Location

Location ANSS

The ANSS event ID is usp000j0wv and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000j0wv/executive.

2011/05/02 13:55:37 30.729 -105.674 5.2 4.2 Chihuahua, MX

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2011/05/02 13:55:37:0 30.73 -105.67 5.2 4.2 Chihuahua, MX Stations used: TA.133A TA.234A TA.333A TA.433A TA.434A TA.435B TA.533A TA.534A TA.633A TA.634A TA.635A TA.733A TA.734A TA.832A TA.833A TA.933A TA.ABTX TA.MSTX TA.T25A TA.W32A TA.X32A US.AMTX US.JCT US.MNTX US.WMOK Filtering commands used: hp c 0.02 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 2.79e+22 dyne-cm Mw = 4.23 Z = 11 km Plane Strike Dip Rake NP1 355 60 -65 NP2 132 38 -126 Principal Axes: Axis Value Plunge Azimuth T 2.79e+22 12 67 N 0.00e+00 21 162 P -2.79e+22 65 311 Moment Tensor: (dyne-cm) Component Value Mxx 1.94e+21 Mxy 1.19e+22 Mxz -4.76e+21 Myy 1.99e+22 Myz 1.31e+22 Mzz -2.19e+22 -------####### ------------########## -----------------########### -------------------########### #---------------------############ ##---------------------############# ##-----------------------########## ###---------- -----------######### T # ####--------- P -----------######### # #####--------- -----------############## ######-----------------------############# ######-----------------------############# #######----------------------############# #######---------------------############ #########-------------------############ #########-----------------############ ##########---------------########### ############------------########## #############--------######### #######################----- ###############------- ##########---- Global CMT Convention Moment Tensor: R T P -2.19e+22 -4.76e+21 -1.31e+22 -4.76e+21 1.94e+21 -1.19e+22 -1.31e+22 -1.19e+22 1.99e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20110502135537/index.html

Preferred Solution

      STK = 355
      DIP = 60
     RAKE = -65
       MW = 4.23
       HS = 11.0

The NDK file is 20110502135537.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.

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

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:

hp c 0.02 n 3
lp c 0.05 n 3

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    0.5   185    70   -60   3.98 0.2592
WVFGRD96    1.0    25    75   -35   3.97 0.2523
WVFGRD96    2.0   190    65   -55   4.03 0.2690
WVFGRD96    3.0    15    45   -35   4.08 0.3023
WVFGRD96    4.0    15    50   -35   4.09 0.3134
WVFGRD96    5.0    15    60   -40   4.11 0.3083
WVFGRD96    6.0    15    75   -55   4.16 0.3145
WVFGRD96    7.0    10    70   -55   4.17 0.3343
WVFGRD96    8.0     0    65   -70   4.23 0.3501
WVFGRD96    9.0   355    60   -70   4.24 0.3755
WVFGRD96   10.0   355    60   -70   4.24 0.3901
WVFGRD96   11.0   355    60   -65   4.23 0.3904
WVFGRD96   12.0   355    60   -65   4.22 0.3834
WVFGRD96   13.0   360    65   -55   4.20 0.3692
WVFGRD96   14.0    -5    65   -55   4.19 0.3582
WVFGRD96   15.0   215    80    35   4.22 0.3517
WVFGRD96   16.0   215    80    35   4.23 0.3532
WVFGRD96   17.0   215    80    35   4.23 0.3535
WVFGRD96   18.0   215    80    35   4.23 0.3526
WVFGRD96   19.0   215    80    30   4.24 0.3501
WVFGRD96   20.0   215    80    30   4.25 0.3470
WVFGRD96   21.0   215    80    30   4.26 0.3434
WVFGRD96   22.0   215    80    30   4.26 0.3392
WVFGRD96   23.0   215    85    25   4.28 0.3345
WVFGRD96   24.0   215    85    25   4.29 0.3294
WVFGRD96   25.0   215    85    25   4.29 0.3238
WVFGRD96   26.0   215    85    25   4.30 0.3181
WVFGRD96   27.0   215    85    25   4.30 0.3126
WVFGRD96   28.0    35    75    25   4.28 0.3079
WVFGRD96   29.0    35    75    25   4.29 0.3044

The best solution is

WVFGRD96   11.0   355    60   -65   4.23 0.3904

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

hp c 0.02 n 3
lp c 0.05 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)

 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