The ANSS event ID is aka2026ltinws and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/aka2026ltinws/executive.
2026/06/15 07:27:36 65.164 -162.022 10.0 3.6 Alaska
USGS/SLU Moment Tensor Solution
ENS 2026/06/15 07:27:36.0 65.16 -162.02 10.0 3.6 Alaska
Stations used:
AK.G19K AK.GCSA AK.H17K AK.J19K AK.J20K AK.K15K AK.RDOG
AT.TTA
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 = 2.75e+21 dyne-cm
Mw = 3.56
Z = 13 km
Plane Strike Dip Rake
NP1 104 85 170
NP2 195 80 5
Principal Axes:
Axis Value Plunge Azimuth
T 2.75e+21 11 59
N 0.00e+00 79 258
P -2.75e+21 4 150
Moment Tensor: (dyne-cm)
Component Value
Mxx -1.36e+21
Mxy 2.36e+21
Mxz 4.02e+20
Myy 1.27e+21
Myz 3.41e+20
Mzz 8.21e+19
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-----------------###########
-----------------#############
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-------------------############# T #
-------------------############## ##
-------------------#####################
#------------------#####################
#######------------#######################
#############------#######################
##################--######################
##################---------###############
################--------------------####
################------------------------
###############-----------------------
#############-----------------------
############----------------------
##########--------------------
#########------------- ---
######------------- P
##------------
Global CMT Convention Moment Tensor:
R T P
8.21e+19 4.02e+20 -3.41e+20
4.02e+20 -1.36e+21 -2.36e+21
-3.41e+20 -2.36e+21 1.27e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260615072736/index.html
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STK = 195
DIP = 80
RAKE = 5
MW = 3.56
HS = 13.0
The NDK file is 20260615072736.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.
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 25 90 -5 3.01 0.2895
WVFGRD96 2.0 20 90 -10 3.16 0.4290
WVFGRD96 3.0 205 75 10 3.24 0.4924
WVFGRD96 4.0 200 80 10 3.27 0.5472
WVFGRD96 5.0 200 80 10 3.32 0.5959
WVFGRD96 6.0 15 70 -10 3.37 0.6409
WVFGRD96 7.0 200 90 5 3.40 0.6824
WVFGRD96 8.0 15 80 -10 3.44 0.7251
WVFGRD96 9.0 15 80 -10 3.47 0.7523
WVFGRD96 10.0 15 75 -5 3.50 0.7709
WVFGRD96 11.0 15 75 -5 3.53 0.7841
WVFGRD96 12.0 195 75 5 3.54 0.7903
WVFGRD96 13.0 195 80 5 3.56 0.7934
WVFGRD96 14.0 195 80 5 3.58 0.7914
WVFGRD96 15.0 195 80 5 3.59 0.7849
WVFGRD96 16.0 15 90 -5 3.60 0.7732
WVFGRD96 17.0 15 90 -5 3.61 0.7590
WVFGRD96 18.0 195 75 5 3.62 0.7443
WVFGRD96 19.0 195 75 5 3.63 0.7261
WVFGRD96 20.0 195 75 5 3.64 0.7042
WVFGRD96 21.0 195 75 5 3.65 0.6790
WVFGRD96 22.0 195 75 5 3.65 0.6514
WVFGRD96 23.0 195 65 10 3.66 0.6238
WVFGRD96 24.0 195 65 10 3.66 0.5939
WVFGRD96 25.0 195 65 10 3.66 0.5613
WVFGRD96 26.0 195 65 10 3.66 0.5266
WVFGRD96 27.0 200 50 10 3.68 0.4935
WVFGRD96 28.0 200 45 10 3.69 0.4618
WVFGRD96 29.0 200 35 10 3.72 0.4352
The best solution is
WVFGRD96 13.0 195 80 5 3.56 0.7934
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