Location

Location ANSS

The ANSS event ID is nm608392 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/nm608392/executive.

2011/02/18 04:59:50 35.257 -92.370 5.0 3.9 Arkansas

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2011/02/18 04:59:50:0  35.26  -92.37   5.0 3.9 Arkansas
 
 Stations used:
   AG.FCAR AG.HHAR AG.LCAR AG.WHAR AG.WLAR NM.MGMO NM.MPH 
   NM.OLIL NM.PBMO NM.PVMO NM.SIUC NM.SLM NM.UALR NM.USIN 
   NM.UTMT NM.X102 NM.X201 TA.137A TA.138A TA.139A TA.141A 
   TA.238A TA.240A TA.O38A TA.O39A TA.P40A TA.Q39A TA.Q40A 
   TA.R35A TA.R36A TA.R37A TA.R40A TA.S34A TA.S35A TA.S36A 
   TA.S38A TA.S39A TA.S40A TA.T34A TA.T35A TA.T36A TA.T37A 
   TA.T38A TA.T40A TA.TUL1 TA.U34A TA.U35A TA.U36A TA.U38A 
   TA.U39A TA.U40A TA.V33A TA.V34A TA.V35A TA.V36A TA.V37A 
   TA.V38A TA.V39A TA.W34A TA.W35A TA.W36A TA.W37B TA.W39A 
   TA.W40A TA.X34A TA.X36A TA.X37A TA.X38A TA.X39A TA.X40A 
   TA.Y36A TA.Y37A TA.Y38A TA.Y39A TA.Y40A TA.Z38A TA.Z39A 
   TA.Z40A US.KSU1 US.LRAL US.MIAR US.OXF 
 
 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 
   br c 0.12 0.25 n 4 p 2
 
 Best Fitting Double Couple
  Mo = 7.00e+21 dyne-cm
  Mw = 3.83 
  Z  = 4 km
  Plane   Strike  Dip  Rake
   NP1      202    85   -160
   NP2      110    70    -5
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   7.00e+21     11     334
    N   0.00e+00     69     214
    P  -7.00e+21     17      68

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     4.56e+21
       Mxy    -4.89e+21
       Mxz     3.76e+20
       Myy    -4.17e+21
       Myz    -2.40e+21
       Mzz    -3.92e+20
                                                     
                                                     
                                                     
                                                     
                     ##############                  
                 # T ##############----              
              ####   #############--------           
             ####################----------          
           #####################-------------        
          #####################---------------       
         #####################-------------   -      
        -####################-------------- P --     
        ---##################--------------   --     
       ------###############---------------------    
       --------############----------------------    
       -----------########-----------------------    
       --------------#####-----------------------    
        -----------------#----------------------     
        ----------------########----------------     
         ---------------#######################      
          -------------#######################       
           -----------#######################        
             ---------#####################          
              -------#####################           
                 ----##################              
                     ##############                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -3.92e+20   3.76e+20   2.40e+21 
  3.76e+20   4.56e+21   4.89e+21 
  2.40e+21   4.89e+21  -4.17e+21 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20110218045950/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 = 110
      DIP = 70
     RAKE = -5
       MW = 3.83
       HS = 4.0

The NDK file is 20110218045950.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 -40 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.10 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   110    90    25   3.65 0.5500
WVFGRD96    1.0   285    75   -35   3.72 0.5801
WVFGRD96    2.0   110    55     0   3.79 0.6298
WVFGRD96    3.0   110    60    -5   3.83 0.6587
WVFGRD96    4.0   110    70    -5   3.83 0.6630
WVFGRD96    5.0   110    75    -5   3.85 0.6513
WVFGRD96    6.0   290    90    10   3.85 0.6286
WVFGRD96    7.0   295    75     5   3.85 0.6176
WVFGRD96    8.0   295    70     5   3.87 0.6117
WVFGRD96    9.0   295    70     5   3.89 0.6032
WVFGRD96   10.0   295    65     5   3.91 0.5936
WVFGRD96   11.0   295    65     5   3.92 0.5791
WVFGRD96   12.0   295    60     5   3.94 0.5646
WVFGRD96   13.0   290    65     5   3.94 0.5516
WVFGRD96   14.0   290    65     5   3.95 0.5403
WVFGRD96   15.0   290    65     5   3.96 0.5297
WVFGRD96   16.0   290    65     5   3.96 0.5198
WVFGRD96   17.0   290    65     5   3.97 0.5114
WVFGRD96   18.0   290    65     5   3.98 0.5032
WVFGRD96   19.0   290    65     5   3.98 0.4955
WVFGRD96   20.0   290    60     5   4.00 0.4874
WVFGRD96   21.0   290    60     5   4.01 0.4799
WVFGRD96   22.0   290    60     5   4.01 0.4727
WVFGRD96   23.0   290    60     5   4.02 0.4657
WVFGRD96   24.0   290    60     5   4.03 0.4588
WVFGRD96   25.0   290    60     5   4.03 0.4522
WVFGRD96   26.0   290    55     5   4.04 0.4457
WVFGRD96   27.0   290    55     5   4.05 0.4402
WVFGRD96   28.0   290    55     5   4.06 0.4346
WVFGRD96   29.0   290    55     5   4.06 0.4293

The best solution is

WVFGRD96    4.0   110    70    -5   3.83 0.6630

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 -40 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.10 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 CUS.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
CUS Model with Q from simple gamma values
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
  1.0000  5.0000  2.8900  2.5000 0.172E-02 0.387E-02 0.00  0.00  1.00  1.00 
  9.0000  6.1000  3.5200  2.7300 0.160E-02 0.363E-02 0.00  0.00  1.00  1.00 
 10.0000  6.4000  3.7000  2.8200 0.149E-02 0.336E-02 0.00  0.00  1.00  1.00 
 20.0000  6.7000  3.8700  2.9020 0.000E-04 0.000E-04 0.00  0.00  1.00  1.00 
  0.0000  8.1500  4.7000  3.3640 0.194E-02 0.431E-02 0.00  0.00  1.00  1.00 
Last Changed Sat Apr 27 11:42:13 AM CDT 2024