The ANSS event ID is nn00862970 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/nn00862970/executive.
2023/07/19 07:34:23 39.511 -116.536 3.7 4.5 Nevada
USGS/SLU Moment Tensor Solution ENS 2023/07/19 07:34:23:0 39.51 -116.54 3.7 4.5 Nevada Stations used: BK.BIGV BK.BUCR BK.EAGL BK.HELL BK.MMI BK.MZTA BK.OVRO BK.RAVE BK.WELL BK.YUBA CI.FUR CI.GRA CI.SHO GS.MCA04 IM.NV31 LB.BMN NC.AFD NN.BEK NN.DIX NN.GMN NN.GWY NN.KVN NN.LHV NN.MPK NN.PAH NN.PNT NN.PRN NN.PYM2 NN.REDF NN.SHP NN.UNVG SN.TPW UO.ADEL UO.JAZZ US.DUG US.ELK US.TPNV US.WVOR UU.BGU UU.CCUT UU.CTU UU.ECUT UU.FOR1 UU.HVU UU.KNB UU.MOUT UU.MPU UU.MTPU UU.NLU UU.NOQ UU.PKCU UU.PSUT UU.SPU UU.SWUT UU.SZCU UU.TCRU UU.VRUT Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 3.94e+22 dyne-cm Mw = 4.33 Z = 3 km Plane Strike Dip Rake NP1 240 55 -75 NP2 35 38 -110 Principal Axes: Axis Value Plunge Azimuth T 3.94e+22 9 319 N 0.00e+00 12 51 P -3.94e+22 75 194 Moment Tensor: (dyne-cm) Component Value Mxx 1.96e+22 Mxy -1.96e+22 Mxz 1.42e+22 Myy 1.62e+22 Myz -1.44e+21 Mzz -3.57e+22 ############## ###################### ########################- # T #########################- ### #########################--- ###################--------------### ################------------------#### ##############---------------------##### ###########------------------------##### ##########--------------------------###### ########---------------------------####### #######----------------------------####### ######------------ -------------######## ####------------- P ------------######## ###-------------- -----------######### #----------------------------######### --------------------------########## -----------------------########### -------------------########### ---------------############# ###################### ############## Global CMT Convention Moment Tensor: R T P -3.57e+22 1.42e+22 1.44e+21 1.42e+22 1.96e+22 1.96e+22 1.44e+21 1.96e+22 1.62e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230719073423/index.html |
STK = 240 DIP = 55 RAKE = -75 MW = 4.33 HS = 3.0
The NDK file is 20230719073423.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 2023/07/19 07:34:23:0 39.51 -116.54 3.7 4.5 Nevada Stations used: BK.BIGV BK.BUCR BK.EAGL BK.HELL BK.MMI BK.MZTA BK.OVRO BK.RAVE BK.WELL BK.YUBA CI.FUR CI.GRA CI.SHO GS.MCA04 IM.NV31 LB.BMN NC.AFD NN.BEK NN.DIX NN.GMN NN.GWY NN.KVN NN.LHV NN.MPK NN.PAH NN.PNT NN.PRN NN.PYM2 NN.REDF NN.SHP NN.UNVG SN.TPW UO.ADEL UO.JAZZ US.DUG US.ELK US.TPNV US.WVOR UU.BGU UU.CCUT UU.CTU UU.ECUT UU.FOR1 UU.HVU UU.KNB UU.MOUT UU.MPU UU.MTPU UU.NLU UU.NOQ UU.PKCU UU.PSUT UU.SPU UU.SWUT UU.SZCU UU.TCRU UU.VRUT Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 3.94e+22 dyne-cm Mw = 4.33 Z = 3 km Plane Strike Dip Rake NP1 240 55 -75 NP2 35 38 -110 Principal Axes: Axis Value Plunge Azimuth T 3.94e+22 9 319 N 0.00e+00 12 51 P -3.94e+22 75 194 Moment Tensor: (dyne-cm) Component Value Mxx 1.96e+22 Mxy -1.96e+22 Mxz 1.42e+22 Myy 1.62e+22 Myz -1.44e+21 Mzz -3.57e+22 ############## ###################### ########################- # T #########################- ### #########################--- ###################--------------### ################------------------#### ##############---------------------##### ###########------------------------##### ##########--------------------------###### ########---------------------------####### #######----------------------------####### ######------------ -------------######## ####------------- P ------------######## ###-------------- -----------######### #----------------------------######### --------------------------########## -----------------------########### -------------------########### ---------------############# ###################### ############## Global CMT Convention Moment Tensor: R T P -3.57e+22 1.42e+22 1.44e+21 1.42e+22 1.96e+22 1.96e+22 1.44e+21 1.96e+22 1.62e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230719073423/index.html |
Regional Moment Tensor (Mwr) Moment 4.268e+15 N-m Magnitude 4.35 Mwr Depth 3.0 km Percent DC 83% Half Duration - Catalog US Data Source US 2 Contributor US 2 Nodal Planes Plane Strike Dip Rake NP1 225 48 -93 NP2 49 43 -87 Principal Axes Axis Value Plunge Azimuth T 4.441e+15 N-m 2 317 N -0.369e+15 N-m 2 227 P -4.072e+15 N-m 87 97 |
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 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 250 55 -55 4.15 0.4911 WVFGRD96 2.0 250 55 -60 4.25 0.5824 WVFGRD96 3.0 240 55 -75 4.33 0.6428 WVFGRD96 4.0 240 55 -70 4.35 0.6330 WVFGRD96 5.0 250 60 -60 4.33 0.5791 WVFGRD96 6.0 95 75 10 4.26 0.5573 WVFGRD96 7.0 95 75 15 4.28 0.5656 WVFGRD96 8.0 95 70 15 4.31 0.5644 WVFGRD96 9.0 95 70 15 4.32 0.5662 WVFGRD96 10.0 280 65 35 4.36 0.5665 WVFGRD96 11.0 280 65 35 4.37 0.5806 WVFGRD96 12.0 280 65 35 4.38 0.5915 WVFGRD96 13.0 280 65 30 4.38 0.5987 WVFGRD96 14.0 280 65 30 4.39 0.6031 WVFGRD96 15.0 280 65 30 4.40 0.6044 WVFGRD96 16.0 280 65 30 4.40 0.6028 WVFGRD96 17.0 275 65 25 4.41 0.5992 WVFGRD96 18.0 275 65 25 4.42 0.5942 WVFGRD96 19.0 275 70 25 4.43 0.5876 WVFGRD96 20.0 275 70 25 4.43 0.5799 WVFGRD96 21.0 275 65 20 4.44 0.5695 WVFGRD96 22.0 275 65 20 4.44 0.5602 WVFGRD96 23.0 275 65 20 4.45 0.5500 WVFGRD96 24.0 275 65 20 4.45 0.5394 WVFGRD96 25.0 275 65 15 4.46 0.5284 WVFGRD96 26.0 275 65 15 4.46 0.5184 WVFGRD96 27.0 275 65 10 4.47 0.5080 WVFGRD96 28.0 275 65 10 4.48 0.4977 WVFGRD96 29.0 275 65 10 4.48 0.4874
The best solution is
WVFGRD96 3.0 240 55 -75 4.33 0.6428
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 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 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