The ANSS event ID is ak024d0dutqb and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak024d0dutqb/executive.
2024/10/09 21:44:36 61.422 -139.993 5.8 3.4 NWT, Canada
USGS/SLU Moment Tensor Solution ENS 2024/10/09 21:44:36:0 61.42 -139.99 5.8 3.4 NWT, Canada Stations used: AK.BARN AK.DOT AK.HIN AK.L26K AK.LOGN AK.MCAR AK.MESA AK.PIN AK.SCRK AK.TGL AK.VRDI AK.YAH CN.BVCY CN.HYT 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 0.10 n 3 Best Fitting Double Couple Mo = 2.75e+21 dyne-cm Mw = 3.56 Z = 6 km Plane Strike Dip Rake NP1 105 55 90 NP2 285 35 90 Principal Axes: Axis Value Plunge Azimuth T 2.75e+21 80 15 N 0.00e+00 -0 285 P -2.75e+21 10 195 Moment Tensor: (dyne-cm) Component Value Mxx -2.41e+21 Mxy -6.47e+20 Mxz 9.10e+20 Myy -1.73e+20 Myz 2.44e+20 Mzz 2.59e+21 -------------- ---------------------- ---------------------------- ----------####---------------- -----###################---------- ---#########################-------- -###############################------ -##################################----- ################### ##############---- --################## T ###############---- ---################# ################--- -----###################################-- -------##################################- ---------############################### ------------###########################- ----------------##################---- ------------------------------------ ---------------------------------- ------------------------------ -------- ----------------- ----- P -------------- - ---------- Global CMT Convention Moment Tensor: R T P 2.59e+21 9.10e+20 -2.44e+20 9.10e+20 -2.41e+21 6.47e+20 -2.44e+20 6.47e+20 -1.73e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20241009214436/index.html |
STK = 285 DIP = 35 RAKE = 90 MW = 3.56 HS = 6.0
The NDK file is 20241009214436.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.
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:
cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 245 20 15 3.61 0.2875 WVFGRD96 2.0 240 30 15 3.51 0.3057 WVFGRD96 3.0 245 30 30 3.50 0.3175 WVFGRD96 4.0 280 30 85 3.56 0.3503 WVFGRD96 5.0 105 55 90 3.57 0.3790 WVFGRD96 6.0 285 35 90 3.56 0.3938 WVFGRD96 7.0 100 55 85 3.56 0.3936 WVFGRD96 8.0 280 40 85 3.55 0.3838 WVFGRD96 9.0 95 55 75 3.54 0.3744 WVFGRD96 10.0 85 60 65 3.55 0.3667 WVFGRD96 11.0 85 60 65 3.55 0.3531 WVFGRD96 12.0 80 65 55 3.54 0.3409 WVFGRD96 13.0 225 65 -45 3.54 0.3306 WVFGRD96 14.0 230 65 -40 3.54 0.3202 WVFGRD96 15.0 230 70 -45 3.55 0.3099 WVFGRD96 16.0 230 65 -40 3.55 0.3010 WVFGRD96 17.0 230 65 -40 3.56 0.2930 WVFGRD96 18.0 230 70 -45 3.56 0.2852 WVFGRD96 19.0 230 70 -45 3.57 0.2782 WVFGRD96 20.0 230 70 -50 3.60 0.2712 WVFGRD96 21.0 230 65 -45 3.60 0.2646 WVFGRD96 22.0 230 70 -50 3.61 0.2582 WVFGRD96 23.0 230 70 -50 3.61 0.2523 WVFGRD96 24.0 230 65 -45 3.61 0.2465 WVFGRD96 25.0 230 65 -45 3.62 0.2408 WVFGRD96 26.0 230 65 -45 3.62 0.2350 WVFGRD96 27.0 230 65 -45 3.63 0.2293 WVFGRD96 28.0 230 65 -45 3.63 0.2233 WVFGRD96 29.0 230 65 -45 3.63 0.2168
The best solution is
WVFGRD96 6.0 285 35 90 3.56 0.3938
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 0.10 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