Location

Location ANSS

The ANSS event ID is ak0193hwnu43 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0193hwnu43/executive.

2019/03/17 13:13:18 69.528 -144.202 5.0 3.4 Alaska

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2019/03/17 13:13:18:0  69.53 -144.20   5.0 3.4 Alaska
 
 Stations used:
   AK.COLD AK.FYU AK.PPD TA.C23K TA.C24K TA.C26K TA.C27K 
   TA.D23K TA.D28M TA.E23K TA.E25K TA.E27K TA.E28M TA.E29M 
   TA.F24K TA.F25K TA.F26K TA.F30M TA.G23K TA.G24K TA.G25K 
   TA.G26K TA.G27K TA.G30M TA.H24K TA.H27K TA.I26K TA.I27K 
   TA.TOLK 
 
 Filtering commands used:
   cut o DIST/3.3 -30 o DIST/3.3 +50
   rtr
   taper w 0.1
   hp c 0.03 n 3 
   lp c 0.08 n 3 
   br c 0.12 0.25 n 4 p 2
 
 Best Fitting Double Couple
  Mo = 2.66e+21 dyne-cm
  Mw = 3.55 
  Z  = 8 km
  Plane   Strike  Dip  Rake
   NP1      200    75    35
   NP2      100    56   162
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   2.66e+21     35      65
    N   0.00e+00     52     220
    P  -2.66e+21     12     326

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx    -1.44e+21
       Mxy     1.86e+21
       Mxz     7.80e+19
       Myy     6.79e+20
       Myz     1.43e+21
       Mzz     7.63e+20
                                                     
                                                     
                                                     
                                                     
                     --------------                  
                   --------------######              
              -- P -------------##########           
             ---   -----------#############          
           ------------------################        
          ------------------##################       
         ------------------############   #####      
        ------------------############# T ######     
        ------------------#############   ######     
       #-----------------########################    
       ##---------------#########################    
       ####-------------#########################    
       ######----------##########################    
        ########-------########################-     
        ############--######################----     
         #############----############---------      
          ###########-------------------------       
           ##########------------------------        
             ########----------------------          
              #######---------------------           
                 ####------------------              
                     --------------                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
  7.63e+20   7.80e+19  -1.43e+21 
  7.80e+19  -1.44e+21  -1.86e+21 
 -1.43e+21  -1.86e+21   6.79e+20 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20190317131318/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 = 200
      DIP = 75
     RAKE = 35
       MW = 3.55
       HS = 8.0

The NDK file is 20190317131318.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 -30 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.08 n 3 
br c 0.12 0.25 n 4 p 2
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   195    90     5   3.29 0.5252
WVFGRD96    2.0    15    80   -15   3.38 0.6070
WVFGRD96    3.0    15    80   -15   3.41 0.6200
WVFGRD96    4.0   195    90    30   3.46 0.6326
WVFGRD96    5.0   200    75    35   3.49 0.6531
WVFGRD96    6.0   200    75    30   3.50 0.6724
WVFGRD96    7.0   200    75    30   3.52 0.6825
WVFGRD96    8.0   200    75    35   3.55 0.6872
WVFGRD96    9.0   200    75    35   3.56 0.6863
WVFGRD96   10.0   200    80    35   3.57 0.6830
WVFGRD96   11.0   200    80    30   3.57 0.6790
WVFGRD96   12.0   195    90    25   3.58 0.6740
WVFGRD96   13.0   195    90    25   3.59 0.6698
WVFGRD96   14.0   195    90    25   3.60 0.6651
WVFGRD96   15.0   195    90    25   3.61 0.6590
WVFGRD96   16.0   195    90    25   3.62 0.6521
WVFGRD96   17.0   195    90    25   3.63 0.6445
WVFGRD96   18.0    15    90   -25   3.64 0.6358
WVFGRD96   19.0    15    90   -25   3.65 0.6254
WVFGRD96   20.0    15    90   -25   3.66 0.6144
WVFGRD96   21.0    15    90   -25   3.67 0.6028
WVFGRD96   22.0    15    85   -20   3.67 0.5901
WVFGRD96   23.0    15    85   -20   3.68 0.5771
WVFGRD96   24.0   195    90    25   3.69 0.5614
WVFGRD96   25.0   195    90    20   3.70 0.5464
WVFGRD96   26.0   195    90    20   3.70 0.5315
WVFGRD96   27.0    15    85   -20   3.71 0.5185
WVFGRD96   28.0   195    90    20   3.72 0.4998
WVFGRD96   29.0    15    85   -20   3.73 0.4871

The best solution is

WVFGRD96    8.0   200    75    35   3.55 0.6872

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 -30 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.08 n 3 
br c 0.12 0.25 n 4 p 2
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 Thu Apr 25 09:48:40 AM CDT 2024