Location

Location ANSS

The ANSS event ID is ak0153yawb1o and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0153yawb1o/executive.

2015/03/27 04:50:05 58.030 -157.060 14.0 4.3 Alaska

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2015/03/27 04:50:05:0  58.03 -157.06  14.0 4.3 Alaska
 
 Stations used:
   AK.CNP AK.SII AK.SKN AK.SSN AT.CHGN AT.OHAK AT.SDPT AT.SVW2 
   II.KDAK TA.O22K 
 
 Filtering commands used:
   cut o DIST/3.3 -30 o DIST/3.3 +70
   rtr
   taper w 0.1
   hp c 0.02 n 3 
   lp c 0.05 n 3 
 
 Best Fitting Double Couple
  Mo = 2.60e+22 dyne-cm
  Mw = 4.21 
  Z  = 18 km
  Plane   Strike  Dip  Rake
   NP1      282    71   -159
   NP2      185    70   -20
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   2.60e+22      1      53
    N   0.00e+00     62     322
    P  -2.60e+22     28     144

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx    -3.94e+21
       Mxy     2.21e+22
       Mxz     8.92e+21
       Myy     9.66e+21
       Myz    -6.06e+21
       Mzz    -5.72e+21
                                                     
                                                     
                                                     
                                                     
                     --------######                  
                 -----------###########              
              -------------###############           
             -------------#################          
           --------------################## T        
          ---------------##################          
         ---------------#######################      
        ----------------########################     
        ###############------###################     
       ################-------------#############    
       ################-----------------#########    
       ################---------------------#####    
       ################------------------------##    
        ###############-------------------------     
        ###############-------------------------     
         ##############------------------------      
          #############------------   --------       
           ############------------ P -------        
             ###########-----------   -----          
              ##########------------------           
                 ########--------------              
                     #####---------                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -5.72e+21   8.92e+21   6.06e+21 
  8.92e+21  -3.94e+21  -2.21e+22 
  6.06e+21  -2.21e+22   9.66e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150327045005/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 = 185
      DIP = 70
     RAKE = -20
       MW = 4.21
       HS = 18.0

The NDK file is 20150327045005.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.

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 +70
rtr
taper w 0.1
hp c 0.02 n 3 
lp c 0.05 n 3 
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   180    70    20   3.92 0.2112
WVFGRD96    2.0     0    70    15   3.98 0.2496
WVFGRD96    3.0   180    70    20   4.03 0.2649
WVFGRD96    4.0     0    85    25   4.04 0.2750
WVFGRD96    5.0   180    90   -25   4.06 0.2849
WVFGRD96    6.0     0    90    25   4.08 0.2943
WVFGRD96    7.0     0    90    20   4.09 0.3031
WVFGRD96    8.0     0    90    30   4.13 0.3118
WVFGRD96    9.0   180    90   -30   4.14 0.3163
WVFGRD96   10.0   180    90   -25   4.15 0.3199
WVFGRD96   11.0   180    60   -20   4.16 0.3237
WVFGRD96   12.0   180    60   -20   4.17 0.3300
WVFGRD96   13.0   180    65   -25   4.18 0.3356
WVFGRD96   14.0   180    65   -25   4.19 0.3394
WVFGRD96   15.0   180    65   -20   4.20 0.3423
WVFGRD96   16.0   180    65   -20   4.21 0.3440
WVFGRD96   17.0   185    65   -20   4.20 0.3446
WVFGRD96   18.0   185    70   -20   4.21 0.3451
WVFGRD96   19.0   185    70   -20   4.22 0.3450
WVFGRD96   20.0   185    70   -20   4.23 0.3441
WVFGRD96   21.0   185    70   -20   4.23 0.3423
WVFGRD96   22.0   185    70   -20   4.24 0.3405
WVFGRD96   23.0   190    75    20   4.25 0.3401
WVFGRD96   24.0   190    80    20   4.25 0.3392
WVFGRD96   25.0   190    80    20   4.26 0.3381
WVFGRD96   26.0   190    80    20   4.27 0.3365
WVFGRD96   27.0   190    80    20   4.28 0.3346
WVFGRD96   28.0   190    80    20   4.29 0.3322
WVFGRD96   29.0   190    80    20   4.30 0.3293

The best solution is

WVFGRD96   18.0   185    70   -20   4.21 0.3451

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 +70
rtr
taper w 0.1
hp c 0.02 n 3 
lp c 0.05 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 02:57:34 PM CDT 2024