Location

Location ANSS

The ANSS event ID is usb000i86c and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usb000i86c/executive.

2013/07/07 08:38:59 36.457 -112.555 5.2 3.5 Arizona

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2013/07/07 08:38:59:0  36.46 -112.56   5.2 3.5 Arizona
 
 Stations used:
   AE.W13A AE.X18A AE.Y14A AZ.KNW AZ.SND AZ.TRO AZ.WMC CI.ADO 
   CI.BC3 CI.BEL CI.BFS CI.DAN CI.FUR CI.GLA CI.GMR CI.GSC 
   CI.HEC CI.IRM CI.MPM CI.MUR CI.PDM CI.PLM CI.RRX CI.SVD 
   CI.SWS CI.TIN CI.TUQ CI.VTV IU.TUC PB.B082A PB.B086A 
   PB.B088A TA.214A TA.R11A TA.S22A TA.W18A TA.Y12C US.DUG 
   US.HWUT US.MVCO US.TPNV US.WUAZ UU.BGU UU.BRPU UU.CCUT 
   UU.HVU UU.KNB UU.LCMT UU.MPU UU.MTPU UU.PKCU UU.PSUT UU.SRU 
   UU.SZCU UU.TCRU UU.TMU 
 
 Filtering commands used:
   cut a -30 a 180
   rtr
   taper w 0.1
   hp c 0.02 n 3 
   lp c 0.08 n 3 
   br c 0.12 0.25 n 4 p 2
 
 Best Fitting Double Couple
  Mo = 2.24e+21 dyne-cm
  Mw = 3.50 
  Z  = 17 km
  Plane   Strike  Dip  Rake
   NP1      111    66   -129
   NP2      355    45   -35
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   2.24e+21     12     229
    N   0.00e+00     35     130
    P  -2.24e+21     52     335

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     2.35e+20
       Mxy     1.39e+21
       Mxz    -1.29e+21
       Myy     1.05e+21
       Myz     1.13e+20
       Mzz    -1.28e+21
                                                     
                                                     
                                                     
                                                     
                     --------######                  
                 --------------########              
              -------------------#########           
             ----------------------########          
           -------------------------#########        
          ------------   ------------#########       
         ------------- P -------------#########      
        #-------------   -------------##########     
        ###----------------------------#########     
       #####---------------------------##########    
       #######-------------------------##########    
       ##########----------------------##########    
       #############-------------------##########    
        ###############----------------#########     
        ####################-----------#########     
         ###########################--######---      
          ###   ######################--------       
           ## T #####################--------        
                ####################-------          
              #####################-------           
                 #################-----              
                     ###########---                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -1.28e+21  -1.29e+21  -1.13e+20 
 -1.29e+21   2.35e+20  -1.39e+21 
 -1.13e+20  -1.39e+21   1.05e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20130707083859/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 = 355
      DIP = 45
     RAKE = -35
       MW = 3.50
       HS = 17.0

The NDK file is 20130707083859.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 a -30 a 180
rtr
taper w 0.1
hp c 0.02 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    0.5   305    50   -90   3.19 0.3116
WVFGRD96    1.0   345    90    -5   3.22 0.3039
WVFGRD96    2.0   170    80   -10   3.29 0.3469
WVFGRD96    3.0   170    75    -5   3.34 0.3453
WVFGRD96    4.0    10    30   -10   3.41 0.3576
WVFGRD96    5.0    10    30   -10   3.41 0.4042
WVFGRD96    6.0     5    35   -15   3.40 0.4310
WVFGRD96    7.0     5    35   -20   3.40 0.4469
WVFGRD96    8.0     5    30   -15   3.45 0.4558
WVFGRD96    9.0     5    35   -15   3.45 0.4654
WVFGRD96   10.0     0    35   -25   3.45 0.4726
WVFGRD96   11.0     0    40   -25   3.45 0.4793
WVFGRD96   12.0    -5    40   -35   3.47 0.4854
WVFGRD96   13.0   355    40   -40   3.48 0.4910
WVFGRD96   14.0   355    45   -35   3.48 0.4959
WVFGRD96   15.0   355    45   -35   3.49 0.4997
WVFGRD96   16.0   355    45   -35   3.49 0.5019
WVFGRD96   17.0   355    45   -35   3.50 0.5026
WVFGRD96   18.0   355    45   -35   3.51 0.5025
WVFGRD96   19.0   355    50   -35   3.53 0.5015
WVFGRD96   20.0   355    50   -35   3.53 0.4994
WVFGRD96   21.0   350    50   -35   3.55 0.4970
WVFGRD96   22.0   350    50   -35   3.56 0.4930
WVFGRD96   23.0   350    50   -35   3.56 0.4876
WVFGRD96   24.0   350    50   -35   3.57 0.4812
WVFGRD96   25.0   350    50   -35   3.58 0.4737
WVFGRD96   26.0   350    50   -35   3.59 0.4652
WVFGRD96   27.0   350    50   -35   3.59 0.4565
WVFGRD96   28.0   350    50   -35   3.60 0.4470
WVFGRD96   29.0   350    50   -35   3.61 0.4377

The best solution is

WVFGRD96   17.0   355    45   -35   3.50 0.5026

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 a -30 a 180
rtr
taper w 0.1
hp c 0.02 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 Fri Apr 26 06:39:12 PM CDT 2024