The ANSS event ID is usp000d8x3 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000d8x3/executive.
2004/11/21 15:50:32 44.412 -114.080 5.0 3.9 Idaho
USGS/SLU Moment Tensor Solution ENS 2004/11/21 15:50:32:0 44.41 -114.08 5.0 3.9 Idaho Stations used: IW.REDW US.AHID US.BOZ US.BW06 US.HLID US.HWUT US.LKWY US.MSO UU.BGU WY.YMR 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 0.07 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 6.10e+21 dyne-cm Mw = 3.79 Z = 12 km Plane Strike Dip Rake NP1 335 65 -50 NP2 92 46 -144 Principal Axes: Axis Value Plunge Azimuth T 6.10e+21 11 37 N 0.00e+00 36 135 P -6.10e+21 52 293 Moment Tensor: (dyne-cm) Component Value Mxx 3.36e+21 Mxy 3.65e+21 Mxz -2.32e+20 Myy 2.18e+20 Myz 3.42e+21 Mzz -3.58e+21 ############## -----################# ----------############### -------------############# T # -----------------########### ### -------------------################# ----------------------################ ---------- -----------################ ---------- P ------------############### ----------- -------------############### ----------------------------############## #---------------------------############## ##---------------------------###########-- ###-------------------------##########-- #####------------------------######----- ########--------------------###------- ############-------------##--------- ###########################------- #########################----- #######################----- ####################-- ############## Global CMT Convention Moment Tensor: R T P -3.58e+21 -2.32e+20 -3.42e+21 -2.32e+20 3.36e+21 -3.65e+21 -3.42e+21 -3.65e+21 2.18e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20041121155032/index.html |
STK = 335 DIP = 65 RAKE = -50 MW = 3.79 HS = 12.0
The NDK file is 20041121155032.ndk The waveform inversion is preferred.
![]() |
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.
![]() |
|
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 165 85 5 3.49 0.4980 WVFGRD96 2.0 165 85 0 3.56 0.5597 WVFGRD96 3.0 345 90 0 3.59 0.5594 WVFGRD96 4.0 350 80 40 3.68 0.5595 WVFGRD96 5.0 175 80 60 3.76 0.5831 WVFGRD96 6.0 175 75 55 3.76 0.6033 WVFGRD96 7.0 175 80 55 3.74 0.6143 WVFGRD96 8.0 170 85 60 3.80 0.6177 WVFGRD96 9.0 340 80 -60 3.79 0.6218 WVFGRD96 10.0 330 65 -60 3.80 0.6341 WVFGRD96 11.0 335 65 -55 3.79 0.6437 WVFGRD96 12.0 335 65 -50 3.79 0.6468 WVFGRD96 13.0 335 65 -50 3.79 0.6460 WVFGRD96 14.0 340 70 -45 3.79 0.6452 WVFGRD96 15.0 340 70 -40 3.80 0.6426 WVFGRD96 16.0 340 70 -40 3.80 0.6384 WVFGRD96 17.0 340 70 -40 3.81 0.6327 WVFGRD96 18.0 340 70 -40 3.81 0.6261 WVFGRD96 19.0 340 70 -35 3.82 0.6189 WVFGRD96 20.0 345 75 -35 3.82 0.6117 WVFGRD96 21.0 345 75 -35 3.83 0.6039 WVFGRD96 22.0 345 75 -35 3.83 0.5958 WVFGRD96 23.0 345 75 -35 3.84 0.5869 WVFGRD96 24.0 345 75 -35 3.85 0.5773 WVFGRD96 25.0 345 75 -35 3.85 0.5671 WVFGRD96 26.0 345 80 -30 3.87 0.5566 WVFGRD96 27.0 345 80 -30 3.87 0.5463 WVFGRD96 28.0 345 80 -30 3.88 0.5358 WVFGRD96 29.0 345 80 -30 3.89 0.5252
The best solution is
WVFGRD96 12.0 335 65 -50 3.79 0.6468
The mechanism corresponding to the best fit is
![]() |
|
The best fit as a function of depth is given in the following figure:
![]() |
|
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 br c 0.12 0.25 n 4 p 2
![]() |
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. |
![]() |
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 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.
![]() |
|
The surface-wave determined focal mechanism is shown here.
NODAL PLANES STK= 184.99 DIP= 70.00 RAKE= 45.00 OR STK= 76.11 DIP= 48.36 RAKE= 152.76 DEPTH = 16.0 km Mw = 3.86 Best Fit 0.8471 - P-T axis plot gives solutions with FIT greater than FIT90
![]() |
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.
![]() |
|
![]() |
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 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