2008/06/05 07:13:15 38.4469 -87.8673 17.5 3.60 Illinois
USGS Felt map for this earthquake
SLU Moment Tensor Solution 2008/06/05 07:13:15 38.4469 -87.8673 17.5 3.60 Illinois Best Fitting Double Couple Mo = 1.43e+21 dyne-cm Mw = 3.37 Z = 17 km Plane Strike Dip Rake NP1 305 90 20 NP2 215 70 180 Principal Axes: Axis Value Plunge Azimuth T 1.43e+21 14 172 N 0.00e+00 70 305 P -1.43e+21 14 78 Moment Tensor: (dyne-cm) Component Value Mxx 1.26e+21 Mxy -4.59e+20 Mxz -4.00e+20 Myy -1.26e+21 Myz -2.80e+20 Mzz 1.19e+13 ############## ###################### #######################----- #####################--------- #####################------------- ---#################---------------- -------############------------------- -----------########----------------- - -------------####------------------- P - ------------------------------------- -- ---------------#####---------------------- --------------########-------------------- -------------############----------------- -----------################------------- -----------##################----------- ---------######################------- -------##########################--- ------############################ ---########################### --############# ########## ############ T ####### ######## ### Harvard Convention Moment Tensor: R T F 1.19e+13 -4.00e+20 2.80e+20 -4.00e+20 1.26e+21 4.59e+20 2.80e+20 4.59e+20 -1.26e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20080605071315/index.html |
STK = 305 DIP = 90 RAKE = 20 MW = 3.37 HS = 17.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution 2008/06/05 07:13:15 38.4469 -87.8673 17.5 3.60 Illinois Best Fitting Double Couple Mo = 1.43e+21 dyne-cm Mw = 3.37 Z = 17 km Plane Strike Dip Rake NP1 305 90 20 NP2 215 70 180 Principal Axes: Axis Value Plunge Azimuth T 1.43e+21 14 172 N 0.00e+00 70 305 P -1.43e+21 14 78 Moment Tensor: (dyne-cm) Component Value Mxx 1.26e+21 Mxy -4.59e+20 Mxz -4.00e+20 Myy -1.26e+21 Myz -2.80e+20 Mzz 1.19e+13 ############## ###################### #######################----- #####################--------- #####################------------- ---#################---------------- -------############------------------- -----------########----------------- - -------------####------------------- P - ------------------------------------- -- ---------------#####---------------------- --------------########-------------------- -------------############----------------- -----------################------------- -----------##################----------- ---------######################------- -------##########################--- ------############################ ---########################### --############# ########## ############ T ####### ######## ### Harvard Convention Moment Tensor: R T F 1.19e+13 -4.00e+20 2.80e+20 -4.00e+20 1.26e+21 4.59e+20 2.80e+20 4.59e+20 -1.26e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20080605071315/index.html |
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:
hp c 0.05 n 3 lp c 0.20 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 145 70 60 3.24 0.5557 WVFGRD96 1.0 145 65 55 3.23 0.5673 WVFGRD96 2.0 320 75 30 3.12 0.5854 WVFGRD96 3.0 315 80 20 3.13 0.6158 WVFGRD96 4.0 310 85 15 3.17 0.6447 WVFGRD96 5.0 130 90 -15 3.19 0.6628 WVFGRD96 6.0 310 85 10 3.20 0.6775 WVFGRD96 7.0 310 85 10 3.21 0.6877 WVFGRD96 8.0 130 90 -25 3.23 0.6943 WVFGRD96 9.0 130 90 -15 3.24 0.7015 WVFGRD96 10.0 310 85 20 3.27 0.7091 WVFGRD96 11.0 130 90 -30 3.29 0.7146 WVFGRD96 12.0 130 90 -30 3.30 0.7359 WVFGRD96 13.0 310 85 20 3.31 0.7559 WVFGRD96 14.0 310 85 20 3.32 0.7650 WVFGRD96 15.0 305 90 20 3.35 0.7620 WVFGRD96 16.0 305 85 10 3.37 0.7706 WVFGRD96 17.0 305 90 20 3.37 0.7795 WVFGRD96 18.0 305 85 15 3.38 0.7685 WVFGRD96 19.0 310 80 10 3.37 0.7662 WVFGRD96 20.0 310 80 15 3.38 0.7716 WVFGRD96 21.0 310 80 15 3.39 0.7504 WVFGRD96 22.0 310 80 20 3.40 0.7570 WVFGRD96 23.0 310 80 25 3.41 0.7480 WVFGRD96 24.0 315 75 25 3.40 0.7371 WVFGRD96 25.0 315 75 25 3.41 0.7432 WVFGRD96 26.0 315 75 25 3.41 0.7247 WVFGRD96 27.0 315 75 30 3.42 0.7345 WVFGRD96 28.0 315 75 25 3.42 0.7180 WVFGRD96 29.0 315 75 30 3.43 0.7238
The best solution is
WVFGRD96 17.0 305 90 20 3.37 0.7795
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 componnet is plotted to the same scale and peak amplitudes are indicated by the numbers to the left of each trace. The number in black at the rightr of each predicted traces 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 bandpass filter used in the processing and for the display was
hp c 0.05 n 3 lp c 0.20 n 3
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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. |
Should the national backbone of the USGS Advanced National Seismic System (ANSS) be implemented with an interstation separation of 300 km, it is very likely that an earthquake such as this would have been recorded at distances on the order of 100-200 km. This means that the closest station would have information on source depth and mechanism that was lacking here.
Dr. Harley Benz, USGS, provided the USGS USNSN digital data. The digital data used in this study were provided by Natural Resources Canada through their AUTODRM site http://www.seismo.nrcan.gc.ca/nwfa/autodrm/autodrm_req_e.php, and IRIS using their BUD interface.
Thanks also to the many seismic network operators whose dedication make this effort possible: University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureas of Mines, UC Berkely, Caltech, UC San Diego, Saint L ouis University, Universityof Memphis, Lamont Doehrty Earth Observatory, Boston College, the Iris stations and the Transportable Array of EarthScope.
The CUS used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
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
Here we tabulate the reasons for not using certain digital data sets
The following stations did not have a valid response files:
DATE=Fri Jun 20 09:26:41 CDT 2008