The ANSS event ID is uu60497322 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/uu60497322/executive.
2022/05/11 13:32:02 44.681 -109.996 13.9 4.22 Wyoming
USGS/SLU Moment Tensor Solution ENS 2022/05/11 13:32:02:0 44.68 -110.00 13.9 4.2 Wyoming Stations used: IM.PD31 IW.DLMT IW.FLWY IW.FXWY IW.IMW IW.LOHW IW.MOOW IW.SNOW IW.TPAW MB.GBMT MB.HLMT MB.SRMT US.BOZ US.BW06 US.EGMT US.HLID US.HWUT US.MSO US.RLMT UU.SPU UU.TCU WY.YHB WY.YMR WY.YNE Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +60 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 3.67e+22 dyne-cm Mw = 4.31 Z = 27 km Plane Strike Dip Rake NP1 310 65 65 NP2 178 35 132 Principal Axes: Axis Value Plunge Azimuth T 3.67e+22 62 181 N 0.00e+00 23 321 P -3.67e+22 16 58 Moment Tensor: (dyne-cm) Component Value Mxx -1.11e+21 Mxy -1.50e+22 Mxz -2.06e+22 Myy -2.44e+22 Myz -8.73e+21 Mzz 2.55e+22 ###----------- #####----------------- ######---------------------- ######------------------------ ------###------------------------- ------########------------------ - -------###########--------------- P -- -------###############------------ --- -------#################---------------- -------####################--------------- -------######################------------- -------########################----------- --------########################---------- -------########### ############------- -------########### T #############------ -------########## #############----- -------##########################--- -------##########################- ------######################## -------##################### ------################ -----######### Global CMT Convention Moment Tensor: R T P 2.55e+22 -2.06e+22 8.73e+21 -2.06e+22 -1.11e+21 1.50e+22 8.73e+21 1.50e+22 -2.44e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20220511133202/index.html |
STK = 310 DIP = 65 RAKE = 65 MW = 4.31 HS = 27.0
The NDK file is 20220511133202.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: 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 +60 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.05 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 125 50 -85 3.96 0.2148 WVFGRD96 2.0 285 45 -95 4.05 0.2572 WVFGRD96 3.0 120 45 -75 4.12 0.2571 WVFGRD96 4.0 130 50 -65 4.15 0.2341 WVFGRD96 5.0 265 35 35 4.15 0.2153 WVFGRD96 6.0 265 35 35 4.15 0.2198 WVFGRD96 7.0 325 20 90 4.13 0.2258 WVFGRD96 8.0 145 70 90 4.20 0.2417 WVFGRD96 9.0 145 70 85 4.20 0.2577 WVFGRD96 10.0 150 70 85 4.20 0.2745 WVFGRD96 11.0 105 80 -65 4.21 0.2907 WVFGRD96 12.0 105 75 -65 4.22 0.3096 WVFGRD96 13.0 105 75 -65 4.23 0.3265 WVFGRD96 14.0 105 75 -65 4.24 0.3410 WVFGRD96 15.0 105 75 -60 4.25 0.3538 WVFGRD96 16.0 105 75 -60 4.25 0.3647 WVFGRD96 17.0 110 80 -60 4.25 0.3742 WVFGRD96 18.0 110 80 -60 4.25 0.3825 WVFGRD96 19.0 310 70 60 4.25 0.3907 WVFGRD96 20.0 310 65 60 4.27 0.4014 WVFGRD96 21.0 310 65 60 4.28 0.4088 WVFGRD96 22.0 310 65 65 4.28 0.4168 WVFGRD96 23.0 310 65 65 4.29 0.4233 WVFGRD96 24.0 310 65 65 4.29 0.4282 WVFGRD96 25.0 310 65 65 4.30 0.4318 WVFGRD96 26.0 310 65 65 4.30 0.4340 WVFGRD96 27.0 310 65 65 4.31 0.4350 WVFGRD96 28.0 310 65 65 4.31 0.4347 WVFGRD96 29.0 310 65 65 4.32 0.4333 WVFGRD96 30.0 310 65 65 4.32 0.4305 WVFGRD96 31.0 310 65 65 4.33 0.4268 WVFGRD96 32.0 310 65 65 4.33 0.4221 WVFGRD96 33.0 305 70 65 4.33 0.4167 WVFGRD96 34.0 310 70 65 4.33 0.4111 WVFGRD96 35.0 310 70 65 4.34 0.4056 WVFGRD96 36.0 310 70 65 4.34 0.4002 WVFGRD96 37.0 310 70 65 4.34 0.3947 WVFGRD96 38.0 310 70 65 4.35 0.3893 WVFGRD96 39.0 310 70 65 4.35 0.3843 WVFGRD96 40.0 305 80 70 4.47 0.3773 WVFGRD96 41.0 310 75 75 4.47 0.3712 WVFGRD96 42.0 310 75 75 4.47 0.3649 WVFGRD96 43.0 310 75 70 4.47 0.3586 WVFGRD96 44.0 310 75 70 4.47 0.3523 WVFGRD96 45.0 310 75 70 4.48 0.3457 WVFGRD96 46.0 310 75 70 4.48 0.3392 WVFGRD96 47.0 310 75 70 4.48 0.3326 WVFGRD96 48.0 310 75 70 4.48 0.3260 WVFGRD96 49.0 315 75 70 4.48 0.3196
The best solution is
WVFGRD96 27.0 310 65 65 4.31 0.4350
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 +60 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.05 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