The ANSS event ID is NONE and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/NONE/executive.
2011/05/21 08:33:21 65.369 -166.891 19.0 5/2 Alaska
USGS/SLU Moment Tensor Solution ENS 2011/05/21 08:33:21:0 65.37 -166.89 19.0 5.0 Alaska Stations used: AK.BPAW AK.CHUM AK.COLD AK.GAMB AK.MLY AK.PPLA AK.TNA IU.COLA 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 0.06 n 3 Best Fitting Double Couple Mo = 1.41e+23 dyne-cm Mw = 4.70 Z = 9 km Plane Strike Dip Rake NP1 120 50 -75 NP2 277 42 -107 Principal Axes: Axis Value Plunge Azimuth T 1.41e+23 4 199 N 0.00e+00 11 290 P -1.41e+23 78 91 Moment Tensor: (dyne-cm) Component Value Mxx 1.25e+23 Mxy 4.42e+22 Mxz -8.77e+21 Myy 9.34e+21 Myz -3.22e+22 Mzz -1.34e+23 ############## ###################### ############################ ############################## ################################## #######-------------------########## -###---------------------------####### ----------------------------------###### -##---------------------------------#### #####----------------------------------### ######----------------- --------------## #######---------------- P ---------------# #########-------------- ---------------- #########------------------------------- ############---------------------------- #############------------------------- ################-------------------- ####################-----------### ############################## ############################ ### ################ T ############ Global CMT Convention Moment Tensor: R T P -1.34e+23 -8.77e+21 3.22e+22 -8.77e+21 1.25e+23 -4.42e+22 3.22e+22 -4.42e+22 9.34e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20110521083321/index.html |
STK = 120 DIP = 50 RAKE = -75 MW = 4.70 HS = 9.0
The NDK file is 20110521083321.ndk The waveform inversion is preferred.
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.
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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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 335 75 -20 4.29 0.3991 WVFGRD96 1.0 335 75 -15 4.31 0.4113 WVFGRD96 2.0 330 65 -30 4.47 0.4417 WVFGRD96 3.0 145 60 -40 4.52 0.4531 WVFGRD96 4.0 140 60 -50 4.55 0.5235 WVFGRD96 5.0 140 60 -50 4.55 0.5919 WVFGRD96 6.0 135 55 -55 4.57 0.6463 WVFGRD96 7.0 125 50 -65 4.60 0.6835 WVFGRD96 8.0 125 50 -70 4.69 0.7181 WVFGRD96 9.0 120 50 -75 4.70 0.7427 WVFGRD96 10.0 120 50 -75 4.69 0.7420 WVFGRD96 11.0 115 50 -80 4.70 0.7308 WVFGRD96 12.0 115 50 -80 4.69 0.7120 WVFGRD96 13.0 110 50 -85 4.70 0.6876 WVFGRD96 14.0 285 40 -95 4.70 0.6662 WVFGRD96 15.0 285 40 -95 4.69 0.6435 WVFGRD96 16.0 90 75 80 4.72 0.6391 WVFGRD96 17.0 90 70 75 4.73 0.6386 WVFGRD96 18.0 90 70 75 4.73 0.6371 WVFGRD96 19.0 90 75 75 4.75 0.6351 WVFGRD96 20.0 90 75 75 4.75 0.6325 WVFGRD96 21.0 90 70 70 4.77 0.6310 WVFGRD96 22.0 90 70 70 4.78 0.6283 WVFGRD96 23.0 90 70 70 4.79 0.6245 WVFGRD96 24.0 90 70 70 4.80 0.6195 WVFGRD96 25.0 90 70 70 4.80 0.6131 WVFGRD96 26.0 90 70 65 4.82 0.6061 WVFGRD96 27.0 90 70 65 4.83 0.6022 WVFGRD96 28.0 90 70 65 4.84 0.5960 WVFGRD96 29.0 90 70 65 4.84 0.5870
The best solution is
WVFGRD96 9.0 120 50 -75 4.70 0.7427
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 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