The ANSS event ID is ak0215dsbmgn and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0215dsbmgn/executive.
2021/04/27 17:54:36 61.342 -149.980 43.8 4.8 Alaska
USGS/SLU Moment Tensor Solution ENS 2021/04/27 17:54:36:0 61.34 -149.98 43.8 4.8 Alaska Stations used: AK.BRLK AK.CNP AK.CUT AK.DHY AK.EYAK AK.FIRE AK.GHO AK.GLI AK.HOM AK.MCK AK.PPLA AK.PWL AK.RC01 AK.SAW AK.SCM AK.SKN AK.SLK AK.SSN AT.PMR AV.ILS AV.RED AV.SPCP TA.M22K 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 = 1.32e+23 dyne-cm Mw = 4.68 Z = 49 km Plane Strike Dip Rake NP1 175 50 -70 NP2 325 44 -112 Principal Axes: Axis Value Plunge Azimuth T 1.32e+23 3 251 N 0.00e+00 15 342 P -1.32e+23 74 150 Moment Tensor: (dyne-cm) Component Value Mxx 6.92e+21 Mxy 4.46e+22 Mxz 2.70e+22 Myy 1.15e+23 Myz -2.40e+22 Mzz -1.22e+23 ----########## ------################ ########----################ ########---------############# #########------------############# #########---------------############ ##########-----------------########### ##########-------------------########### ##########---------------------######### ###########----------------------######### ###########----------------------######### ###########---------- ----------######## ###########---------- P -----------####### #########--------- -----------###### T #########-----------------------###### ##########----------------------##### ##########----------------------#### ##########---------------------### #########-------------------## ##########----------------## ########-------------- #######------- Global CMT Convention Moment Tensor: R T P -1.22e+23 2.70e+22 2.40e+22 2.70e+22 6.92e+21 -4.46e+22 2.40e+22 -4.46e+22 1.15e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210427175436/index.html |
STK = 175 DIP = 50 RAKE = -70 MW = 4.68 HS = 49.0
The NDK file is 20210427175436.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 2021/04/27 17:54:36:0 61.34 -149.98 43.8 4.8 Alaska Stations used: AK.BRLK AK.CNP AK.CUT AK.DHY AK.EYAK AK.FIRE AK.GHO AK.GLI AK.HOM AK.MCK AK.PPLA AK.PWL AK.RC01 AK.SAW AK.SCM AK.SKN AK.SLK AK.SSN AT.PMR AV.ILS AV.RED AV.SPCP TA.M22K 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 = 1.32e+23 dyne-cm Mw = 4.68 Z = 49 km Plane Strike Dip Rake NP1 175 50 -70 NP2 325 44 -112 Principal Axes: Axis Value Plunge Azimuth T 1.32e+23 3 251 N 0.00e+00 15 342 P -1.32e+23 74 150 Moment Tensor: (dyne-cm) Component Value Mxx 6.92e+21 Mxy 4.46e+22 Mxz 2.70e+22 Myy 1.15e+23 Myz -2.40e+22 Mzz -1.22e+23 ----########## ------################ ########----################ ########---------############# #########------------############# #########---------------############ ##########-----------------########### ##########-------------------########### ##########---------------------######### ###########----------------------######### ###########----------------------######### ###########---------- ----------######## ###########---------- P -----------####### #########--------- -----------###### T #########-----------------------###### ##########----------------------##### ##########----------------------#### ##########---------------------### #########-------------------## ##########----------------## ########-------------- #######------- Global CMT Convention Moment Tensor: R T P -1.22e+23 2.70e+22 2.40e+22 2.70e+22 6.92e+21 -4.46e+22 2.40e+22 -4.46e+22 1.15e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210427175436/index.html |
W-phase Moment Tensor (Mww) Moment 1.515e+16 N-m Magnitude 4.72 Mww Depth 45.5 km Percent DC 70% Half Duration 0.59 s Catalog US Data Source US 3 Contributor US 3 Nodal Planes Plane Strike Dip Rake NP1 337 41 -107 NP2 179 51 -76 Principal Axes Axis Value Plunge Azimuth T 1.379e+16 N-m 5 259 N 0.241e+16 N-m 11 350 P -1.621e+16 N-m 78 143 |
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.
![]() |
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.
![]() |
|
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 1.0 175 35 110 3.78 0.1485 WVFGRD96 2.0 280 55 -85 3.96 0.2156 WVFGRD96 3.0 285 55 -80 4.02 0.2440 WVFGRD96 4.0 315 75 -50 3.99 0.2592 WVFGRD96 5.0 315 80 65 4.04 0.2924 WVFGRD96 6.0 275 90 60 4.06 0.3213 WVFGRD96 7.0 275 90 60 4.07 0.3427 WVFGRD96 8.0 270 90 60 4.15 0.3574 WVFGRD96 9.0 90 85 -60 4.17 0.3718 WVFGRD96 10.0 315 80 60 4.18 0.3819 WVFGRD96 11.0 315 80 60 4.20 0.3898 WVFGRD96 12.0 320 75 60 4.22 0.3958 WVFGRD96 13.0 320 75 60 4.23 0.3990 WVFGRD96 14.0 320 75 60 4.25 0.4000 WVFGRD96 15.0 320 80 55 4.26 0.3998 WVFGRD96 16.0 320 80 55 4.27 0.4005 WVFGRD96 17.0 185 55 35 4.28 0.4010 WVFGRD96 18.0 185 50 30 4.29 0.4018 WVFGRD96 19.0 185 50 30 4.30 0.4015 WVFGRD96 20.0 185 50 30 4.31 0.4004 WVFGRD96 21.0 190 45 35 4.33 0.3989 WVFGRD96 22.0 190 45 35 4.34 0.3955 WVFGRD96 23.0 190 45 35 4.35 0.3928 WVFGRD96 24.0 230 40 30 4.36 0.3907 WVFGRD96 25.0 230 35 30 4.37 0.3903 WVFGRD96 26.0 230 35 30 4.38 0.3909 WVFGRD96 27.0 230 35 30 4.39 0.3899 WVFGRD96 28.0 230 35 30 4.39 0.3882 WVFGRD96 29.0 230 35 30 4.40 0.3853 WVFGRD96 30.0 225 40 30 4.41 0.3836 WVFGRD96 31.0 185 55 -65 4.43 0.4087 WVFGRD96 32.0 185 55 -65 4.45 0.4436 WVFGRD96 33.0 185 55 -65 4.46 0.4744 WVFGRD96 34.0 185 55 -65 4.47 0.5047 WVFGRD96 35.0 185 55 -65 4.48 0.5284 WVFGRD96 36.0 180 50 -65 4.49 0.5478 WVFGRD96 37.0 185 55 -65 4.50 0.5639 WVFGRD96 38.0 185 55 -65 4.51 0.5778 WVFGRD96 39.0 185 55 -60 4.52 0.5928 WVFGRD96 40.0 180 50 -70 4.60 0.5845 WVFGRD96 41.0 180 50 -70 4.62 0.5954 WVFGRD96 42.0 180 50 -70 4.63 0.6069 WVFGRD96 43.0 180 50 -70 4.64 0.6152 WVFGRD96 44.0 180 50 -70 4.65 0.6210 WVFGRD96 45.0 175 50 -70 4.66 0.6267 WVFGRD96 46.0 175 50 -70 4.67 0.6296 WVFGRD96 47.0 175 50 -75 4.67 0.6307 WVFGRD96 48.0 175 50 -70 4.68 0.6307 WVFGRD96 49.0 175 50 -70 4.68 0.6318 WVFGRD96 50.0 175 50 -75 4.69 0.6293 WVFGRD96 51.0 175 50 -70 4.69 0.6272 WVFGRD96 52.0 175 50 -75 4.69 0.6244 WVFGRD96 53.0 180 55 -65 4.70 0.6217 WVFGRD96 54.0 180 55 -65 4.70 0.6175 WVFGRD96 55.0 180 55 -65 4.70 0.6136 WVFGRD96 56.0 180 55 -65 4.70 0.6101 WVFGRD96 57.0 180 55 -65 4.71 0.6043 WVFGRD96 58.0 180 55 -65 4.71 0.5986 WVFGRD96 59.0 180 55 -65 4.71 0.5940
The best solution is
WVFGRD96 49.0 175 50 -70 4.68 0.6318
The mechanism corresponding to the best fit is
![]() |
|
The best fit as a function of depth is given in the following figure:
![]() |
|
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
![]() |
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. |
![]() |
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