Location

Location ANSS

The ANSS event ID is us6000tms8 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us6000tms8/executive.

2026/08/22 10:19:13 35.313 -107.533 10.0 4.1 New Mexico

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2026/08/22 10:19:13.0 35.31 -107.53 10.0 4.1 New Mexico Stations used: AE.DOVA AE.DUN6 AE.HANNA AE.PRCT AE.U15A AE.W18A AE.X16A AE.X18A C0.S22A C0.YECK GS.NM01 IU.ANMO IU.TUC JW.BRR SC.121A SC.LEM SC.LPM SC.MLM SC.Y22A SC.Y22D US.MVCO US.SDCO US.WUAZ UU.HMU YX.UNM2 YX.UNM3 YX.UNM5 Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.04 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.17e+22 dyne-cm Mw = 3.98 Z = 20 km Plane Strike Dip Rake NP1 144 76 154 NP2 240 65 15 Principal Axes: Axis Value Plunge Azimuth T 1.17e+22 28 100 N 0.00e+00 61 298 P -1.17e+22 8 194 Moment Tensor: (dyne-cm) Component Value Mxx -1.07e+22 Mxy -4.13e+21 Mxz 7.05e+20 Myy 8.33e+21 Myz 5.13e+21 Mzz 2.33e+21 -------------- ---------------------- ##-------------------------- ###--------------------------- ######---------------------------- ########-------------------######### ##########------------################ ############-------##################### #############--######################### ##############-########################### ###########-----########################## #########--------################## #### ########-----------################ T #### #####--------------############### ### ####-----------------################### ##-------------------################# ----------------------############## -----------------------########### -----------------------####### -------------------------### ----- -------------- - P ---------- Global CMT Convention Moment Tensor: R T P 2.33e+21 7.05e+20 -5.13e+21 7.05e+20 -1.07e+22 4.13e+21 -5.13e+21 4.13e+21 8.33e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260822101913/index.html

Preferred Solution

      STK = 240
      DIP = 65
     RAKE = 15
       MW = 3.98
       HS = 20.0

The NDK file is 20260822101913.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.

Map showing station locations used for computing the ML's. No distinction is made whether the vertical (Z) or horizontal (H) components were used.

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:

cut o DIST/3.3 -40 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.04 n 3 
lp c 0.10 n 3 

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   100    45   -95   3.46 0.1440
WVFGRD96    2.0   285    45   -85   3.61 0.2104
WVFGRD96    3.0   145    80     0   3.49 0.2334
WVFGRD96    4.0   145    75     0   3.54 0.2552
WVFGRD96    5.0   145    70     5   3.59 0.2780
WVFGRD96    6.0   145    70     5   3.64 0.3015
WVFGRD96    7.0   145    70    20   3.69 0.3293
WVFGRD96    8.0   150    65    25   3.76 0.3574
WVFGRD96    9.0   150    70    30   3.79 0.3797
WVFGRD96   10.0   145    75    25   3.81 0.3986
WVFGRD96   11.0   145    75    25   3.84 0.4132
WVFGRD96   12.0   145    75    25   3.87 0.4241
WVFGRD96   13.0   145    80    25   3.89 0.4318
WVFGRD96   14.0   145    80    25   3.91 0.4362
WVFGRD96   15.0   145    80    25   3.93 0.4373
WVFGRD96   16.0   240    65    15   3.93 0.4399
WVFGRD96   17.0   240    65    15   3.94 0.4466
WVFGRD96   18.0   240    65    15   3.96 0.4515
WVFGRD96   19.0   240    65    15   3.97 0.4539
WVFGRD96   20.0   240    65    15   3.98 0.4548
WVFGRD96   21.0   240    60    15   4.00 0.4535
WVFGRD96   22.0   240    60    15   4.01 0.4510
WVFGRD96   23.0   240    60    15   4.02 0.4468
WVFGRD96   24.0   245    55    20   4.03 0.4421
WVFGRD96   25.0   245    55    20   4.04 0.4371
WVFGRD96   26.0   245    55    20   4.05 0.4324
WVFGRD96   27.0   245    55    20   4.05 0.4270
WVFGRD96   28.0   245    55    20   4.06 0.4204
WVFGRD96   29.0   245    55    20   4.06 0.4127

The best solution is

WVFGRD96   20.0   240    65    15   3.98 0.4548

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 0.04 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)

 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