Location

Location ANSS

The ANSS event ID is aka2026tfvugv and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/aka2026tfvugv/executive.

2026/09/28 14:55:54 63.507 -151.604 5.0 4.2 Alaska

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2026/09/28 14:55:54.0  63.51 -151.60   5.0 4.2 Alaska
 
 Stations used:
   AK.BPAW AK.CAPN AK.CAST AK.CCB AK.CUT AK.DIV AK.DOT AK.F21K 
   AK.FID AK.G19K AK.G24K AK.GCSA AK.GHO AK.H17K AK.H22K 
   AK.H23K AK.H24K AK.HDA AK.HIN AK.I21K AK.I23K AK.J19K 
   AK.J20K AK.J25K AK.K20K AK.K24K AK.KNK AK.L17K AK.L22K 
   AK.MCK AK.NEA2 AK.O19K AK.PAX AK.POKR AK.RC01 AK.RIDG 
   AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.WRH AT.PMR 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 = 7.24e+21 dyne-cm
  Mw = 3.84 
  Z  = 16 km
  Plane   Strike  Dip  Rake
   NP1      252    58   116
   NP2       30    40    55
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   7.24e+21     66     212
    N   0.00e+00     22      58
    P  -7.24e+21     10     324

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx    -3.77e+21
       Mxy     3.87e+21
       Mxz    -3.27e+21
       Myy    -2.07e+21
       Myz    -6.99e+20
       Mzz     5.84e+21
                                                     
                                                     
                                                     
                                                     
                     --------------                  
                   --------------------              
              -- P ---------------------##           
             ---   ----------------------##          
           ------------------------------####        
          --------------------------------####       
         -------------------##############-####      
        --------------####################-----#     
        -----------#######################------     
       ---------##########################-------    
       ------#############################-------    
       -----#############################--------    
       ---##############   #############---------    
        -############### T #############--------     
        ################   ############---------     
         ############################----------      
          ##########################----------       
           #######################-----------        
             ###################-----------          
              ###############-------------           
                 #######---------------              
                     --------------                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
  5.84e+21  -3.27e+21   6.99e+20 
 -3.27e+21  -3.77e+21  -3.87e+21 
  6.99e+20  -3.87e+21  -2.07e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260928145554/index.html
        

Preferred Solution

The preferred solution from an analysis of the surface-wave spectral amplitude radiation pattern, waveform inversion or first motion observations is

      STK = 30
      DIP = 40
     RAKE = 55
       MW = 3.84
       HS = 16.0

The NDK file is 20260928145554.ndk The waveform inversion is preferred.

Magnitudes

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.

ML Magnitude


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.

Context

The left panel of the next figure presents the focal mechanism for this earthquake (red) in the context of other nearby events (blue) in the SLU Moment Tensor Catalog. The right panel shows the inferred direction of maximum compressive stress and the type of faulting (green is strike-slip, red is normal, blue is thrust; oblique is shown by a combination of colors). Thus context plot is useful for assessing the appropriateness of the moment tensor of this event.

Waveform Inversion using wvfgrd96

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.
Location of broadband stations used for waveform inversion

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 3 
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   250    45   -95   3.40 0.2604
WVFGRD96    2.0    65    45   -90   3.53 0.3358
WVFGRD96    3.0   195    55   -15   3.46 0.2601
WVFGRD96    4.0   190    35    -5   3.51 0.2844
WVFGRD96    5.0   195    35     5   3.53 0.3189
WVFGRD96    6.0    85    80   -70   3.56 0.3607
WVFGRD96    7.0    10    25     0   3.57 0.4005
WVFGRD96    8.0    10    25     0   3.66 0.4302
WVFGRD96    9.0    30    30    45   3.70 0.4765
WVFGRD96   10.0    35    35    55   3.74 0.5231
WVFGRD96   11.0    35    35    55   3.76 0.5663
WVFGRD96   12.0    35    40    60   3.78 0.6019
WVFGRD96   13.0    35    40    60   3.80 0.6290
WVFGRD96   14.0    35    40    60   3.82 0.6467
WVFGRD96   15.0    35    40    60   3.83 0.6563
WVFGRD96   16.0    30    40    55   3.84 0.6586
WVFGRD96   17.0    30    40    50   3.85 0.6547
WVFGRD96   18.0    30    40    50   3.87 0.6456
WVFGRD96   19.0    25    40    50   3.88 0.6317
WVFGRD96   20.0    25    40    45   3.88 0.6142
WVFGRD96   21.0    35    30    65   3.89 0.5937
WVFGRD96   22.0    35    25    65   3.90 0.5751
WVFGRD96   23.0    35    25    65   3.90 0.5547
WVFGRD96   24.0    30    25    60   3.91 0.5334
WVFGRD96   25.0    30    25    60   3.92 0.5113
WVFGRD96   26.0   340    30    20   3.95 0.4897
WVFGRD96   27.0   335    30    15   3.95 0.4731
WVFGRD96   28.0   335    30    15   3.96 0.4547
WVFGRD96   29.0   335    30    15   3.96 0.4344

The best solution is

WVFGRD96   16.0    30    40    55   3.84 0.6586

The mechanism corresponding to the best fit is
Figure 1. Waveform inversion focal mechanism

The best fit as a function of depth is given in the following figure:

Figure 2. Depth sensitivity for waveform mechanism

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:

Assuming only a mislocation, the time shifts are fit to a functional form:

 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.

Velocity Model

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    
Last Changed Mon Sep 28 10:26:01 CDT 2026