The ANSS event ID is ak0163bfjfdc and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0163bfjfdc/executive.
2016/03/12 21:57:55 60.261 -152.304 99.8 4.7 Alaska
USGS/SLU Moment Tensor Solution ENS 2016/03/12 21:57:55:0 60.26 -152.30 99.8 4.7 Alaska Stations used: AK.BRLK AK.CAPN AK.CNP AK.CUT AK.FIRE AK.HOM AK.KNK AK.RC01 AK.SWD AT.PMR AT.SVW2 AV.ILSW TA.L19K TA.M19K TA.M22K TA.N19K TA.O19K TA.O22K TA.P18K Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.41e+23 dyne-cm Mw = 4.70 Z = 90 km Plane Strike Dip Rake NP1 235 75 -20 NP2 330 71 -164 Principal Axes: Axis Value Plunge Azimuth T 1.41e+23 3 283 N 0.00e+00 65 20 P -1.41e+23 25 192 Moment Tensor: (dyne-cm) Component Value Mxx -1.04e+23 Mxy -5.52e+22 Mxz 5.40e+22 Myy 1.28e+23 Myz 4.14e+21 Mzz -2.42e+22 -------------- ##-------------------- #######--------------------- ###########------------------- ##############-------------------- #################------------####### ###################------############# ####################-################# T ##################---################# ###############-------################# ################----------################ ##############-------------############### ###########-----------------############## #########-------------------############ #######---------------------############ ####------------------------########## ##-------------------------######### ---------------------------####### ---------- ------------##### --------- P ------------#### ------ ------------# -------------- Global CMT Convention Moment Tensor: R T P -2.42e+22 5.40e+22 -4.14e+21 5.40e+22 -1.04e+23 5.52e+22 -4.14e+21 5.52e+22 1.28e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20160312215755/index.html |
STK = 235 DIP = 75 RAKE = -20 MW = 4.70 HS = 90.0
The NDK file is 20160312215755.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 2016/03/12 21:57:55:0 60.26 -152.30 99.8 4.7 Alaska Stations used: AK.BRLK AK.CAPN AK.CNP AK.CUT AK.FIRE AK.HOM AK.KNK AK.RC01 AK.SWD AT.PMR AT.SVW2 AV.ILSW TA.L19K TA.M19K TA.M22K TA.N19K TA.O19K TA.O22K TA.P18K Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3 Best Fitting Double Couple Mo = 1.41e+23 dyne-cm Mw = 4.70 Z = 90 km Plane Strike Dip Rake NP1 235 75 -20 NP2 330 71 -164 Principal Axes: Axis Value Plunge Azimuth T 1.41e+23 3 283 N 0.00e+00 65 20 P -1.41e+23 25 192 Moment Tensor: (dyne-cm) Component Value Mxx -1.04e+23 Mxy -5.52e+22 Mxz 5.40e+22 Myy 1.28e+23 Myz 4.14e+21 Mzz -2.42e+22 -------------- ##-------------------- #######--------------------- ###########------------------- ##############-------------------- #################------------####### ###################------############# ####################-################# T ##################---################# ###############-------################# ################----------################ ##############-------------############### ###########-----------------############## #########-------------------############ #######---------------------############ ####------------------------########## ##-------------------------######### ---------------------------####### ---------- ------------##### --------- P ------------#### ------ ------------# -------------- Global CMT Convention Moment Tensor: R T P -2.42e+22 5.40e+22 -4.14e+21 5.40e+22 -1.04e+23 5.52e+22 -4.14e+21 5.52e+22 1.28e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20160312215755/index.html |
Regional Moment Tensor (Mwr) Moment 1.328e+16 N-m Magnitude 4.68 Depth 92.0 km Percent DC 64% Half Duration – Catalog US (us10004x3k) Data Source US3 Contributor US3 Nodal Planes Plane Strike Dip Rake NP1 235 74 -9 NP2 327 81 -164 Principal Axes Axis Value Plunge Azimuth T 1.182 5 100 N 0.255 72 355 P -1.437 18 192 |
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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 2.0 55 75 15 3.81 0.2638 WVFGRD96 4.0 50 90 -10 3.88 0.3245 WVFGRD96 6.0 55 90 -15 3.96 0.3637 WVFGRD96 8.0 50 85 -15 4.02 0.3965 WVFGRD96 10.0 50 85 -15 4.06 0.4146 WVFGRD96 12.0 50 80 -10 4.09 0.4237 WVFGRD96 14.0 50 85 -10 4.12 0.4264 WVFGRD96 16.0 50 85 -10 4.14 0.4265 WVFGRD96 18.0 50 85 -10 4.16 0.4240 WVFGRD96 20.0 230 90 10 4.18 0.4215 WVFGRD96 22.0 50 90 -10 4.20 0.4210 WVFGRD96 24.0 50 90 -10 4.21 0.4218 WVFGRD96 26.0 230 90 10 4.23 0.4244 WVFGRD96 28.0 50 90 -5 4.25 0.4294 WVFGRD96 30.0 230 90 5 4.26 0.4351 WVFGRD96 32.0 230 90 0 4.28 0.4408 WVFGRD96 34.0 50 90 5 4.30 0.4456 WVFGRD96 36.0 50 90 5 4.33 0.4496 WVFGRD96 38.0 230 85 -5 4.36 0.4544 WVFGRD96 40.0 230 85 -10 4.40 0.4634 WVFGRD96 42.0 230 85 -10 4.42 0.4689 WVFGRD96 44.0 230 85 -15 4.44 0.4746 WVFGRD96 46.0 230 80 -15 4.47 0.4795 WVFGRD96 48.0 230 80 -20 4.49 0.4860 WVFGRD96 50.0 230 80 -20 4.51 0.4934 WVFGRD96 52.0 230 80 -20 4.52 0.5005 WVFGRD96 54.0 230 75 -25 4.55 0.5095 WVFGRD96 56.0 230 75 -20 4.55 0.5187 WVFGRD96 58.0 230 70 -25 4.59 0.5286 WVFGRD96 60.0 230 70 -25 4.60 0.5375 WVFGRD96 62.0 230 70 -25 4.61 0.5477 WVFGRD96 64.0 230 70 -25 4.62 0.5563 WVFGRD96 66.0 230 70 -25 4.63 0.5637 WVFGRD96 68.0 230 70 -25 4.64 0.5712 WVFGRD96 70.0 230 70 -20 4.64 0.5784 WVFGRD96 72.0 235 75 -25 4.65 0.5842 WVFGRD96 74.0 235 75 -25 4.66 0.5895 WVFGRD96 76.0 235 75 -20 4.66 0.5946 WVFGRD96 78.0 235 75 -20 4.66 0.5987 WVFGRD96 80.0 235 75 -20 4.67 0.6021 WVFGRD96 82.0 235 75 -20 4.68 0.6047 WVFGRD96 84.0 235 75 -20 4.68 0.6069 WVFGRD96 86.0 235 75 -20 4.69 0.6075 WVFGRD96 88.0 235 75 -20 4.69 0.6087 WVFGRD96 90.0 235 75 -20 4.70 0.6087 WVFGRD96 92.0 235 75 -20 4.70 0.6078 WVFGRD96 94.0 235 75 -15 4.70 0.6066 WVFGRD96 96.0 235 75 -15 4.71 0.6054 WVFGRD96 98.0 235 75 -15 4.71 0.6046 WVFGRD96 100.0 235 80 -15 4.70 0.6039 WVFGRD96 102.0 235 80 -15 4.70 0.6024 WVFGRD96 104.0 235 80 -15 4.71 0.6004 WVFGRD96 106.0 60 80 45 4.72 0.5998 WVFGRD96 108.0 60 80 45 4.72 0.6012
The best solution is
WVFGRD96 90.0 235 75 -20 4.70 0.6087
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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 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