The ANSS event ID is aka2026ovufno and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/aka2026ovufno/executive.
2026/07/28 20:49:24 63.611 -150.673 5.0 5.0 Alaska
USGS/SLU Moment Tensor Solution
ENS 2026/07/28 20:49:24.0 63.61 -150.67 5.0 5.0 Alaska
Stations used:
AK.BAE AK.BPAW AK.CAST AK.CCB AK.COLD AK.CUT AK.DIV AK.DOT
AK.EYAK AK.F21K AK.FID AK.G19K AK.G24K AK.GHO AK.GLI
AK.H22K AK.H23K AK.H24K AK.HDA AK.HIN AK.I21K AK.I26K
AK.J19K AK.J20K AK.J25K AK.K24K AK.K27K AK.KNK AK.L17K
AK.L22K AK.M26K AK.MCK AK.N18K AK.NEA2 AK.O19K AK.P23K
AK.PAX AK.POKR AK.PPD AK.PPLA AK.RC01 AK.RIDG AK.RND AK.SAW
AK.SCM AK.SCRK AK.SKN AK.SWD AK.WRH AT.PMR AT.TTA AV.RED
AV.SPCL AV.STLK AV.WAZA IM.IL31 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 = 7.59e+22 dyne-cm
Mw = 4.52
Z = 16 km
Plane Strike Dip Rake
NP1 48 62 101
NP2 205 30 70
Principal Axes:
Axis Value Plunge Azimuth
T 7.59e+22 71 342
N 0.00e+00 10 222
P -7.59e+22 16 130
Moment Tensor: (dyne-cm)
Component Value
Mxx -2.10e+22
Mxy 3.20e+22
Mxz 3.54e+22
Myy -4.08e+22
Myz -2.28e+22
Mzz 6.17e+22
--------------
---------#############
---------###################
-------#######################
--------########################--
-------##########################---
-------##########################-----
-------########## ##############------
------########### T #############-------
------############ ############---------
------#########################-----------
------########################------------
------######################--------------
-----####################---------------
-----##################-----------------
----################------------------
----############-------------- ---
---########------------------ P --
--#------------------------
##--------------------------
#---------------------
--------------
Global CMT Convention Moment Tensor:
R T P
6.17e+22 3.54e+22 2.28e+22
3.54e+22 -2.10e+22 -3.20e+22
2.28e+22 -3.20e+22 -4.08e+22
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260728204924/index.html
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STK = 205
DIP = 30
RAKE = 70
MW = 4.52
HS = 16.0
The NDK file is 20260728204924.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 2026/07/28 20:49:24.0 63.61 -150.67 5.0 5.0 Alaska
Stations used:
AK.BAE AK.BPAW AK.CAST AK.CCB AK.COLD AK.CUT AK.DIV AK.DOT
AK.EYAK AK.F21K AK.FID AK.G19K AK.G24K AK.GHO AK.GLI
AK.H22K AK.H23K AK.H24K AK.HDA AK.HIN AK.I21K AK.I26K
AK.J19K AK.J20K AK.J25K AK.K24K AK.K27K AK.KNK AK.L17K
AK.L22K AK.M26K AK.MCK AK.N18K AK.NEA2 AK.O19K AK.P23K
AK.PAX AK.POKR AK.PPD AK.PPLA AK.RC01 AK.RIDG AK.RND AK.SAW
AK.SCM AK.SCRK AK.SKN AK.SWD AK.WRH AT.PMR AT.TTA AV.RED
AV.SPCL AV.STLK AV.WAZA IM.IL31 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 = 7.59e+22 dyne-cm
Mw = 4.52
Z = 16 km
Plane Strike Dip Rake
NP1 48 62 101
NP2 205 30 70
Principal Axes:
Axis Value Plunge Azimuth
T 7.59e+22 71 342
N 0.00e+00 10 222
P -7.59e+22 16 130
Moment Tensor: (dyne-cm)
Component Value
Mxx -2.10e+22
Mxy 3.20e+22
Mxz 3.54e+22
Myy -4.08e+22
Myz -2.28e+22
Mzz 6.17e+22
--------------
---------#############
---------###################
-------#######################
--------########################--
-------##########################---
-------##########################-----
-------########## ##############------
------########### T #############-------
------############ ############---------
------#########################-----------
------########################------------
------######################--------------
-----####################---------------
-----##################-----------------
----################------------------
----############-------------- ---
---########------------------ P --
--#------------------------
##--------------------------
#---------------------
--------------
Global CMT Convention Moment Tensor:
R T P
6.17e+22 3.54e+22 2.28e+22
3.54e+22 -2.10e+22 -3.20e+22
2.28e+22 -3.20e+22 -4.08e+22
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260728204924/index.html
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Regional Moment Tensor (Mwr) Moment 7.584e+15 N-m Magnitude 4.52 Mwr Depth 16.0 km Percent DC 86% Half Duration - Catalog US Data Source US Contributor US Nodal Planes Plane Strike Dip Rake NP1 207 25 67 NP2 52 67 101 Principal Axes Axis Value Plunge Azimuth T 7.300e+15 67 341 N 0.540e+15 10 228 P -7.840e+15 21 134 |
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.
Map showing station locations used for computing the ML's. No distinction is made whether the vertical (Z) or horizontal (H) components were used.
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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 60 45 -90 4.09 0.2948
WVFGRD96 2.0 60 45 -90 4.22 0.3750
WVFGRD96 3.0 265 40 -50 4.21 0.2647
WVFGRD96 4.0 315 20 -20 4.24 0.3245
WVFGRD96 5.0 320 20 -15 4.26 0.3888
WVFGRD96 6.0 345 20 15 4.27 0.4399
WVFGRD96 7.0 355 20 30 4.28 0.4791
WVFGRD96 8.0 5 20 35 4.37 0.5061
WVFGRD96 9.0 200 25 60 4.40 0.5484
WVFGRD96 10.0 200 25 65 4.42 0.5925
WVFGRD96 11.0 205 30 70 4.45 0.6266
WVFGRD96 12.0 205 30 70 4.46 0.6536
WVFGRD96 13.0 210 30 75 4.48 0.6723
WVFGRD96 14.0 205 30 70 4.49 0.6835
WVFGRD96 15.0 205 30 70 4.51 0.6884
WVFGRD96 16.0 205 30 70 4.52 0.6885
WVFGRD96 17.0 205 30 70 4.53 0.6844
WVFGRD96 18.0 205 30 70 4.54 0.6762
WVFGRD96 19.0 200 30 65 4.55 0.6651
WVFGRD96 20.0 200 30 65 4.56 0.6514
WVFGRD96 21.0 200 30 60 4.57 0.6356
WVFGRD96 22.0 200 30 60 4.58 0.6190
WVFGRD96 23.0 200 30 60 4.58 0.6011
WVFGRD96 24.0 200 30 60 4.59 0.5827
WVFGRD96 25.0 195 30 55 4.60 0.5637
WVFGRD96 26.0 200 25 60 4.61 0.5443
WVFGRD96 27.0 200 25 60 4.61 0.5256
WVFGRD96 28.0 200 25 60 4.62 0.5060
WVFGRD96 29.0 200 25 60 4.62 0.4862
The best solution is
WVFGRD96 16.0 205 30 70 4.52 0.6885
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