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.
The ANSS event ID is tx2024mydx and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/tx2024mydx/executive.
2024/07/02 23:39:59 31.669 -104.195 6.1 3.6 Texas
USGS/SLU Moment Tensor Solution
ENS 2024/07/02 23:39:59:0 31.67 -104.19 6.1 3.6 Texas
Stations used:
4O.BP01 4O.CV01 4O.DB04 4O.LWM1 4O.LWM2 4O.MBBB2 4O.MID01
4O.MID03 4O.SA04 4O.SA07 4O.SA09 4O.VW01 4O.WB02 4O.WB03
4O.WB04 4O.WB06 4O.WB07 4O.WB08 4O.WB09 4O.WB10 4O.WB11
4O.WB12 4T.NM01 4T.NM02 TX.ALPN TX.MB18 TX.MB25 TX.ODSA
TX.PB01 TX.PB03 TX.PB04 TX.PB06 TX.PB07 TX.PB09 TX.PB10
TX.PB11 TX.PB12 TX.PB13 TX.PB16 TX.PB23 TX.PB24 TX.PB25
TX.PB26 TX.PB28 TX.PB29 TX.PB30 TX.PB31 TX.PB33 TX.PB34
TX.PB35 TX.PB37 TX.PB38 TX.PB40 TX.PB43 TX.PB44 TX.PB46
TX.PB47 TX.PB51 TX.PCOS TX.PECS TX.VHRN
Filtering commands used:
cut o DIST/3.3 -30 o DIST/3.3 +30
rtr
taper w 0.1
hp c 0.05 n 3
lp c 0.15 n 3
Best Fitting Double Couple
Mo = 2.16e+21 dyne-cm
Mw = 3.49
Z = 7 km
Plane Strike Dip Rake
NP1 95 60 -109
NP2 310 35 -60
Principal Axes:
Axis Value Plunge Azimuth
T 2.16e+21 13 199
N 0.00e+00 17 105
P -2.16e+21 69 325
Moment Tensor: (dyne-cm)
Component Value
Mxx 1.64e+21
Mxy 7.59e+20
Mxz -1.06e+21
Myy 1.16e+20
Myz 2.67e+20
Mzz -1.76e+21
##############
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---------------------------#########
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--------------- --------------########
--------------- P ----------------######
---------------- -----------------######
#------------------------------------#####
###----------------------------------#####
#####---------------------------------###-
########--------------------------------
#############-------------------#####---
####################################--
###################################-
#################################-
##############################
####### ##################
#### T ###############
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Global CMT Convention Moment Tensor:
R T P
-1.76e+21 -1.06e+21 -2.67e+20
-1.06e+21 1.64e+21 -7.59e+20
-2.67e+20 -7.59e+20 1.16e+20
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20240702233959/index.html
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STK = 310
DIP = 35
RAKE = -60
MW = 3.49
HS = 7.0
The NDK file is 20240702233959.ndk The waveform inversion is preferred.
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.
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.
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.
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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.
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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 +30 rtr taper w 0.1 hp c 0.05 n 3 lp c 0.15 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 75 65 -10 2.99 0.1817
WVFGRD96 2.0 245 55 -35 3.21 0.2311
WVFGRD96 3.0 325 25 -30 3.33 0.2791
WVFGRD96 4.0 315 30 -50 3.40 0.3757
WVFGRD96 5.0 310 35 -60 3.44 0.4390
WVFGRD96 6.0 315 35 -55 3.47 0.4684
WVFGRD96 7.0 310 35 -60 3.49 0.4760
WVFGRD96 8.0 310 35 -60 3.58 0.4733
WVFGRD96 9.0 310 35 -65 3.60 0.4643
WVFGRD96 10.0 310 35 -65 3.62 0.4457
WVFGRD96 11.0 305 35 -70 3.64 0.4234
WVFGRD96 12.0 305 35 -70 3.65 0.3972
WVFGRD96 13.0 305 30 -70 3.65 0.3704
WVFGRD96 14.0 305 30 -70 3.66 0.3440
WVFGRD96 15.0 300 30 -80 3.67 0.3196
WVFGRD96 16.0 305 30 -75 3.68 0.2974
WVFGRD96 17.0 285 20 -85 3.68 0.2811
WVFGRD96 18.0 105 70 -90 3.69 0.2693
WVFGRD96 19.0 285 20 -85 3.70 0.2593
WVFGRD96 20.0 285 20 -85 3.70 0.2506
WVFGRD96 21.0 295 45 -85 3.72 0.2495
WVFGRD96 22.0 110 45 -95 3.72 0.2518
WVFGRD96 23.0 290 50 -90 3.73 0.2512
WVFGRD96 24.0 290 50 -90 3.74 0.2517
WVFGRD96 25.0 105 45 -100 3.74 0.2495
WVFGRD96 26.0 95 40 65 3.74 0.2480
WVFGRD96 27.0 95 40 65 3.74 0.2486
WVFGRD96 28.0 95 40 65 3.75 0.2485
WVFGRD96 29.0 95 45 60 3.76 0.2481
The best solution is
WVFGRD96 7.0 310 35 -60 3.49 0.4760
The mechanism corresponding to the best fit is
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The best fit as a function of depth is given in the following figure:
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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 +30 rtr taper w 0.1 hp c 0.05 n 3 lp c 0.15 n 3
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| 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. |
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| 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:
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.
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