Location

Location ANSS

The ANSS event ID is tx2024ejzm and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/tx2024ejzm/executive.

2024/03/03 09:15:23 31.611 -103.990 8.4 3.9 Texas

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2024/03/03 09:15:23:0 31.61 -103.99 8.4 3.9 Texas Stations used: 4O.DB02 4O.DB04 4O.LWM2 4O.MBBB2 4O.MID01 4O.MID02 4O.MID03 4O.SA02 4O.SA06 4O.SA07 4O.SA09 4O.WB02 4O.WB05 4O.WB06 4O.WB08 4O.WB09 4T.NM01 4T.NM02 4T.NM03 TX.ALPN TX.MB01 TX.MB02 TX.MB07 TX.MB08 TX.MB09 TX.MB10 TX.MB18 TX.MB25 TX.MNHN TX.ODSA TX.PB01 TX.PB03 TX.PB04 TX.PB05 TX.PB07 TX.PB09 TX.PB10 TX.PB11 TX.PB12 TX.PB13 TX.PB16 TX.PB17 TX.PB18 TX.PB19 TX.PB21 TX.PB22 TX.PB28 TX.PB30 TX.PB35 TX.PB37 TX.PB38 TX.PB44 TX.PB46 TX.PB47 TX.PB51 TX.PCOS TX.PECS 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 Best Fitting Double Couple Mo = 1.35e+22 dyne-cm Mw = 4.02 Z = 11 km Plane Strike Dip Rake NP1 94 76 -133 NP2 350 45 -20 Principal Axes: Axis Value Plunge Azimuth T 1.35e+22 19 215 N 0.00e+00 42 107 P -1.35e+22 42 324 Moment Tensor: (dyne-cm) Component Value Mxx 3.20e+21 Mxy 9.21e+21 Mxz -8.83e+21 Myy 1.41e+21 Myz 1.56e+21 Mzz -4.61e+21 ------######## -------------######### ------------------########## ---------------------######### -------- -------------########## --------- P --------------########## ---------- ---------------########## ------------------------------########## ------------------------------########## --------------------------------########## ##------------------------------########## ######--------------------------########## ##############------------------######---- ###############################--------- ###############################--------- ##############################-------- ############################-------- ###### ##################------- #### T #################------ ### ################------ ##################---- ############-- Global CMT Convention Moment Tensor: R T P -4.61e+21 -8.83e+21 -1.56e+21 -8.83e+21 3.20e+21 -9.21e+21 -1.56e+21 -9.21e+21 1.41e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20240303091523/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 = 350
      DIP = 45
     RAKE = -20
       MW = 4.02
       HS = 11.0

The NDK file is 20240303091523.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 M_L by application of the respective IASPEI formulae. As a research study, the linear distance term of the IASPEI formula for M_L is adjusted to remove a linear distance trend in residuals to give a regionally defined M_L. The defined M_L 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

The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   350    80     0   3.50 0.2431
WVFGRD96    2.0    -5    75    10   3.65 0.3268
WVFGRD96    3.0   350    40   -10   3.78 0.3692
WVFGRD96    4.0   345    35   -20   3.84 0.4502
WVFGRD96    5.0   345    40   -25   3.86 0.5151
WVFGRD96    6.0   345    40   -30   3.89 0.5602
WVFGRD96    7.0   345    40   -30   3.91 0.5898
WVFGRD96    8.0   345    40   -30   3.98 0.6086
WVFGRD96    9.0   345    40   -30   3.99 0.6253
WVFGRD96   10.0   345    40   -30   4.01 0.6328
WVFGRD96   11.0   350    45   -20   4.02 0.6344
WVFGRD96   12.0   350    45   -20   4.03 0.6325
WVFGRD96   13.0   350    45   -20   4.05 0.6253
WVFGRD96   14.0   350    45   -20   4.06 0.6133
WVFGRD96   15.0   350    45   -20   4.07 0.5987
WVFGRD96   16.0   355    45   -10   4.08 0.5822
WVFGRD96   17.0   355    50    -5   4.09 0.5657
WVFGRD96   18.0    -5    50    -5   4.09 0.5481
WVFGRD96   19.0    -5    50    -5   4.10 0.5292
WVFGRD96   20.0    -5    50    -5   4.11 0.5104
WVFGRD96   21.0     0    50    10   4.12 0.4933
WVFGRD96   22.0     0    50    10   4.12 0.4769
WVFGRD96   23.0     0    50    10   4.13 0.4610
WVFGRD96   24.0     0    50    10   4.13 0.4451
WVFGRD96   25.0     0    50    15   4.14 0.4305
WVFGRD96   26.0     5    45    20   4.14 0.4164
WVFGRD96   27.0     5    45    20   4.15 0.4030
WVFGRD96   28.0     5    45    20   4.15 0.3907
WVFGRD96   29.0     5    45    20   4.16 0.3788

The best solution is

WVFGRD96   11.0   350    45   -20   4.02 0.6344

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

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:

The origin time and epicentral distance are incorrect
The velocity model used for the inversion is incorrect
The velocity model used to define the P-arrival time is not the same as the velocity model used for the waveform inversion (assuming that the initial trace alignment is based on the P arrival time)

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 Sun Apr 28 08:18:43 PM CDT 2024