Location

Location ANSS

The ANSS event ID is ak018coiadru and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak018coiadru/executive.

2018/10/03 03:29:37 64.898 -148.919 19.7 3.9 Alaska

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2018/10/03 03:29:37:0  64.90 -148.92  19.7 3.9 Alaska
 
 Stations used:
   AK.BPAW AK.BWN AK.CCB AK.COLD AK.CUT AK.DHY AK.FYU AK.GHO 
   AK.HDA AK.KNK AK.KTH AK.MCK AK.MLY AK.NEA2 AK.PPD AK.PPLA 
   AK.RC01 AK.RIDG AK.RND AK.SAW AK.SCM AK.SCRK AK.SKN AK.SSN 
   AK.WRH AT.MENT AT.PMR IM.IL31 IU.COLA TA.E23K TA.E24K 
   TA.F20K TA.F21K TA.F24K TA.F25K TA.F26K TA.G19K TA.G21K 
   TA.G23K TA.G24K TA.G27K TA.H19K TA.H21K TA.H23K TA.H24K 
   TA.I20K TA.I23K TA.I26K TA.I28M TA.J18K TA.J19K TA.J20K 
   TA.J25K TA.J26L TA.K20K TA.K27K TA.L26K TA.L27K TA.M19K 
   TA.M20K TA.M22K TA.M26K TA.N25K TA.POKR TA.TOLK US.EGAK 
 
 Filtering commands used:
   cut o DIST/3.3 -20 o DIST/3.3 +60
   rtr
   taper w 0.1
   hp c 0.03 n 3 
   lp c 0.08 n 3 
 
 Best Fitting Double Couple
  Mo = 1.84e+22 dyne-cm
  Mw = 4.11 
  Z  = 19 km
  Plane   Strike  Dip  Rake
   NP1      138    79   123
   NP2      245    35    20
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   1.84e+22     46      82
    N   0.00e+00     33     311
    P  -1.84e+22     26     203

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx    -1.25e+22
       Mxy    -4.11e+21
       Mxz     7.94e+21
       Myy     6.54e+21
       Myz     1.19e+22
       Mzz     5.92e+21
                                                     
                                                     
                                                     
                                                     
                     --------------                  
                 ----------------------              
              ----------------------------           
             ##------------###########-----          
           #####------#####################--        
          #######--##########################-       
         #######--#############################      
        ######-----#############################     
        #####--------###########################     
       #####----------###############   #########    
       ####------------############## T #########    
       ###---------------############   #########    
       ###-----------------######################    
        #-------------------####################     
        #---------------------##################     
         -----------------------###############      
          ------------------------############       
           ---------   -------------#########        
             ------- P ----------------####          
              ------   -------------------           
                 ----------------------              
                     --------------                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
  5.92e+21   7.94e+21  -1.19e+22 
  7.94e+21  -1.25e+22   4.11e+21 
 -1.19e+22   4.11e+21   6.54e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20181003032937/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 = 245
      DIP = 35
     RAKE = 20
       MW = 4.11
       HS = 19.0

The NDK file is 20181003032937.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.

mLg Magnitude


Left: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated. Right: residuals as a function of distance and azimuth.

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.

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 -20 o DIST/3.3 +60
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.08 n 3 
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   350    45   -90   3.62 0.2697
WVFGRD96    2.0   175    45   -90   3.76 0.3802
WVFGRD96    3.0     5    40   -75   3.81 0.3315
WVFGRD96    4.0   240    50    15   3.78 0.3305
WVFGRD96    5.0   240    35    10   3.83 0.3716
WVFGRD96    6.0   240    30    10   3.85 0.4275
WVFGRD96    7.0   240    35    10   3.87 0.4785
WVFGRD96    8.0   240    30    10   3.95 0.5182
WVFGRD96    9.0   245    30    15   3.96 0.5686
WVFGRD96   10.0   245    30    20   3.98 0.6132
WVFGRD96   11.0   245    30    20   4.00 0.6520
WVFGRD96   12.0   245    35    20   4.02 0.6860
WVFGRD96   13.0   245    35    20   4.04 0.7148
WVFGRD96   14.0   250    35    25   4.05 0.7381
WVFGRD96   15.0   245    35    20   4.06 0.7569
WVFGRD96   16.0   245    35    20   4.08 0.7711
WVFGRD96   17.0   245    35    20   4.09 0.7811
WVFGRD96   18.0   245    35    20   4.10 0.7870
WVFGRD96   19.0   245    35    20   4.11 0.7888
WVFGRD96   20.0   245    35    20   4.12 0.7882
WVFGRD96   21.0   245    35    20   4.14 0.7840
WVFGRD96   22.0   245    35    20   4.15 0.7778
WVFGRD96   23.0   245    35    20   4.15 0.7697
WVFGRD96   24.0   245    35    20   4.16 0.7588
WVFGRD96   25.0   245    35    20   4.17 0.7465
WVFGRD96   26.0   245    35    20   4.17 0.7319
WVFGRD96   27.0   245    35    20   4.18 0.7162
WVFGRD96   28.0   245    35    20   4.18 0.6978
WVFGRD96   29.0   245    35    20   4.19 0.6790

The best solution is

WVFGRD96   19.0   245    35    20   4.11 0.7888

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 -20 o DIST/3.3 +60
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.08 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 Fri Apr 26 02:48:19 AM CDT 2024