Location

Location ANSS

2021/06/11 18:19:27 28.370 -105.156 10.0 4.1 Chihuahua, Mexico

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2021/06/11 18:19:27:0 28.37 -105.16 10.0 4.1 Chihuahua, Mexico Stations used: EP.KIDD GM.NMP01 GM.NMP11 GM.NMP23 GM.NMP25 GM.NMP35 GM.NMP44 IM.TX31 MX.HPIG MX.HSIG NX.WTX29 TX.833A TX.ALPN TX.MB01 TX.MB06 TX.MNHN TX.ODSA TX.OZNA TX.PB01 TX.PB03 TX.PB04 TX.PB07 TX.PB10 TX.PB11 TX.PB16 TX.PB28 TX.PECS TX.SAND TX.SGCY TX.VHRN US.JCT US.MNTX Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 5.69e+21 dyne-cm Mw = 3.77 Z = 3 km Plane Strike Dip Rake NP1 127 51 -98 NP2 320 40 -80 Principal Axes: Axis Value Plunge Azimuth T 5.69e+21 5 223 N 0.00e+00 6 132 P -5.69e+21 82 353 Moment Tensor: (dyne-cm) Component Value Mxx 2.90e+21 Mxy 2.83e+21 Mxz -1.20e+21 Myy 2.61e+21 Myz -2.59e+20 Mzz -5.52e+21 ############## ###################### ------------################ -----------------############# ----------------------############ #------------------------########### ###-------------------------########## ####---------------------------######### ####-------------- -----------######## ######------------- P ------------######## #######------------ -------------####### ########---------------------------####### ##########--------------------------###### ##########-------------------------##### ############-----------------------##### ##############--------------------#### ################-----------------### ## ##############-------------## T ##########################- #########################- ###################### ############## Global CMT Convention Moment Tensor: R T P -5.52e+21 -1.20e+21 2.59e+20 -1.20e+21 2.90e+21 -2.83e+21 2.59e+20 -2.83e+21 2.61e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210611181927/index.html

Preferred Solution

The preferred solution from an analysis of the surface-wave spectral amplitude radiation pattern, waveform inversion and first motion observations is

      STK = 320
      DIP = 40
     RAKE = -80
       MW = 3.77
       HS = 3.0

The NDK file is 20210611181927.ndk The waveform inversion is preferred.

Moment Tensor Comparison

The following compares this source inversion to others

SLU

USGS/SLU Moment Tensor Solution ENS 2021/06/11 18:19:27:0 28.37 -105.16 10.0 4.1 Chihuahua, Mexico Stations used: EP.KIDD GM.NMP01 GM.NMP11 GM.NMP23 GM.NMP25 GM.NMP35 GM.NMP44 IM.TX31 MX.HPIG MX.HSIG NX.WTX29 TX.833A TX.ALPN TX.MB01 TX.MB06 TX.MNHN TX.ODSA TX.OZNA TX.PB01 TX.PB03 TX.PB04 TX.PB07 TX.PB10 TX.PB11 TX.PB16 TX.PB28 TX.PECS TX.SAND TX.SGCY TX.VHRN US.JCT US.MNTX Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 5.69e+21 dyne-cm Mw = 3.77 Z = 3 km Plane Strike Dip Rake NP1 127 51 -98 NP2 320 40 -80 Principal Axes: Axis Value Plunge Azimuth T 5.69e+21 5 223 N 0.00e+00 6 132 P -5.69e+21 82 353 Moment Tensor: (dyne-cm) Component Value Mxx 2.90e+21 Mxy 2.83e+21 Mxz -1.20e+21 Myy 2.61e+21 Myz -2.59e+20 Mzz -5.52e+21 ############## ###################### ------------################ -----------------############# ----------------------############ #------------------------########### ###-------------------------########## ####---------------------------######### ####-------------- -----------######## ######------------- P ------------######## #######------------ -------------####### ########---------------------------####### ##########--------------------------###### ##########-------------------------##### ############-----------------------##### ##############--------------------#### ################-----------------### ## ##############-------------## T ##########################- #########################- ###################### ############## Global CMT Convention Moment Tensor: R T P -5.52e+21 -1.20e+21 2.59e+20 -1.20e+21 2.90e+21 -2.83e+21 2.59e+20 -2.83e+21 2.61e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210611181927/index.html

Magnitudes

mLg Magnitude

(a) mLg computed using the IASPEI formula; (b) mLg residuals ; the values used for the trimmed mean are indicated.

ML Magnitude

(a) ML computed using the IASPEI formula for Horizontal components; (b) 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.

(a) ML computed using the IASPEI formula for Vertical components (research); (b) 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.

Context

The next figure presents the focal mechanism for this earthquake (red) in the context of other events (blue) in the SLU Moment Tensor Catalog which are within ± 0.5 degrees of the new event. This comparison is shown in the left panel of the figure. 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).

Waveform Inversion using wvfgrd96

The focal mechanism was determined using broadband seismic waveforms. The location of the event and the and stations used for 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 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 0.025 n 3 
lp c 0.06 n 3

The results of this grid search from 0.5 to 19 km depth are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   150    50   -70   3.62 0.4406
WVFGRD96    2.0   155    50   -60   3.68 0.4916
WVFGRD96    3.0   320    40   -80   3.77 0.5296
WVFGRD96    4.0   325    40   -70   3.81 0.5125
WVFGRD96    5.0   340    45   -45   3.79 0.4713
WVFGRD96    6.0   350    55   -15   3.76 0.4406
WVFGRD96    7.0    -5    60     0   3.76 0.4330
WVFGRD96    8.0   350    45   -20   3.81 0.4318
WVFGRD96    9.0   185    50    25   3.82 0.4361
WVFGRD96   10.0   190    45    30   3.83 0.4511
WVFGRD96   11.0   190    50    35   3.85 0.4641
WVFGRD96   12.0   190    50    35   3.86 0.4742
WVFGRD96   13.0   190    50    35   3.86 0.4815
WVFGRD96   14.0   190    50    35   3.87 0.4865
WVFGRD96   15.0   190    50    35   3.88 0.4895
WVFGRD96   16.0   195    50    45   3.90 0.4909
WVFGRD96   17.0   195    50    45   3.91 0.4914
WVFGRD96   18.0   225    30    95   3.98 0.4941
WVFGRD96   19.0    40    60    85   3.98 0.4964
WVFGRD96   20.0    40    60    85   3.98 0.4976
WVFGRD96   21.0   225    30    95   4.00 0.4965
WVFGRD96   22.0    40    60    85   4.00 0.4948
WVFGRD96   23.0   225    30    95   4.01 0.4932
WVFGRD96   24.0    35    60    85   4.02 0.4894
WVFGRD96   25.0    35    60    85   4.02 0.4855
WVFGRD96   26.0    35    60    85   4.03 0.4811
WVFGRD96   27.0   230    30   105   4.03 0.4764
WVFGRD96   28.0    35    60    85   4.04 0.4704
WVFGRD96   29.0    35    60    85   4.04 0.4645

The best solution is

WVFGRD96    3.0   320    40   -80   3.77 0.5296

The mechanism correspond 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 and because the velocity model used in the predictions may not be perfect. 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 0.025 n 3 
lp c 0.06 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.

Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to thewavefroms. 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.

Discussion

Acknowledgements

Thanks also to the many seismic network operators whose dedication make this effort possible: University of Nevada Reno, University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureau of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Oklahoma Geological Survey, TexNet, the Iris stations, the Transportable Array of EarthScope and other networks.

Velocity Model

The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:

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

Quality Control

Here we tabulate the reasons for not using certain digital data sets

The following stations did not have a valid response files:

Last Changed Fri Jun 11 17:21:05 CDT 2021