The ANSS event ID is ak0147utj430 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0147utj430/executive.
2014/06/20 01:06:22 63.133 -149.311 82.1 4.2 Alaska
USGS/SLU Moment Tensor Solution ENS 2014/06/20 01:06:22:0 63.13 -149.31 82.1 4.2 Alaska Stations used: AK.BPAW AK.BRLK AK.CCB AK.CNP AK.CRQ AK.DHY AK.FID AK.FYU AK.GHO AK.HIN AK.MCAR AK.MCK AK.PAX AK.RAG AK.RC01 AK.RIDG AK.RND AK.SAW AK.SCM AK.TRF AK.VRDI AK.WRH AT.PMR IM.IL31 IU.COLA Filtering commands used: cut a -30 a 180 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 2.79e+22 dyne-cm Mw = 4.23 Z = 86 km Plane Strike Dip Rake NP1 110 75 25 NP2 13 66 164 Principal Axes: Axis Value Plunge Azimuth T 2.79e+22 28 333 N 0.00e+00 61 139 P -2.79e+22 6 240 Moment Tensor: (dyne-cm) Component Value Mxx 1.05e+22 Mxy -2.06e+22 Mxz 1.18e+22 Myy -1.64e+22 Myz -2.65e+21 Mzz 5.89e+21 ############-- #################----- ###### ###########-------- ####### T ############-------- ######### ############---------- #########################----------- ##########################------------ -##########################------------- ---########################------------- -------#####################-------------- ----------#################--------------- -------------##############--------------- ------------------#########--------------- ----------------------###--------------- ------------------------#####----------- - -------------------############### P ------------------############### -----------------############### ----------------############## --------------############## ---------############# ---########### Global CMT Convention Moment Tensor: R T P 5.89e+21 1.18e+22 2.65e+21 1.18e+22 1.05e+22 2.06e+22 2.65e+21 2.06e+22 -1.64e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20140620010622/index.html |
STK = 110 DIP = 75 RAKE = 25 MW = 4.23 HS = 86.0
The NDK file is 20140620010622.ndk The waveform inversion is preferred.
The following compares this source inversion to those provided by others. The purpose is to look for major differences and also to note slight differences that might be inherent to the processing procedure. For completeness the USGS/SLU solution is repeated from above.
USGS/SLU Moment Tensor Solution ENS 2014/06/20 01:06:22:0 63.13 -149.31 82.1 4.2 Alaska Stations used: AK.BPAW AK.BRLK AK.CCB AK.CNP AK.CRQ AK.DHY AK.FID AK.FYU AK.GHO AK.HIN AK.MCAR AK.MCK AK.PAX AK.RAG AK.RC01 AK.RIDG AK.RND AK.SAW AK.SCM AK.TRF AK.VRDI AK.WRH AT.PMR IM.IL31 IU.COLA Filtering commands used: cut a -30 a 180 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 2.79e+22 dyne-cm Mw = 4.23 Z = 86 km Plane Strike Dip Rake NP1 110 75 25 NP2 13 66 164 Principal Axes: Axis Value Plunge Azimuth T 2.79e+22 28 333 N 0.00e+00 61 139 P -2.79e+22 6 240 Moment Tensor: (dyne-cm) Component Value Mxx 1.05e+22 Mxy -2.06e+22 Mxz 1.18e+22 Myy -1.64e+22 Myz -2.65e+21 Mzz 5.89e+21 ############-- #################----- ###### ###########-------- ####### T ############-------- ######### ############---------- #########################----------- ##########################------------ -##########################------------- ---########################------------- -------#####################-------------- ----------#################--------------- -------------##############--------------- ------------------#########--------------- ----------------------###--------------- ------------------------#####----------- - -------------------############### P ------------------############### -----------------############### ----------------############## --------------############## ---------############# ---########### Global CMT Convention Moment Tensor: R T P 5.89e+21 1.18e+22 2.65e+21 1.18e+22 1.05e+22 2.06e+22 2.65e+21 2.06e+22 -1.64e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20140620010622/index.html |
Moment 2.92e+15 N-m Magnitude 4.2 Percent DC 82% Depth 86.0 km Updated 2014-06-20 01:50:47 UTC Author us Catalog us Contributor us Code us_c000rii9_mwr Principal Axes Axis Value Plunge Azimuth T 3.040 28 336 N -0.259 61 136 P -2.781 8 242 Nodal Planes Plane Strike Dip Rake NP1 112° 77 26 NP2 16° 65 166 |
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 a -30 a 180 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 2.0 195 65 -20 3.47 0.1995 WVFGRD96 4.0 260 80 -5 3.51 0.2430 WVFGRD96 6.0 260 85 0 3.56 0.2711 WVFGRD96 8.0 85 75 5 3.61 0.2955 WVFGRD96 10.0 85 75 -5 3.65 0.3131 WVFGRD96 12.0 85 75 -5 3.68 0.3254 WVFGRD96 14.0 90 75 5 3.69 0.3359 WVFGRD96 16.0 90 75 5 3.71 0.3481 WVFGRD96 18.0 90 75 5 3.73 0.3581 WVFGRD96 20.0 90 75 5 3.75 0.3668 WVFGRD96 22.0 95 75 5 3.77 0.3760 WVFGRD96 24.0 95 75 10 3.78 0.3849 WVFGRD96 26.0 95 75 10 3.80 0.3933 WVFGRD96 28.0 95 75 10 3.82 0.4011 WVFGRD96 30.0 100 75 10 3.84 0.4082 WVFGRD96 32.0 100 75 10 3.86 0.4150 WVFGRD96 34.0 105 75 15 3.88 0.4219 WVFGRD96 36.0 105 75 15 3.91 0.4278 WVFGRD96 38.0 105 75 10 3.94 0.4347 WVFGRD96 40.0 105 65 20 4.00 0.4556 WVFGRD96 42.0 105 65 20 4.02 0.4662 WVFGRD96 44.0 105 65 20 4.04 0.4768 WVFGRD96 46.0 105 65 20 4.06 0.4862 WVFGRD96 48.0 110 65 20 4.08 0.4962 WVFGRD96 50.0 110 65 20 4.10 0.5059 WVFGRD96 52.0 110 65 25 4.11 0.5159 WVFGRD96 54.0 110 65 25 4.12 0.5247 WVFGRD96 56.0 110 70 20 4.13 0.5327 WVFGRD96 58.0 110 70 25 4.14 0.5413 WVFGRD96 60.0 110 70 25 4.15 0.5492 WVFGRD96 62.0 110 70 25 4.16 0.5569 WVFGRD96 64.0 110 70 25 4.17 0.5631 WVFGRD96 66.0 110 70 25 4.18 0.5698 WVFGRD96 68.0 110 70 25 4.18 0.5746 WVFGRD96 70.0 110 70 25 4.19 0.5784 WVFGRD96 72.0 110 75 25 4.19 0.5830 WVFGRD96 74.0 110 75 25 4.20 0.5871 WVFGRD96 76.0 110 75 25 4.21 0.5904 WVFGRD96 78.0 110 75 25 4.21 0.5924 WVFGRD96 80.0 110 75 25 4.22 0.5940 WVFGRD96 82.0 110 75 25 4.22 0.5952 WVFGRD96 84.0 110 75 25 4.23 0.5962 WVFGRD96 86.0 110 75 25 4.23 0.5965 WVFGRD96 88.0 110 75 25 4.24 0.5960 WVFGRD96 90.0 110 80 25 4.24 0.5957 WVFGRD96 92.0 110 80 25 4.24 0.5956 WVFGRD96 94.0 110 80 25 4.25 0.5950 WVFGRD96 96.0 110 80 30 4.24 0.5942 WVFGRD96 98.0 110 80 30 4.25 0.5928 WVFGRD96 100.0 110 80 30 4.25 0.5912 WVFGRD96 102.0 110 80 30 4.26 0.5893 WVFGRD96 104.0 110 80 30 4.26 0.5873 WVFGRD96 106.0 110 80 30 4.26 0.5853 WVFGRD96 108.0 110 80 30 4.27 0.5831 WVFGRD96 110.0 110 80 30 4.27 0.5802 WVFGRD96 112.0 110 80 30 4.27 0.5772 WVFGRD96 114.0 110 85 30 4.27 0.5738 WVFGRD96 116.0 110 85 30 4.28 0.5710 WVFGRD96 118.0 110 85 35 4.27 0.5686
The best solution is
WVFGRD96 86.0 110 75 25 4.23 0.5965
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 a -30 a 180 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 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