The ANSS event ID is uu80117176 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/uu80117176/executive.
2025/09/10 23:57:47 40.475 -109.696 69.4 4.1 Utah
USGS/SLU Moment Tensor Solution ENS 2025/09/10 23:57:47.0 40.47 -109.70 69.4 4.1 Utah Stations used: C0.HAYD C0.MOFF N4.K22A N4.O20A UU.BRPU UU.BSUT UU.CTU UU.GAWY UU.HDUT UU.HLJ UU.LIUT UU.MCU UU.SRU UU.SVWY UU.TMU 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 = 1.66e+22 dyne-cm Mw = 4.08 Z = 64 km Plane Strike Dip Rake NP1 110 65 40 NP2 0 54 149 Principal Axes: Axis Value Plunge Azimuth T 1.66e+22 45 330 N 0.00e+00 44 137 P -1.66e+22 6 233 Moment Tensor: (dyne-cm) Component Value Mxx 1.90e+20 Mxy -1.15e+22 Mxz 8.28e+21 Myy -8.36e+21 Myz -2.70e+21 Mzz 8.17e+21 #########----- ###############------- ###################--------- #####################--------- ########## ###########---------- ########### T ###########----------- ############ ############----------- -###########################------------ --###########################----------- -----#########################------------ -------#######################------------ ---------#####################------------ ------------##################------------ ---------------##############----------- -------------------#########------------ ----------------------------------#### - ---------------------########### P ---------------------########## --------------------######### -------------------######### --------------######## ---------##### Global CMT Convention Moment Tensor: R T P 8.17e+21 8.28e+21 2.70e+21 8.28e+21 1.90e+20 1.15e+22 2.70e+21 1.15e+22 -8.36e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20250910235747/index.html |
STK = 110 DIP = 65 RAKE = 40 MW = 4.08 HS = 64.0
The NDK file is 20250910235747.ndk The waveform inversion is preferred.
The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
USGS/SLU Moment Tensor Solution ENS 2025/09/10 23:57:47.0 40.47 -109.70 69.4 4.1 Utah Stations used: C0.HAYD C0.MOFF N4.K22A N4.O20A UU.BRPU UU.BSUT UU.CTU UU.GAWY UU.HDUT UU.HLJ UU.LIUT UU.MCU UU.SRU UU.SVWY UU.TMU 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 = 1.66e+22 dyne-cm Mw = 4.08 Z = 64 km Plane Strike Dip Rake NP1 110 65 40 NP2 0 54 149 Principal Axes: Axis Value Plunge Azimuth T 1.66e+22 45 330 N 0.00e+00 44 137 P -1.66e+22 6 233 Moment Tensor: (dyne-cm) Component Value Mxx 1.90e+20 Mxy -1.15e+22 Mxz 8.28e+21 Myy -8.36e+21 Myz -2.70e+21 Mzz 8.17e+21 #########----- ###############------- ###################--------- #####################--------- ########## ###########---------- ########### T ###########----------- ############ ############----------- -###########################------------ --###########################----------- -----#########################------------ -------#######################------------ ---------#####################------------ ------------##################------------ ---------------##############----------- -------------------#########------------ ----------------------------------#### - ---------------------########### P ---------------------########## --------------------######### -------------------######### --------------######## ---------##### Global CMT Convention Moment Tensor: R T P 8.17e+21 8.28e+21 2.70e+21 8.28e+21 1.90e+20 1.15e+22 2.70e+21 1.15e+22 -8.36e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20250910235747/index.html |
Regional Moment Tensor (Mwr) Moment 1.842e+15 N-m Magnitude 4.11 Mwr Depth 67.0 km Percent DC 88% Half Duration - Catalog US Data Source US Contributor US Nodal Planes Plane Strike Dip Rake NP1 3 58 145 NP2 113 61 37 Principal Axes Axis Value Plunge Azimuth T 1.784e+15 46 330 N 0.112e+15 44 146 P -1.896e+15 2 238 |
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: 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.
![]() |
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.
![]() |
|
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 2.0 150 50 -85 3.21 0.1881 WVFGRD96 4.0 350 65 -50 3.25 0.2211 WVFGRD96 6.0 350 60 -45 3.31 0.2406 WVFGRD96 8.0 350 65 -45 3.42 0.2522 WVFGRD96 10.0 190 75 35 3.46 0.2470 WVFGRD96 12.0 270 60 -25 3.52 0.2362 WVFGRD96 14.0 5 60 -30 3.56 0.2260 WVFGRD96 16.0 285 65 25 3.60 0.2282 WVFGRD96 18.0 285 60 30 3.64 0.2407 WVFGRD96 20.0 285 60 30 3.68 0.2636 WVFGRD96 22.0 285 60 35 3.71 0.2784 WVFGRD96 24.0 285 65 40 3.72 0.2950 WVFGRD96 26.0 285 65 35 3.74 0.3121 WVFGRD96 28.0 285 65 35 3.74 0.3171 WVFGRD96 30.0 290 65 35 3.75 0.3166 WVFGRD96 32.0 290 55 40 3.76 0.3364 WVFGRD96 34.0 120 65 35 3.80 0.3665 WVFGRD96 36.0 115 70 35 3.81 0.3946 WVFGRD96 38.0 115 70 35 3.84 0.4136 WVFGRD96 40.0 295 55 45 3.90 0.4279 WVFGRD96 42.0 290 60 40 3.94 0.4345 WVFGRD96 44.0 115 70 35 3.98 0.4375 WVFGRD96 46.0 115 65 35 4.00 0.4377 WVFGRD96 48.0 115 55 35 4.02 0.4530 WVFGRD96 50.0 115 60 35 4.03 0.4841 WVFGRD96 52.0 115 60 35 4.05 0.5126 WVFGRD96 54.0 115 60 40 4.06 0.5391 WVFGRD96 56.0 115 60 40 4.07 0.5611 WVFGRD96 58.0 115 60 40 4.07 0.5739 WVFGRD96 60.0 115 60 40 4.08 0.5876 WVFGRD96 62.0 110 65 40 4.08 0.5928 WVFGRD96 64.0 110 65 40 4.08 0.5964 WVFGRD96 66.0 110 65 40 4.08 0.5949 WVFGRD96 68.0 110 65 40 4.08 0.5926 WVFGRD96 70.0 110 65 40 4.08 0.5874 WVFGRD96 72.0 110 65 40 4.08 0.5798 WVFGRD96 74.0 110 65 40 4.08 0.5707 WVFGRD96 76.0 110 65 40 4.08 0.5626 WVFGRD96 78.0 105 65 40 4.08 0.5551 WVFGRD96 80.0 105 65 40 4.08 0.5462 WVFGRD96 82.0 105 65 40 4.08 0.5354 WVFGRD96 84.0 105 65 35 4.08 0.5279 WVFGRD96 86.0 105 65 35 4.08 0.5199 WVFGRD96 88.0 105 65 35 4.08 0.5131 WVFGRD96 90.0 100 60 40 4.09 0.5084 WVFGRD96 92.0 100 60 40 4.09 0.5038 WVFGRD96 94.0 100 60 40 4.09 0.4995 WVFGRD96 96.0 100 60 40 4.09 0.4947 WVFGRD96 98.0 100 60 40 4.10 0.4899
The best solution is
WVFGRD96 64.0 110 65 40 4.08 0.5964
The mechanism corresponding to the best fit is
![]() |
|
The best fit as a function of depth is given in the following figure:
![]() |
|
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
![]() |
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:
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