Location

Location ANSS

2019/11/18 19:51:28 66.303 -157.167 9.7 3.9 Alaska

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2019/11/18 19:51:28:0  66.30 -157.17   9.7 3.9 Alaska
 
 Stations used:
   AK.ANM AK.BPAW AK.BWN AK.COLD AK.H21K AK.H22K AK.I23K 
   AK.J17K AK.J20K AK.KTH AK.MLY AK.NEA2 AK.RDOG TA.C16K 
   TA.C19K TA.D20K TA.D22K TA.E18K TA.G19K TA.G23K TA.G24K 
   TA.I17K TA.TOLK 
 
 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 = 1.30e+22 dyne-cm
  Mw = 4.01 
  Z  = 11 km
  Plane   Strike  Dip  Rake
   NP1      330    70   -45
   NP2       79    48   -153
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   1.30e+22     13      29
    N   0.00e+00     42     131
    P  -1.30e+22     45     285

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     8.98e+21
       Mxy     6.89e+21
       Mxz     8.00e+20
       Myy    -3.06e+21
       Myz     7.69e+21
       Mzz    -5.92e+21
                                                     
                                                     
                                                     
                                                     
                     ##############                  
                 -#################   #              
              -------############## T ####           
             -----------###########   #####          
           --------------####################        
          -----------------###################       
         --------------------##################      
        ----------------------##################     
        --------   ------------#################     
       --------- P -------------################-    
       ---------   --------------##############--    
       ---------------------------############---    
       ----------------------------#########-----    
        ----------------------------######------     
        ##---------------------------###--------     
         ####-----------------------#----------      
          ########------------########--------       
           ###########################-------        
             #########################-----          
              ########################----           
                 #####################-              
                     ##############                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -5.92e+21   8.00e+20  -7.69e+21 
  8.00e+20   8.98e+21  -6.89e+21 
 -7.69e+21  -6.89e+21  -3.06e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20191118195128/index.html
        

Preferred Solution

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

      STK = 330
      DIP = 70
     RAKE = -45
       MW = 4.01
       HS = 11.0

The NDK file is 20191118195128.ndk The waveform inversion is preferred.

Moment Tensor Comparison

The following compares this source inversion to others
SLU
 USGS/SLU Moment Tensor Solution
 ENS  2019/11/18 19:51:28:0  66.30 -157.17   9.7 3.9 Alaska
 
 Stations used:
   AK.ANM AK.BPAW AK.BWN AK.COLD AK.H21K AK.H22K AK.I23K 
   AK.J17K AK.J20K AK.KTH AK.MLY AK.NEA2 AK.RDOG TA.C16K 
   TA.C19K TA.D20K TA.D22K TA.E18K TA.G19K TA.G23K TA.G24K 
   TA.I17K TA.TOLK 
 
 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 = 1.30e+22 dyne-cm
  Mw = 4.01 
  Z  = 11 km
  Plane   Strike  Dip  Rake
   NP1      330    70   -45
   NP2       79    48   -153
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   1.30e+22     13      29
    N   0.00e+00     42     131
    P  -1.30e+22     45     285

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     8.98e+21
       Mxy     6.89e+21
       Mxz     8.00e+20
       Myy    -3.06e+21
       Myz     7.69e+21
       Mzz    -5.92e+21
                                                     
                                                     
                                                     
                                                     
                     ##############                  
                 -#################   #              
              -------############## T ####           
             -----------###########   #####          
           --------------####################        
          -----------------###################       
         --------------------##################      
        ----------------------##################     
        --------   ------------#################     
       --------- P -------------################-    
       ---------   --------------##############--    
       ---------------------------############---    
       ----------------------------#########-----    
        ----------------------------######------     
        ##---------------------------###--------     
         ####-----------------------#----------      
          ########------------########--------       
           ###########################-------        
             #########################-----          
              ########################----           
                 #####################-              
                     ##############                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -5.92e+21   8.00e+20  -7.69e+21 
  8.00e+20   8.98e+21  -6.89e+21 
 -7.69e+21  -6.89e+21  -3.06e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20191118195128/index.html
	

Magnitudes

mLg Magnitude


(a) mLg computed using the IASPEI formula; (b) mLg residuals ; the values used for the trimmed mean are indicated.

ML Magnitude


(a) ML computed using the IASPEI formula for Horizontal components; (b) 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.


(a) ML computed using the IASPEI formula for Vertical components (research); (b) 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.

Context

The next figure presents the focal mechanism for this earthquake (red) in the context of other events (blue) in the SLU Moment Tensor Catalog which are within ± 0.5 degrees of the new event. This comparison is shown in the left panel of the figure. 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).

Waveform Inversion using wvfgrd96

The focal mechanism was determined using broadband seismic waveforms. The location of the event and the and stations used for 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 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 from 0.5 to 19 km depth are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   335    85   -10   3.59 0.2994
WVFGRD96    2.0   335    75   -25   3.71 0.3383
WVFGRD96    3.0   335    80   -35   3.77 0.3341
WVFGRD96    4.0   175    65    45   3.82 0.3550
WVFGRD96    5.0   270    30    40   3.87 0.3867
WVFGRD96    6.0   325    65   -50   3.88 0.4331
WVFGRD96    7.0   325    65   -50   3.90 0.4693
WVFGRD96    8.0   325    65   -55   3.98 0.5007
WVFGRD96    9.0   325    65   -55   3.99 0.5234
WVFGRD96   10.0   325    65   -50   3.99 0.5341
WVFGRD96   11.0   330    70   -45   4.01 0.5376
WVFGRD96   12.0   330    70   -45   4.02 0.5370
WVFGRD96   13.0   330    70   -40   4.03 0.5327
WVFGRD96   14.0   330    70   -40   4.04 0.5245
WVFGRD96   15.0   330    70   -40   4.05 0.5127
WVFGRD96   16.0   330    70   -40   4.06 0.5001
WVFGRD96   17.0   150    70   -45   4.07 0.4923
WVFGRD96   18.0   150    70   -45   4.08 0.4809
WVFGRD96   19.0   150    70   -45   4.09 0.4682
WVFGRD96   20.0   150    70   -45   4.10 0.4531
WVFGRD96   21.0   150    70   -45   4.11 0.4384
WVFGRD96   22.0   150    70   -45   4.12 0.4215
WVFGRD96   23.0   150    70   -45   4.12 0.4040
WVFGRD96   24.0   150    70   -40   4.13 0.3865
WVFGRD96   25.0   150    65   -40   4.13 0.3699
WVFGRD96   26.0   150    65   -40   4.13 0.3544
WVFGRD96   27.0   150    65   -40   4.13 0.3390
WVFGRD96   28.0   150    65   -40   4.14 0.3241
WVFGRD96   29.0   150    60   -40   4.14 0.3099

The best solution is

WVFGRD96   11.0   330    70   -45   4.01 0.5376

The mechanism correspond 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 and because the velocity model used in the predictions may not be perfect. 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.
Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to thewavefroms. 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.

Discussion

Acknowledgements

Thanks also to the many seismic network operators whose dedication make this effort possible: University of Nevada Reno, University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureau of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Oklahoma Geological Survey, TexNet, the Iris stations, the Transportable Array of EarthScope and other networks.

Velocity Model

The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:

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    

Quality Control

Here we tabulate the reasons for not using certain digital data sets

The following stations did not have a valid response files:

Last Changed Mon Nov 18 14:26:59 CST 2019