Location

Location ANSS

The ANSS event ID is tx2025deqh and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/tx2025deqh/executive.

2025/02/15 05:23:21 31.661 -104.180 6.6 5.0 Texas

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2025/02/15 05:23:21:0  31.66 -104.18   6.6 5.0 Texas
 
 Stations used:
   4O.AT01 4O.BB01 4O.BP01 4O.CT01 4O.CT02 4O.CV01 4O.CW01 
   4O.DB02 4O.DB03 4O.DB04 4O.EE02 4O.EE03 4O.EE04 4O.GV02 
   4O.GV03 4O.GV04 4O.LWM1 4O.LWM2 4O.LWM3 4O.MBBB2 4O.MBBB5 
   4O.MG01 4O.MID01 4O.MID02 4O.MID03 4O.NGL01 4O.NGL02 
   4O.OE01 4O.OE02 4O.PL01 4O.PR01 4O.SA07 4O.SA09 4O.SD01 
   4O.SE01 4O.SM01 4O.SM02 4O.SM03 4O.SM04 4O.SM05 4O.VW01 
   4O.WB02 4O.WB03 4O.WB05 4O.WB06 
 
 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 0.07 n 3 
 
 Best Fitting Double Couple
  Mo = 2.92e+23 dyne-cm
  Mw = 4.91 
  Z  = 10 km
  Plane   Strike  Dip  Rake
   NP1      246    55   -87
   NP2       60    35   -95
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   2.92e+23     10     334
    N   0.00e+00      3      64
    P  -2.92e+23     80     170

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     2.17e+23
       Mxy    -1.11e+23
       Mxz     9.65e+22
       Myy     5.56e+22
       Myz    -3.17e+22
       Mzz    -2.73e+23
                                                     
                                                     
                                                     
                                                     
                     ##############                  
                 # T ##################              
              ####   #####################           
             ##############################          
           ##################################        
          #####################------------###       
         ################---------------------#      
        #############-------------------------##     
        ##########----------------------------##     
       #########------------------------------###    
       #######-------------------------------####    
       ######--------------   ---------------####    
       ####---------------- P --------------#####    
        ##-----------------   -------------#####     
        ##-------------------------------#######     
         ------------------------------########      
          ---------------------------#########       
           #----------------------###########        
             ###--------------#############          
              ############################           
                 ######################              
                     ##############                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -2.73e+23   9.65e+22   3.17e+22 
  9.65e+22   2.17e+23   1.11e+23 
  3.17e+22   1.11e+23   5.56e+22 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20250215052321/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 = 60
      DIP = 35
     RAKE = -95
       MW = 4.91
       HS = 10.0

The NDK file is 20250215052321.ndk The waveform inversion is preferred.

Moment Tensor Comparison

The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
SLU
USGSMWR
USGSW
 USGS/SLU Moment Tensor Solution
 ENS  2025/02/15 05:23:21:0  31.66 -104.18   6.6 5.0 Texas
 
 Stations used:
   4O.AT01 4O.BB01 4O.BP01 4O.CT01 4O.CT02 4O.CV01 4O.CW01 
   4O.DB02 4O.DB03 4O.DB04 4O.EE02 4O.EE03 4O.EE04 4O.GV02 
   4O.GV03 4O.GV04 4O.LWM1 4O.LWM2 4O.LWM3 4O.MBBB2 4O.MBBB5 
   4O.MG01 4O.MID01 4O.MID02 4O.MID03 4O.NGL01 4O.NGL02 
   4O.OE01 4O.OE02 4O.PL01 4O.PR01 4O.SA07 4O.SA09 4O.SD01 
   4O.SE01 4O.SM01 4O.SM02 4O.SM03 4O.SM04 4O.SM05 4O.VW01 
   4O.WB02 4O.WB03 4O.WB05 4O.WB06 
 
 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 0.07 n 3 
 
 Best Fitting Double Couple
  Mo = 2.92e+23 dyne-cm
  Mw = 4.91 
  Z  = 10 km
  Plane   Strike  Dip  Rake
   NP1      246    55   -87
   NP2       60    35   -95
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   2.92e+23     10     334
    N   0.00e+00      3      64
    P  -2.92e+23     80     170

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     2.17e+23
       Mxy    -1.11e+23
       Mxz     9.65e+22
       Myy     5.56e+22
       Myz    -3.17e+22
       Mzz    -2.73e+23
                                                     
                                                     
                                                     
                                                     
                     ##############                  
                 # T ##################              
              ####   #####################           
             ##############################          
           ##################################        
          #####################------------###       
         ################---------------------#      
        #############-------------------------##     
        ##########----------------------------##     
       #########------------------------------###    
       #######-------------------------------####    
       ######--------------   ---------------####    
       ####---------------- P --------------#####    
        ##-----------------   -------------#####     
        ##-------------------------------#######     
         ------------------------------########      
          ---------------------------#########       
           #----------------------###########        
             ###--------------#############          
              ############################           
                 ######################              
                     ##############                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
 -2.73e+23   9.65e+22   3.17e+22 
  9.65e+22   2.17e+23   1.11e+23 
  3.17e+22   1.11e+23   5.56e+22 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20250215052321/index.html
	
Regional Moment Tensor (Mwr)
Moment 2.599e+16 N-m
Magnitude 4.88 Mwr
Depth 9.0 km
Percent DC 96%
Half Duration
-
Catalog US
Data Source US
Contributor US
Nodal Planes
Plane	Strike	Dip	Rake
NP1	52	34	-105
NP2	249	58	-80
Principal Axes
Axis	Value	Plunge	Azimuth
T	2.625e+16	12	332
N	-0.053e+16	8	64
P	-2.573e+16	75	187

        
W-phase Moment Tensor (Mww)
Moment 2.833e+16 N-m
Magnitude 4.90 Mww
Depth 11.5 km
Percent DC 63%
Half Duration 0.50 s
Catalog US
Data Source US
Contributor US
Nodal Planes
Plane	Strike	Dip	Rake
NP1	78	59	-59
NP2	209	43	-130
Principal Axes
Axis	Value	Plunge	Azimuth
T	2.505e+16	9	146
N	0.569e+16	26	240
P	-3.074e+16	62	39

        

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 0.07 n 3 
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   240    45   -85   4.51 0.1941
WVFGRD96    2.0   240    45   -90   4.64 0.2536
WVFGRD96    3.0    75    50   -70   4.68 0.2443
WVFGRD96    4.0    80    20   -65   4.76 0.2940
WVFGRD96    5.0    75    20   -75   4.78 0.3458
WVFGRD96    6.0    70    25   -80   4.79 0.3870
WVFGRD96    7.0    65    30   -90   4.82 0.4224
WVFGRD96    8.0    60    30   -95   4.89 0.4553
WVFGRD96    9.0    65    30   -90   4.90 0.4781
WVFGRD96   10.0    60    35   -95   4.91 0.4893
WVFGRD96   11.0   245    55   -90   4.92 0.4853
WVFGRD96   12.0   245    55   -90   4.92 0.4727
WVFGRD96   13.0   240    55   -95   4.92 0.4527
WVFGRD96   14.0    65    40   -85   4.91 0.4291
WVFGRD96   15.0    70    40   -80   4.91 0.4058
WVFGRD96   16.0    70    40   -80   4.91 0.3817
WVFGRD96   17.0    80    35   -70   4.90 0.3576
WVFGRD96   18.0    80    35   -70   4.90 0.3387
WVFGRD96   19.0    80    35   -70   4.90 0.3213
WVFGRD96   20.0    85    35   -65   4.89 0.3060
WVFGRD96   21.0    85    35   -65   4.90 0.2959
WVFGRD96   22.0    95    60   -35   4.91 0.2834
WVFGRD96   23.0    95    60   -35   4.92 0.2743
WVFGRD96   24.0   100    65   -25   4.92 0.2658
WVFGRD96   25.0   100    65   -25   4.92 0.2585
WVFGRD96   26.0   100    65   -20   4.92 0.2513
WVFGRD96   27.0   100    65   -20   4.93 0.2445
WVFGRD96   28.0   215    70    50   4.93 0.2409
WVFGRD96   29.0   215    70    50   4.93 0.2378

The best solution is

WVFGRD96   10.0    60    35   -95   4.91 0.4893

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 0.07 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 Sat Feb 15 08:40:13 CST 2025