USGS/SLU Moment Tensor Solution ENS 2020/11/20 10:10:05:0 38.19 -117.78 14.4 3.9 Nevada Stations used: BK.WELL CI.CCC CI.CLC CI.CWC CI.FUR CI.GRA CI.ISA CI.LRL CI.RAG CI.TIN CI.VES GS.MCA04 IM.NV31 LB.BMN NC.AFD NN.CMK6 NN.KVN NN.LHV NN.PAH NN.PIO NN.PNT NN.PRN NN.Q09A NN.S11A UU.FOR1 UU.PSUT Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 2.95e+21 dyne-cm Mw = 3.58 Z = 10 km Plane Strike Dip Rake NP1 90 90 -30 NP2 180 60 -180 Principal Axes: Axis Value Plunge Azimuth T 2.95e+21 21 139 N 0.00e+00 60 270 P -2.95e+21 21 41 Moment Tensor: (dyne-cm) Component Value Mxx 9.44e+13 Mxy -2.56e+21 Mxz -1.48e+21 Myy -2.23e+14 Myz 4.72e+13 Mzz 1.29e+14 ######-------- ########-------------- ##########------------------ ##########--------------- -- ###########---------------- P ---- ############---------------- ----- ############-------------------------- #############--------------------------- #############--------------------------- #############----------------------------- #############----------------------------- -------------############################# -------------############################# -------------########################### -------------########################### ------------########################## ------------################ ##### -----------################ T #### ----------############### ## ----------################## --------############## ------######## Global CMT Convention Moment Tensor: R T P 1.29e+14 -1.48e+21 -4.72e+13 -1.48e+21 9.44e+13 2.56e+21 -4.72e+13 2.56e+21 -2.23e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20201120101005/index.html |
STK = 90 DIP = 90 RAKE = -30 MW = 3.58 HS = 10.0
The NDK file is 20201120101005.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2020/11/20 10:10:05:0 38.19 -117.78 14.4 3.9 Nevada Stations used: BK.WELL CI.CCC CI.CLC CI.CWC CI.FUR CI.GRA CI.ISA CI.LRL CI.RAG CI.TIN CI.VES GS.MCA04 IM.NV31 LB.BMN NC.AFD NN.CMK6 NN.KVN NN.LHV NN.PAH NN.PIO NN.PNT NN.PRN NN.Q09A NN.S11A UU.FOR1 UU.PSUT Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 2.95e+21 dyne-cm Mw = 3.58 Z = 10 km Plane Strike Dip Rake NP1 90 90 -30 NP2 180 60 -180 Principal Axes: Axis Value Plunge Azimuth T 2.95e+21 21 139 N 0.00e+00 60 270 P -2.95e+21 21 41 Moment Tensor: (dyne-cm) Component Value Mxx 9.44e+13 Mxy -2.56e+21 Mxz -1.48e+21 Myy -2.23e+14 Myz 4.72e+13 Mzz 1.29e+14 ######-------- ########-------------- ##########------------------ ##########--------------- -- ###########---------------- P ---- ############---------------- ----- ############-------------------------- #############--------------------------- #############--------------------------- #############----------------------------- #############----------------------------- -------------############################# -------------############################# -------------########################### -------------########################### ------------########################## ------------################ ##### -----------################ T #### ----------############### ## ----------################## --------############## ------######## Global CMT Convention Moment Tensor: R T P 1.29e+14 -1.48e+21 -4.72e+13 -1.48e+21 9.44e+13 2.56e+21 -4.72e+13 2.56e+21 -2.23e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20201120101005/index.html |
(a) ML computed using the IASPEI formula for Horizontal components; (b) 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.
(a) ML computed using the IASPEI formula for Vertical components (research); (b) 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.
The focal mechanism was determined using broadband seismic waveforms. The location of the event and the and stations used for 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 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 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 90 85 -5 3.26 0.4487 WVFGRD96 2.0 90 90 -5 3.38 0.6015 WVFGRD96 3.0 275 75 20 3.45 0.6502 WVFGRD96 4.0 275 75 30 3.49 0.6918 WVFGRD96 5.0 270 85 35 3.52 0.7275 WVFGRD96 6.0 270 85 35 3.53 0.7502 WVFGRD96 7.0 270 85 30 3.54 0.7644 WVFGRD96 8.0 90 90 -35 3.57 0.7704 WVFGRD96 9.0 90 90 -30 3.57 0.7744 WVFGRD96 10.0 90 90 -30 3.58 0.7754 WVFGRD96 11.0 270 85 25 3.59 0.7747 WVFGRD96 12.0 90 90 -25 3.59 0.7712 WVFGRD96 13.0 270 85 25 3.60 0.7668 WVFGRD96 14.0 90 90 -25 3.61 0.7613 WVFGRD96 15.0 270 90 20 3.62 0.7573 WVFGRD96 16.0 90 90 -20 3.63 0.7529 WVFGRD96 17.0 90 90 -20 3.63 0.7471 WVFGRD96 18.0 90 90 -20 3.64 0.7402 WVFGRD96 19.0 90 90 -20 3.65 0.7333 WVFGRD96 20.0 90 90 -20 3.66 0.7259 WVFGRD96 21.0 90 90 -20 3.67 0.7175 WVFGRD96 22.0 270 90 20 3.67 0.7088 WVFGRD96 23.0 90 90 -20 3.68 0.7004 WVFGRD96 24.0 90 85 -15 3.69 0.6935 WVFGRD96 25.0 90 85 -15 3.70 0.6856 WVFGRD96 26.0 270 90 15 3.70 0.6766 WVFGRD96 27.0 90 85 -15 3.72 0.6684 WVFGRD96 28.0 90 90 -15 3.72 0.6603 WVFGRD96 29.0 270 90 15 3.73 0.6524
The best solution is
WVFGRD96 10.0 90 90 -30 3.58 0.7754
The mechanism correspond 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 and because the velocity model used in the predictions may not be perfect. 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 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2
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Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to thewavefroms. 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.
Thanks also to the many seismic network operators whose dedication make this effort possible: University of Nevada Reno, University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureau of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Oklahoma Geological Survey, TexNet, the Iris stations, the Transportable Array of EarthScope and other networks.
The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
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
Here we tabulate the reasons for not using certain digital data sets
The following stations did not have a valid response files: