2011/11/05 07:12:45 35.570 -96.703 5 4.70 Arizona
USGS Felt map for this earthquake
USGS/SLU Moment Tensor Solution ENS 2011/11/05 07:12:45:0 35.57 -96.70 5.0 4.7 Arizona Stations used: AG.CCAR AG.FCAR AG.HHAR AG.LCAR AG.WHAR AG.WLAR IU.CCM NM.MGMO NM.PBMO NM.UALR TA.P34A TA.P35A TA.Q34A TA.Q35A TA.Q36A TA.Q37A TA.R34A TA.R35A TA.R36A TA.R37A TA.R38A TA.R39A TA.R40A TA.R41A TA.S34A TA.S35A TA.S36A TA.S37A TA.S38A TA.S39A TA.S40A TA.S41A TA.T34A TA.T35A TA.T36A TA.T37A TA.T38A TA.T39A TA.T40A TA.T41A TA.TUL1 TA.U35A TA.U36A TA.U37A TA.U38A TA.U39A TA.U41A TA.V35A TA.V36A TA.V37A TA.V38A TA.V39A TA.V40A TA.V41A TA.W35A TA.W36A TA.W37B TA.W38A TA.W39A TA.W40A TA.W41B TA.WHTX TA.X35A TA.X36A TA.X37A TA.X38A TA.Y35A TA.Y36A TA.Y37A TA.Y38A TA.Y39A TA.Z37A TA.Z38A US.CBKS US.KSU1 US.MIAR US.WMOK Filtering commands used: hp c 0.02 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.41e+23 dyne-cm Mw = 4.70 Z = 3 km Plane Strike Dip Rake NP1 32 80 -170 NP2 300 80 -10 Principal Axes: Axis Value Plunge Azimuth T 1.41e+23 0 166 N 0.00e+00 76 75 P -1.41e+23 14 256 Moment Tensor: (dyne-cm) Component Value Mxx 1.25e+23 Mxy -6.49e+22 Mxz 7.88e+21 Myy -1.17e+23 Myz 3.24e+22 Mzz -8.39e+21 ############## ###################### ########################---- #########################----- ##########################-------- -#########################---------- --------##################------------ -------------##############------------- -----------------#########-------------- ---------------------#####---------------- ------------------------#----------------- -----------------------####--------------- -- -----------------########------------ - P ----------------############-------- - ---------------###############------ ----------------###################--- --------------###################### ------------###################### --------###################### -----####################### ############### #### ########### T Global CMT Convention Moment Tensor: R T P -8.39e+21 7.88e+21 -3.24e+22 7.88e+21 1.25e+23 6.49e+22 -3.24e+22 6.49e+22 -1.17e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20111105071245/index.html |
STK = 300 DIP = 80 RAKE = -10 MW = 4.70 HS = 3.0
The NDK file is 20111105071245.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2011/11/05 07:12:45:0 35.57 -96.70 5.0 4.7 Arizona Stations used: AG.CCAR AG.FCAR AG.HHAR AG.LCAR AG.WHAR AG.WLAR IU.CCM NM.MGMO NM.PBMO NM.UALR TA.P34A TA.P35A TA.Q34A TA.Q35A TA.Q36A TA.Q37A TA.R34A TA.R35A TA.R36A TA.R37A TA.R38A TA.R39A TA.R40A TA.R41A TA.S34A TA.S35A TA.S36A TA.S37A TA.S38A TA.S39A TA.S40A TA.S41A TA.T34A TA.T35A TA.T36A TA.T37A TA.T38A TA.T39A TA.T40A TA.T41A TA.TUL1 TA.U35A TA.U36A TA.U37A TA.U38A TA.U39A TA.U41A TA.V35A TA.V36A TA.V37A TA.V38A TA.V39A TA.V40A TA.V41A TA.W35A TA.W36A TA.W37B TA.W38A TA.W39A TA.W40A TA.W41B TA.WHTX TA.X35A TA.X36A TA.X37A TA.X38A TA.Y35A TA.Y36A TA.Y37A TA.Y38A TA.Y39A TA.Z37A TA.Z38A US.CBKS US.KSU1 US.MIAR US.WMOK Filtering commands used: hp c 0.02 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.41e+23 dyne-cm Mw = 4.70 Z = 3 km Plane Strike Dip Rake NP1 32 80 -170 NP2 300 80 -10 Principal Axes: Axis Value Plunge Azimuth T 1.41e+23 0 166 N 0.00e+00 76 75 P -1.41e+23 14 256 Moment Tensor: (dyne-cm) Component Value Mxx 1.25e+23 Mxy -6.49e+22 Mxz 7.88e+21 Myy -1.17e+23 Myz 3.24e+22 Mzz -8.39e+21 ############## ###################### ########################---- #########################----- ##########################-------- -#########################---------- --------##################------------ -------------##############------------- -----------------#########-------------- ---------------------#####---------------- ------------------------#----------------- -----------------------####--------------- -- -----------------########------------ - P ----------------############-------- - ---------------###############------ ----------------###################--- --------------###################### ------------###################### --------###################### -----####################### ############### #### ########### T Global CMT Convention Moment Tensor: R T P -8.39e+21 7.88e+21 -3.24e+22 7.88e+21 1.25e+23 6.49e+22 -3.24e+22 6.49e+22 -1.17e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20111105071245/index.html |
(a) mLg computed using the IASPEI formula; (b) mLg residuals ; the values used for the trimmed mean are indicated.
(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:
hp c 0.02 n 3 lp c 0.07 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 295 70 -20 4.52 0.4237 WVFGRD96 1.0 300 80 -15 4.54 0.4546 WVFGRD96 2.0 295 70 -20 4.67 0.5549 WVFGRD96 3.0 300 80 -10 4.70 0.5851 WVFGRD96 4.0 120 85 0 4.72 0.5844 WVFGRD96 5.0 120 80 0 4.75 0.5721 WVFGRD96 6.0 120 75 0 4.78 0.5599 WVFGRD96 7.0 120 70 0 4.80 0.5551 WVFGRD96 8.0 120 65 0 4.84 0.5587 WVFGRD96 9.0 120 65 0 4.85 0.5526 WVFGRD96 10.0 120 65 0 4.86 0.5486 WVFGRD96 11.0 300 90 25 4.86 0.5437 WVFGRD96 12.0 120 90 -25 4.87 0.5405 WVFGRD96 13.0 120 90 -25 4.87 0.5359 WVFGRD96 14.0 120 90 -25 4.88 0.5304 WVFGRD96 15.0 120 90 -25 4.89 0.5238 WVFGRD96 16.0 120 90 -25 4.90 0.5168 WVFGRD96 17.0 300 90 25 4.91 0.5088 WVFGRD96 18.0 120 90 -25 4.92 0.5009 WVFGRD96 19.0 120 90 -25 4.92 0.4925 WVFGRD96 20.0 120 90 -25 4.93 0.4834 WVFGRD96 21.0 300 85 25 4.94 0.4754 WVFGRD96 22.0 120 90 -25 4.95 0.4648 WVFGRD96 23.0 120 90 -25 4.95 0.4550 WVFGRD96 24.0 300 85 25 4.96 0.4482 WVFGRD96 25.0 300 85 25 4.96 0.4395 WVFGRD96 26.0 300 85 25 4.97 0.4311 WVFGRD96 27.0 300 85 25 4.97 0.4226 WVFGRD96 28.0 300 85 25 4.98 0.4146 WVFGRD96 29.0 300 85 25 4.99 0.4066
The best solution is
WVFGRD96 3.0 300 80 -10 4.70 0.5851
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
hp c 0.02 n 3 lp c 0.07 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. |
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 following figure shows the stations used in the grid search for the best focal mechanism to fit the surface-wave spectral amplitudes of the Love and Rayleigh waves.
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The surface-wave determined focal mechanism is shown here.
NODAL PLANES STK= 29.99 DIP= 90.00 RAKE= -165.00 OR STK= 299.99 DIP= 75.00 RAKE= 0.00 DEPTH = 5.0 km Mw = 4.93 Best Fit 0.8008 - P-T axis plot gives solutions with FIT greater than FIT90
The P-wave first motion data for focal mechanism studies are as follow:
Sta Az Dist First motion
Surface wave analysis was performed using codes from Computer Programs in Seismology, specifically the multiple filter analysis program do_mft and the surface-wave radiation pattern search program srfgrd96.
Digital data were collected, instrument response removed and traces converted
to Z, R an T components. Multiple filter analysis was applied to the Z and T traces to obtain the Rayleigh- and Love-wave spectral amplitudes, respectively.
These were input to the search program which examined all depths between 1 and 25 km
and all possible mechanisms.
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Pressure-tension axis trends. Since the surface-wave spectra search does not distinguish between P and T axes and since there is a 180 ambiguity in strike, all possible P and T axes are plotted. First motion data and waveforms will be used to select the preferred mechanism. The purpose of this plot is to provide an idea of the possible range of solutions. The P and T-axes for all mechanisms with goodness of fit greater than 0.9 FITMAX (above) are plotted here. |
Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to the Love and Rayleigh wave radiation patterns. 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. Because of the symmetry of the spectral amplitude rediation patterns, only strikes from 0-180 degrees are sampled. |
The distribution of broadband stations with azimuth and distance is
Listing of broadband stations used
Since the analysis of the surface-wave radiation patterns uses only spectral amplitudes and because the surfave-wave radiation patterns have a 180 degree symmetry, each surface-wave solution consists of four possible focal mechanisms corresponding to the interchange of the P- and T-axes and a roation of the mechanism by 180 degrees. To select one mechanism, P-wave first motion can be used. This was not possible in this case because all the P-wave first motions were emergent ( a feature of the P-wave wave takeoff angle, the station location and the mechanism). The other way to select among the mechanisms is to compute forward synthetics and compare the observed and predicted waveforms.
The fits to the waveforms with the given mechanism are show below:
This figure shows the fit to the three components of motion (Z - vertical, R-radial and T - transverse). For each station and component, the observed traces is shown in red and the model predicted trace in blue. The traces represent filtered ground velocity in units of meters/sec (the peak value is printed adjacent to each trace; each pair of traces to plotted to the same scale to emphasize the difference in levels). Both synthetic and observed traces have been filtered using the SAC commands:
hp c 0.02 n 3 lp c 0.07 n 3
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 Bureas of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Iris stations and the Transportable Array of EarthScope.
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: