD96 13.0 250 65 20 3.42 0.5345 WVFGRD96 14.0 250 70 10 3.43 0.5486 WVFGRD96 15.0 250 70 10 3.44 0.5612 WVFGRD96 16.0 250 70 10 3.46 0.5722 WVFGRD96 17.0 250 75 10 3.47 0.5818 WVFGRD96 18.0 250 75 10 3.48 0.5912 WVFGRD96 19.0 250 75 5 3.49 0.5992 WVFGRD96 20.0 250 75 5 3.50 0.6063 WVFGRD96 21.0 250 80 10 3.51 0.6126 WVFGRD96 22.0 250 75 5 3.52 0.6178 WVFGRD96 23.0 250 80 5 3.53 0.6224 WVFGRD96 24.0 250 80 5 3.54 0.6267 WVFGRD96 25.0 250 80 5 3.55 0.6297 WVFGRD96 26.0 70 90 -10 3.56 0.6316 WVFGRD96 27.0 250 80 5 3.57 0.6341 WVFGRD96 28.0 250 85 5 3.57 0.6354 WVFGRD96 29.0 70 85 -10 3.58 0.6372 WVFGRD96 30.0 70 85 -10 3.59 0.6380 WVFGRD96 31.0 70 85 -10 3.60 0.6379 WVFGRD96 32.0 250 90 15 3.61 0.6376 WVFGRD96 33.0 70 85 -15 3.62 0.6376 WVFGRD96 34.0 70 85 -15 3.64 0.6366 WVFGRD96 35.0 250 90 10 3.64 0.6335 WVFGRD96 36.0 70 85 -15 3.66 0.6361 WVFGRD96 37.0 250 90 10 3.67 0.6359 WVFGRD96 38.0 250 90 10 3.69 0.6385 WVFGRD96 39.0 250 90 10 3.71 0.6412 WVFGRD96 40.0 70 85 -15 3.74 0.6486 WVFGRD96 41.0 70 80 -15 3.75 0.6517 WVFGRD96 42.0 70 80 -15 3.76 0.6541 WVFGRD96 43.0 70 80 -15 3.77 0.6555 WVFGRD96 44.0 70 80 -15 3.78 0.6561 WVFGRD96 45.0 70 80 -15 3.79 0.6568 WVFGRD96 46.0 70 80 -15 3.79 0.6565 WVFGRD96 47.0 70 80 -15 3.80 0.6568 WVFGRD96 48.0 70 80 -15 3.81 0.6557 WVFGRD96 49.0 70 80 -15 3.82 0.6554 WVFGRD96 50.0 70 80 -15 3.82 0.6543 WVFGRD96 51.0 70 85 -15 3.83 0.6533 WVFGRD96 52.0 70 85 -15 3.84 0.6522 WVFGRD96 53.0 70 85 -15 3.84 0.6506 WVFGRD96 54.0 70 85 -15 3.85 0.6499 WVFGRD96 55.0 70 85 -15 3.85 0.6485 WVFGRD96 56.0 250 90 10 3.85 0.6430 WVFGRD96 57.0 70 85 -15 3.86 0.6454 WVFGRD96 58.0 70 85 -10 3.86 0.6433 WVFGRD96 59.0 70 85 -10 3.87 0.6414
The best solution is
WVFGRD96 47.0 70 80 -15 3.80 0.6568
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 0.06 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