The ANSS event ID is usp000h0gp and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000h0gp/executive.
2009/08/17 00:22:12 38.470 -102.684 5.0 3.9 Colorado
USGS/SLU Moment Tensor Solution ENS 2009/08/17 00:22:12:0 38.47 -102.68 5.0 3.9 Colorado Stations used: TA.KSCO TA.P26A TA.P27A TA.P28A TA.P29A TA.P30A TA.Q25A TA.Q26A TA.Q28A TA.Q29A TA.R23A TA.R25A TA.R26A TA.R27A TA.R28A TA.R29A TA.R30A TA.R31A TA.S25A TA.S26A TA.S27A TA.S28A TA.S29A TA.S30A TA.T25A TA.T26A TA.T27A TA.T28A TA.T29A TA.U25A TA.U26A TA.U27A TA.U28A TA.U29A Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 7.50e+21 dyne-cm Mw = 3.85 Z = 10 km Plane Strike Dip Rake NP1 70 50 -80 NP2 235 41 -102 Principal Axes: Axis Value Plunge Azimuth T 7.50e+21 5 153 N 0.00e+00 8 244 P -7.50e+21 81 33 Moment Tensor: (dyne-cm) Component Value Mxx 5.78e+21 Mxy -3.10e+21 Mxz -1.49e+21 Myy 1.49e+21 Myz -3.48e+20 Mzz -7.27e+21 ############## ###################### ############################ ################------------## #############--------------------- ###########------------------------- ##########---------------------------- #########------------------------------# #######------------- ----------------# #######-------------- P ---------------### ######--------------- --------------#### #####--------------------------------##### #####------------------------------####### ###-----------------------------######## ###--------------------------########### -#-----------------------############# -###---------------################# ################################## ############################## ###################### ### ################### T ############## Global CMT Convention Moment Tensor: R T P -7.27e+21 -1.49e+21 3.48e+20 -1.49e+21 5.78e+21 3.10e+21 3.48e+20 3.10e+21 1.49e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20090817002212/index.html |
STK = 70 DIP = 50 RAKE = -80 MW = 3.85 HS = 10.0
The NDK file is 20090817002212.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 2009/08/17 00:22:12:0 38.47 -102.68 5.0 3.9 Colorado Stations used: TA.KSCO TA.P26A TA.P27A TA.P28A TA.P29A TA.P30A TA.Q25A TA.Q26A TA.Q28A TA.Q29A TA.R23A TA.R25A TA.R26A TA.R27A TA.R28A TA.R29A TA.R30A TA.R31A TA.S25A TA.S26A TA.S27A TA.S28A TA.S29A TA.S30A TA.T25A TA.T26A TA.T27A TA.T28A TA.T29A TA.U25A TA.U26A TA.U27A TA.U28A TA.U29A Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 7.50e+21 dyne-cm Mw = 3.85 Z = 10 km Plane Strike Dip Rake NP1 70 50 -80 NP2 235 41 -102 Principal Axes: Axis Value Plunge Azimuth T 7.50e+21 5 153 N 0.00e+00 8 244 P -7.50e+21 81 33 Moment Tensor: (dyne-cm) Component Value Mxx 5.78e+21 Mxy -3.10e+21 Mxz -1.49e+21 Myy 1.49e+21 Myz -3.48e+20 Mzz -7.27e+21 ############## ###################### ############################ ################------------## #############--------------------- ###########------------------------- ##########---------------------------- #########------------------------------# #######------------- ----------------# #######-------------- P ---------------### ######--------------- --------------#### #####--------------------------------##### #####------------------------------####### ###-----------------------------######## ###--------------------------########### -#-----------------------############# -###---------------################# ################################## ############################## ###################### ### ################### T ############## Global CMT Convention Moment Tensor: R T P -7.27e+21 -1.49e+21 3.48e+20 -1.49e+21 5.78e+21 3.10e+21 3.48e+20 3.10e+21 1.49e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20090817002212/index.html |
First motion plot using elocate take-off angles and azimuths |
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:
hp c 0.02 n 3 lp c 0.10 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 100 85 -70 3.85 0.3432 WVFGRD96 1.0 100 85 -70 3.87 0.3437 WVFGRD96 2.0 100 85 -60 3.76 0.3576 WVFGRD96 3.0 100 85 -55 3.73 0.3759 WVFGRD96 4.0 70 65 -80 3.79 0.4107 WVFGRD96 5.0 70 60 -80 3.80 0.4487 WVFGRD96 6.0 70 55 -80 3.81 0.4732 WVFGRD96 7.0 70 55 -80 3.81 0.4908 WVFGRD96 8.0 70 55 -80 3.81 0.4982 WVFGRD96 9.0 70 50 -80 3.82 0.4991 WVFGRD96 10.0 70 50 -80 3.85 0.4995 WVFGRD96 11.0 70 50 -80 3.84 0.4900 WVFGRD96 12.0 75 50 -75 3.84 0.4762 WVFGRD96 13.0 75 50 -75 3.84 0.4599 WVFGRD96 14.0 85 55 -65 3.83 0.4433 WVFGRD96 15.0 90 55 -55 3.83 0.4271 WVFGRD96 16.0 90 55 -55 3.83 0.4111 WVFGRD96 17.0 95 60 -50 3.83 0.3949 WVFGRD96 18.0 95 60 -50 3.83 0.3792 WVFGRD96 19.0 95 60 -45 3.84 0.3632 WVFGRD96 20.0 95 60 -50 3.86 0.3544 WVFGRD96 21.0 95 60 -45 3.87 0.3418 WVFGRD96 22.0 95 60 -45 3.87 0.3299 WVFGRD96 23.0 95 60 -45 3.87 0.3194 WVFGRD96 24.0 95 60 -45 3.88 0.3098 WVFGRD96 25.0 95 60 -45 3.88 0.3018 WVFGRD96 26.0 95 60 -45 3.89 0.2943 WVFGRD96 27.0 275 55 -45 3.92 0.2892 WVFGRD96 28.0 275 55 -45 3.92 0.2858 WVFGRD96 29.0 275 55 -45 3.93 0.2821
The best solution is
WVFGRD96 10.0 70 50 -80 3.85 0.4995
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
hp c 0.02 n 3 lp c 0.10 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 CUS.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 CUS Model with Q from simple gamma values 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 1.0000 5.0000 2.8900 2.5000 0.172E-02 0.387E-02 0.00 0.00 1.00 1.00 9.0000 6.1000 3.5200 2.7300 0.160E-02 0.363E-02 0.00 0.00 1.00 1.00 10.0000 6.4000 3.7000 2.8200 0.149E-02 0.336E-02 0.00 0.00 1.00 1.00 20.0000 6.7000 3.8700 2.9020 0.000E-04 0.000E-04 0.00 0.00 1.00 1.00 0.0000 8.1500 4.7000 3.3640 0.194E-02 0.431E-02 0.00 0.00 1.00 1.00