The ANSS event ID is ak023e0o5q4j and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak023e0o5q4j/executive.
2023/11/01 15:53:07 61.873 -148.040 8.9 3.7 Alaska
USGS/SLU Moment Tensor Solution ENS 2023/11/01 15:53:07:0 61.87 -148.04 8.9 3.7 Alaska Stations used: AK.BAE AK.CUT AK.DHY AK.DIV AK.EYAK AK.FID AK.GHO AK.GLI AK.KLU AK.KNK AK.PAX AK.PWL AK.RC01 AK.SAW AK.SCM AK.WAT6 AT.PMR 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 0.08 n 3 Best Fitting Double Couple Mo = 6.76e+21 dyne-cm Mw = 3.82 Z = 42 km Plane Strike Dip Rake NP1 74 65 -95 NP2 265 25 -80 Principal Axes: Axis Value Plunge Azimuth T 6.76e+21 20 167 N 0.00e+00 4 76 P -6.76e+21 69 335 Moment Tensor: (dyne-cm) Component Value Mxx 4.98e+21 Mxy -9.31e+20 Mxz -4.17e+21 Myy 1.25e+20 Myz 1.43e+21 Mzz -5.10e+21 ############## ###################### #############---############ ######-------------------##### #####-------------------------#### ####-----------------------------### ###---------------------------------## ###------------- -------------------## #--------------- P --------------------# ##--------------- -------------------##- #------------------------------------##### ----------------------------------######## -------------------------------########### --------------------------############## ##------------------#################### ###################################### #################################### ################################## ################# ########## ################ T ######### ############# ###### ############## Global CMT Convention Moment Tensor: R T P -5.10e+21 -4.17e+21 -1.43e+21 -4.17e+21 4.98e+21 9.31e+20 -1.43e+21 9.31e+20 1.25e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20231101155307/index.html |
STK = 265 DIP = 25 RAKE = -80 MW = 3.82 HS = 42.0
The NDK file is 20231101155307.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 0.08 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 105 40 85 3.00 0.1820 WVFGRD96 2.0 105 40 85 3.15 0.2410 WVFGRD96 3.0 85 40 -85 3.21 0.2065 WVFGRD96 4.0 225 65 -55 3.17 0.1951 WVFGRD96 5.0 235 80 80 3.24 0.2182 WVFGRD96 6.0 235 85 75 3.24 0.2409 WVFGRD96 7.0 235 85 75 3.24 0.2598 WVFGRD96 8.0 235 85 80 3.33 0.2763 WVFGRD96 9.0 235 85 80 3.34 0.2940 WVFGRD96 10.0 55 90 -75 3.35 0.3108 WVFGRD96 11.0 55 90 -75 3.37 0.3267 WVFGRD96 12.0 65 70 -75 3.39 0.3470 WVFGRD96 13.0 65 70 -75 3.41 0.3652 WVFGRD96 14.0 65 70 -75 3.42 0.3812 WVFGRD96 15.0 65 70 -75 3.43 0.3945 WVFGRD96 16.0 65 70 -75 3.45 0.4058 WVFGRD96 17.0 65 70 -80 3.46 0.4156 WVFGRD96 18.0 70 75 -80 3.47 0.4266 WVFGRD96 19.0 70 75 -80 3.48 0.4373 WVFGRD96 20.0 70 75 -80 3.49 0.4472 WVFGRD96 21.0 70 75 -85 3.52 0.4566 WVFGRD96 22.0 230 15 -110 3.53 0.4663 WVFGRD96 23.0 70 75 -85 3.54 0.4756 WVFGRD96 24.0 70 75 -90 3.55 0.4850 WVFGRD96 25.0 250 15 -90 3.57 0.4958 WVFGRD96 26.0 255 15 -85 3.58 0.5068 WVFGRD96 27.0 255 15 -85 3.59 0.5170 WVFGRD96 28.0 255 15 -85 3.60 0.5269 WVFGRD96 29.0 260 20 -75 3.61 0.5377 WVFGRD96 30.0 260 20 -80 3.62 0.5488 WVFGRD96 31.0 260 20 -80 3.63 0.5597 WVFGRD96 32.0 255 20 -90 3.63 0.5707 WVFGRD96 33.0 260 20 -85 3.64 0.5826 WVFGRD96 34.0 260 20 -85 3.65 0.5921 WVFGRD96 35.0 260 20 -85 3.65 0.5973 WVFGRD96 36.0 260 25 -85 3.66 0.6061 WVFGRD96 37.0 265 25 -80 3.67 0.6120 WVFGRD96 38.0 260 25 -85 3.67 0.6147 WVFGRD96 39.0 260 25 -85 3.68 0.6142 WVFGRD96 40.0 265 25 -80 3.80 0.6106 WVFGRD96 41.0 265 25 -80 3.81 0.6145 WVFGRD96 42.0 265 25 -80 3.82 0.6151 WVFGRD96 43.0 265 25 -80 3.82 0.6127 WVFGRD96 44.0 265 25 -80 3.83 0.6093 WVFGRD96 45.0 265 25 -80 3.83 0.6032 WVFGRD96 46.0 265 25 -80 3.84 0.5971 WVFGRD96 47.0 265 25 -80 3.84 0.5903 WVFGRD96 48.0 270 30 -75 3.85 0.5839 WVFGRD96 49.0 270 30 -75 3.85 0.5774 WVFGRD96 50.0 270 30 -75 3.85 0.5698 WVFGRD96 51.0 270 30 -70 3.86 0.5622 WVFGRD96 52.0 270 30 -70 3.86 0.5536 WVFGRD96 53.0 270 30 -70 3.86 0.5449 WVFGRD96 54.0 270 30 -70 3.86 0.5362 WVFGRD96 55.0 265 30 -75 3.86 0.5271 WVFGRD96 56.0 270 30 -70 3.86 0.5189 WVFGRD96 57.0 265 30 -75 3.86 0.5100 WVFGRD96 58.0 265 30 -75 3.86 0.5025 WVFGRD96 59.0 265 30 -75 3.86 0.4944
The best solution is
WVFGRD96 42.0 265 25 -80 3.82 0.6151
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 0.08 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