The ANSS event ID is ak0217ti4bu9 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0217ti4bu9/executive.
2021/06/19 21:43:05 63.999 -149.780 12.7 4.4 Alaska
USGS/SLU Moment Tensor Solution ENS 2021/06/19 21:43:05:0 64.00 -149.78 12.7 4.4 Alaska Stations used: AK.BPAW AK.CAST AK.CCB AK.COLD AK.CUT AK.DHY AK.DIV AK.DOT AK.EYAK AK.F21K AK.FID AK.G23K AK.G24K AK.GHO AK.GLB AK.GLI AK.H21K AK.H22K AK.H23K AK.H24K AK.HARP AK.HDA AK.HIN AK.I21K AK.I23K AK.I27K AK.J19K AK.J20K AK.J25K AK.K20K AK.K24K AK.KLU AK.KNK AK.KTH AK.L19K AK.L20K AK.L26K AK.M19K AK.M20K AK.M26K AK.M27K AK.MCAR AK.MCK AK.MLY AK.NEA2 AK.PAX AK.POKR AK.PPD AK.PPLA AK.PWL AK.RC01 AK.RIDG AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.SLK AK.SSN AK.SWD AK.TRF AK.VRDI AK.WRH AT.MENT AT.PMR AV.RED AV.SPCP AV.STLK IU.COLA 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 = 3.20e+22 dyne-cm Mw = 4.27 Z = 15 km Plane Strike Dip Rake NP1 40 55 65 NP2 259 42 121 Principal Axes: Axis Value Plunge Azimuth T 3.20e+22 69 255 N 0.00e+00 20 55 P -3.20e+22 7 148 Moment Tensor: (dyne-cm) Component Value Mxx -2.22e+22 Mxy 1.53e+22 Mxz 4.34e+20 Myy -5.08e+21 Myz -1.26e+22 Mzz 2.72e+22 -------------- ---------------------- ---------------------------# -----------------------------# -----------------######--------### -----------####################-#### --------#########################--### ------###########################-----## ----#############################------- ----#############################--------- ---########### ###############---------- --############ T ##############----------- -############# #############------------ ############################------------ ##########################-------------- #######################--------------- ####################---------------- #################----------------- ###########-------------- -- #####------------------- P - --------------------- -------------- Global CMT Convention Moment Tensor: R T P 2.72e+22 4.34e+20 1.26e+22 4.34e+20 -2.22e+22 -1.53e+22 1.26e+22 -1.53e+22 -5.08e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210619214305/index.html |
STK = 40 DIP = 55 RAKE = 65 MW = 4.27 HS = 15.0
The NDK file is 20210619214305.ndk The waveform inversion is preferred.
The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
USGS/SLU Moment Tensor Solution ENS 2021/06/19 21:43:05:0 64.00 -149.78 12.7 4.4 Alaska Stations used: AK.BPAW AK.CAST AK.CCB AK.COLD AK.CUT AK.DHY AK.DIV AK.DOT AK.EYAK AK.F21K AK.FID AK.G23K AK.G24K AK.GHO AK.GLB AK.GLI AK.H21K AK.H22K AK.H23K AK.H24K AK.HARP AK.HDA AK.HIN AK.I21K AK.I23K AK.I27K AK.J19K AK.J20K AK.J25K AK.K20K AK.K24K AK.KLU AK.KNK AK.KTH AK.L19K AK.L20K AK.L26K AK.M19K AK.M20K AK.M26K AK.M27K AK.MCAR AK.MCK AK.MLY AK.NEA2 AK.PAX AK.POKR AK.PPD AK.PPLA AK.PWL AK.RC01 AK.RIDG AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.SLK AK.SSN AK.SWD AK.TRF AK.VRDI AK.WRH AT.MENT AT.PMR AV.RED AV.SPCP AV.STLK IU.COLA 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 = 3.20e+22 dyne-cm Mw = 4.27 Z = 15 km Plane Strike Dip Rake NP1 40 55 65 NP2 259 42 121 Principal Axes: Axis Value Plunge Azimuth T 3.20e+22 69 255 N 0.00e+00 20 55 P -3.20e+22 7 148 Moment Tensor: (dyne-cm) Component Value Mxx -2.22e+22 Mxy 1.53e+22 Mxz 4.34e+20 Myy -5.08e+21 Myz -1.26e+22 Mzz 2.72e+22 -------------- ---------------------- ---------------------------# -----------------------------# -----------------######--------### -----------####################-#### --------#########################--### ------###########################-----## ----#############################------- ----#############################--------- ---########### ###############---------- --############ T ##############----------- -############# #############------------ ############################------------ ##########################-------------- #######################--------------- ####################---------------- #################----------------- ###########-------------- -- #####------------------- P - --------------------- -------------- Global CMT Convention Moment Tensor: R T P 2.72e+22 4.34e+20 1.26e+22 4.34e+20 -2.22e+22 -1.53e+22 1.26e+22 -1.53e+22 -5.08e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210619214305/index.html |
Regional Moment Tensor (Mwr) Moment 3.430e+15 N-m Magnitude 4.29 Mwr Depth 15.0 km Percent DC 91% Half Duration - Catalog US Data Source US 2 Contributor US 2 Nodal Planes Plane Strike Dip Rake NP1 255° 35° 112° NP2 48° 58° 75° Principal Axes Axis Value Plunge Azimuth T 3.345e+15 N-m 73° 281° N 0.165e+15 N-m 13° 56° P -3.510e+15 N-m 12° 149° |
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 1.0 230 45 -90 3.82 0.2522 WVFGRD96 2.0 50 45 -90 3.97 0.3382 WVFGRD96 3.0 75 70 -65 3.97 0.2522 WVFGRD96 4.0 75 75 -70 3.99 0.3060 WVFGRD96 5.0 75 80 -75 4.01 0.3684 WVFGRD96 6.0 75 75 -75 4.03 0.4210 WVFGRD96 7.0 75 75 -75 4.04 0.4613 WVFGRD96 8.0 75 75 -75 4.13 0.4923 WVFGRD96 9.0 35 30 55 4.15 0.5301 WVFGRD96 10.0 40 60 65 4.19 0.5817 WVFGRD96 11.0 40 55 65 4.21 0.6271 WVFGRD96 12.0 40 55 65 4.23 0.6616 WVFGRD96 13.0 40 55 65 4.25 0.6841 WVFGRD96 14.0 40 55 65 4.26 0.6962 WVFGRD96 15.0 40 55 65 4.27 0.6993 WVFGRD96 16.0 40 50 65 4.28 0.6964 WVFGRD96 17.0 40 50 65 4.29 0.6882 WVFGRD96 18.0 40 50 65 4.30 0.6751 WVFGRD96 19.0 40 45 60 4.31 0.6588 WVFGRD96 20.0 35 45 60 4.32 0.6407 WVFGRD96 21.0 30 45 55 4.33 0.6201 WVFGRD96 22.0 30 45 55 4.34 0.5989 WVFGRD96 23.0 30 45 55 4.34 0.5766 WVFGRD96 24.0 30 40 50 4.35 0.5530 WVFGRD96 25.0 30 40 50 4.35 0.5290 WVFGRD96 26.0 30 40 50 4.35 0.5045 WVFGRD96 27.0 230 60 80 4.36 0.4823 WVFGRD96 28.0 235 60 85 4.36 0.4619 WVFGRD96 29.0 60 30 90 4.36 0.4399
The best solution is
WVFGRD96 15.0 40 55 65 4.27 0.6993
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