The ANSS event ID is us200030nt and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us200030nt/executive.
2015/07/28 01:18:27 35.991 -97.581 5.3 4.1 Oklahoma
USGS/SLU Moment Tensor Solution ENS 2015/07/28 01:18:27:0 35.99 -97.58 5.3 4.1 Oklahoma Stations used: AG.HHAR GS.KAN05 GS.KAN08 GS.KAN10 GS.KAN11 GS.KAN12 GS.KAN13 GS.KAN17 GS.KS20 GS.KS21 GS.OK025 GS.OK029 GS.OK031 N4.R32B N4.T35B N4.U38B N4.Z35B OK.BCOK OK.BLOK OK.CCOK OK.CHOK OK.CROK OK.FNO OK.LOOK OK.QUOK OK.U32A OK.X34A OK.X37A TA.ABTX TA.W39A US.CBKS US.KSU1 US.MIAR US.WMOK Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.97e+22 dyne-cm Mw = 4.13 Z = 6 km Plane Strike Dip Rake NP1 183 80 170 NP2 275 80 10 Principal Axes: Axis Value Plunge Azimuth T 1.97e+22 14 139 N 0.00e+00 76 320 P -1.97e+22 0 229 Moment Tensor: (dyne-cm) Component Value Mxx 2.16e+21 Mxy -1.89e+22 Mxz -3.50e+21 Myy -3.33e+21 Myz 3.08e+21 Mzz 1.17e+21 ########------ ###########----------- ##############-------------- ##############---------------- ################------------------ #################------------------- #################--------------------- ##################---------------------- ##################---------------------- #######-----------#----------------------- -------------------##############--------- ------------------#####################--- ------------------######################## -----------------####################### -----------------####################### ----------------###################### ---------------##################### - ----------############# #### P -----------############ T ## -----------############ # ---------############# -----######### Global CMT Convention Moment Tensor: R T P 1.17e+21 -3.50e+21 -3.08e+21 -3.50e+21 2.16e+21 1.89e+22 -3.08e+21 1.89e+22 -3.33e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150728011827/index.html |
STK = 275 DIP = 80 RAKE = 10 MW = 4.13 HS = 6.0
The NDK file is 20150728011827.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 2015/07/28 01:18:27:0 35.99 -97.58 5.3 4.1 Oklahoma Stations used: AG.HHAR GS.KAN05 GS.KAN08 GS.KAN10 GS.KAN11 GS.KAN12 GS.KAN13 GS.KAN17 GS.KS20 GS.KS21 GS.OK025 GS.OK029 GS.OK031 N4.R32B N4.T35B N4.U38B N4.Z35B OK.BCOK OK.BLOK OK.CCOK OK.CHOK OK.CROK OK.FNO OK.LOOK OK.QUOK OK.U32A OK.X34A OK.X37A TA.ABTX TA.W39A US.CBKS US.KSU1 US.MIAR US.WMOK Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.97e+22 dyne-cm Mw = 4.13 Z = 6 km Plane Strike Dip Rake NP1 183 80 170 NP2 275 80 10 Principal Axes: Axis Value Plunge Azimuth T 1.97e+22 14 139 N 0.00e+00 76 320 P -1.97e+22 0 229 Moment Tensor: (dyne-cm) Component Value Mxx 2.16e+21 Mxy -1.89e+22 Mxz -3.50e+21 Myy -3.33e+21 Myz 3.08e+21 Mzz 1.17e+21 ########------ ###########----------- ##############-------------- ##############---------------- ################------------------ #################------------------- #################--------------------- ##################---------------------- ##################---------------------- #######-----------#----------------------- -------------------##############--------- ------------------#####################--- ------------------######################## -----------------####################### -----------------####################### ----------------###################### ---------------##################### - ----------############# #### P -----------############ T ## -----------############ # ---------############# -----######### Global CMT Convention Moment Tensor: R T P 1.17e+21 -3.50e+21 -3.08e+21 -3.50e+21 2.16e+21 1.89e+22 -3.08e+21 1.89e+22 -3.33e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150728011827/index.html |
Regional Moment Tensor (Mwr) Moment 1.762e+15 N-m Magnitude 4.10 Depth 4.0 km Percent DC 91% Half Duration – Catalog US (us200030nt) Data Source US1 Contributor US1 Nodal Planes Plane Strike Dip Rake NP1 97 78 -25 NP2 193 65 -167 Principal Axes Axis Value Plunge Azimuth T 1.718 9 147 N 0.083 62 254 P -1.802 26 53 |
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: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated.
Right: residuals as a function of distance and azimuth.
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 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 275 70 -10 3.88 0.3441 WVFGRD96 2.0 90 75 -25 4.00 0.4382 WVFGRD96 3.0 95 80 -15 4.04 0.4695 WVFGRD96 4.0 95 85 -15 4.07 0.4819 WVFGRD96 5.0 95 90 -15 4.10 0.4847 WVFGRD96 6.0 275 80 10 4.13 0.4858 WVFGRD96 7.0 275 80 10 4.15 0.4841 WVFGRD96 8.0 275 80 15 4.18 0.4803 WVFGRD96 9.0 275 80 15 4.19 0.4724 WVFGRD96 10.0 275 80 15 4.21 0.4645 WVFGRD96 11.0 275 80 15 4.22 0.4566 WVFGRD96 12.0 275 80 15 4.23 0.4486 WVFGRD96 13.0 275 80 15 4.24 0.4400 WVFGRD96 14.0 275 80 15 4.25 0.4314 WVFGRD96 15.0 275 80 15 4.26 0.4230 WVFGRD96 16.0 275 75 10 4.27 0.4147 WVFGRD96 17.0 275 75 10 4.28 0.4064 WVFGRD96 18.0 275 75 10 4.28 0.3982 WVFGRD96 19.0 275 75 10 4.29 0.3897 WVFGRD96 20.0 275 75 15 4.30 0.3820 WVFGRD96 21.0 275 75 15 4.30 0.3754 WVFGRD96 22.0 275 75 15 4.31 0.3683 WVFGRD96 23.0 275 75 15 4.31 0.3620 WVFGRD96 24.0 275 75 15 4.32 0.3558 WVFGRD96 25.0 90 80 15 4.30 0.3485 WVFGRD96 26.0 90 85 10 4.31 0.3442 WVFGRD96 27.0 90 85 15 4.31 0.3405 WVFGRD96 28.0 90 85 15 4.32 0.3369 WVFGRD96 29.0 90 85 15 4.32 0.3334
The best solution is
WVFGRD96 6.0 275 80 10 4.13 0.4858
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 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 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