The ANSS event ID is ak023g35jxin and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak023g35jxin/executive.
2023/12/16 19:24:39 60.248 -153.613 188.2 4.7 Alaska
USGS/SLU Moment Tensor Solution ENS 2023/12/16 19:24:39:0 60.25 -153.61 188.2 4.7 Alaska Stations used: AK.BAE AK.BRLK AK.CAST AK.CNP AK.CUT AK.FID AK.GHO AK.GLI AK.HIN AK.HOM AK.J19K AK.J20K AK.K20K AK.KLU AK.KNK AK.KTH AK.L20K AK.L22K AK.M16K AK.N15K AK.N18K AK.O14K AK.O18K AK.O19K AK.P16K AK.P17K AK.P23K AK.PPLA AK.RC01 AK.SAW AK.SCM AK.SKN AK.SLK AK.SWD AK.TRF AK.WAT6 AT.PMR AV.RED AV.STLK II.KDAK Filtering commands used: cut o DIST/3.7 -60 o DIST/3.7 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 9.66e+22 dyne-cm Mw = 4.59 Z = 202 km Plane Strike Dip Rake NP1 5 80 75 NP2 242 18 146 Principal Axes: Axis Value Plunge Azimuth T 9.66e+22 53 257 N 0.00e+00 15 8 P -9.66e+22 33 108 Moment Tensor: (dyne-cm) Component Value Mxx -4.52e+21 Mxy 2.70e+22 Mxz 3.32e+21 Myy -2.74e+22 Myz -8.77e+22 Mzz 3.19e+22 ---------##### ----------###---###### -------##########--------### -----#############-----------# ----################-------------# ----#################--------------- ---###################---------------- ---####################----------------- --#####################----------------- ---#####################------------------ --######################------------------ --######## ##########------------------- --######## T ##########---------- ------ -######## ##########---------- P ----- -#####################---------- ----- #####################----------------- ###################----------------- ##################---------------- ###############--------------- ##############-------------- ##########------------ ######-------- Global CMT Convention Moment Tensor: R T P 3.19e+22 3.32e+21 8.77e+22 3.32e+21 -4.52e+21 -2.70e+22 8.77e+22 -2.70e+22 -2.74e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20231216192439/index.html |
STK = 5 DIP = 80 RAKE = 75 MW = 4.59 HS = 202.0
The NDK file is 20231216192439.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 2023/12/16 19:24:39:0 60.25 -153.61 188.2 4.7 Alaska Stations used: AK.BAE AK.BRLK AK.CAST AK.CNP AK.CUT AK.FID AK.GHO AK.GLI AK.HIN AK.HOM AK.J19K AK.J20K AK.K20K AK.KLU AK.KNK AK.KTH AK.L20K AK.L22K AK.M16K AK.N15K AK.N18K AK.O14K AK.O18K AK.O19K AK.P16K AK.P17K AK.P23K AK.PPLA AK.RC01 AK.SAW AK.SCM AK.SKN AK.SLK AK.SWD AK.TRF AK.WAT6 AT.PMR AV.RED AV.STLK II.KDAK Filtering commands used: cut o DIST/3.7 -60 o DIST/3.7 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 9.66e+22 dyne-cm Mw = 4.59 Z = 202 km Plane Strike Dip Rake NP1 5 80 75 NP2 242 18 146 Principal Axes: Axis Value Plunge Azimuth T 9.66e+22 53 257 N 0.00e+00 15 8 P -9.66e+22 33 108 Moment Tensor: (dyne-cm) Component Value Mxx -4.52e+21 Mxy 2.70e+22 Mxz 3.32e+21 Myy -2.74e+22 Myz -8.77e+22 Mzz 3.19e+22 ---------##### ----------###---###### -------##########--------### -----#############-----------# ----################-------------# ----#################--------------- ---###################---------------- ---####################----------------- --#####################----------------- ---#####################------------------ --######################------------------ --######## ##########------------------- --######## T ##########---------- ------ -######## ##########---------- P ----- -#####################---------- ----- #####################----------------- ###################----------------- ##################---------------- ###############--------------- ##############-------------- ##########------------ ######-------- Global CMT Convention Moment Tensor: R T P 3.19e+22 3.32e+21 8.77e+22 3.32e+21 -4.52e+21 -2.70e+22 8.77e+22 -2.70e+22 -2.74e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20231216192439/index.html |
W-phase Moment Tensor (Mww) Moment 1.607e+16 N-m Magnitude 4.74 Mww Depth 180.5 km Percent DC 60% Half Duration 0.61 s Catalog US Data Source US 3 Contributor US 3 Nodal Planes Plane Strike Dip Rake NP1 265 11 156 NP2 19 86 80 Principal Axes Axis Value Plunge Azimuth T 1.753e+16 48 279 N -0.349e+16 10 20 P -1.404e+16 40 118 |
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/3.7 -60 o DIST/3.7 +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 100.0 255 55 -70 4.29 0.1367 WVFGRD96 102.0 250 55 -75 4.29 0.1400 WVFGRD96 104.0 255 55 -70 4.30 0.1440 WVFGRD96 106.0 255 55 -70 4.31 0.1503 WVFGRD96 108.0 250 50 -60 4.31 0.1568 WVFGRD96 110.0 250 50 -55 4.32 0.1632 WVFGRD96 112.0 250 50 -55 4.32 0.1686 WVFGRD96 114.0 250 50 -55 4.33 0.1723 WVFGRD96 116.0 250 50 -55 4.33 0.1745 WVFGRD96 118.0 215 70 50 4.41 0.1846 WVFGRD96 120.0 220 65 50 4.42 0.2021 WVFGRD96 122.0 225 60 55 4.42 0.2208 WVFGRD96 124.0 55 45 55 4.38 0.2501 WVFGRD96 126.0 55 45 55 4.40 0.2856 WVFGRD96 128.0 55 45 55 4.42 0.3232 WVFGRD96 130.0 55 45 55 4.43 0.3627 WVFGRD96 132.0 55 45 55 4.45 0.4137 WVFGRD96 134.0 25 60 55 4.48 0.4520 WVFGRD96 136.0 20 65 55 4.49 0.4873 WVFGRD96 138.0 20 65 55 4.50 0.5226 WVFGRD96 140.0 20 65 55 4.51 0.5387 WVFGRD96 142.0 15 70 55 4.52 0.5474 WVFGRD96 144.0 15 70 55 4.52 0.5524 WVFGRD96 146.0 15 70 55 4.52 0.5567 WVFGRD96 148.0 15 70 55 4.52 0.5619 WVFGRD96 150.0 15 70 55 4.53 0.5663 WVFGRD96 152.0 15 70 55 4.53 0.5694 WVFGRD96 154.0 15 70 55 4.53 0.5747 WVFGRD96 156.0 15 70 55 4.53 0.5785 WVFGRD96 158.0 15 70 55 4.54 0.5815 WVFGRD96 160.0 15 70 55 4.54 0.5869 WVFGRD96 162.0 15 70 55 4.54 0.5902 WVFGRD96 164.0 15 70 55 4.54 0.5938 WVFGRD96 166.0 15 70 55 4.55 0.5977 WVFGRD96 168.0 15 70 55 4.55 0.6015 WVFGRD96 170.0 15 70 55 4.55 0.6044 WVFGRD96 162.0 15 70 55 4.54 0.5902 WVFGRD96 164.0 15 70 55 4.54 0.5938 WVFGRD96 166.0 15 70 55 4.55 0.5977 WVFGRD96 168.0 15 70 55 4.55 0.6015 WVFGRD96 180.0 5 80 70 4.57 0.6211 WVFGRD96 182.0 5 80 70 4.57 0.6247 WVFGRD96 184.0 5 80 70 4.57 0.6309 WVFGRD96 186.0 5 80 70 4.57 0.6344 WVFGRD96 188.0 5 80 70 4.58 0.6381 WVFGRD96 190.0 5 80 70 4.58 0.6426 WVFGRD96 192.0 5 80 70 4.58 0.6457 WVFGRD96 194.0 5 80 70 4.58 0.6486 WVFGRD96 196.0 5 80 75 4.58 0.6511 WVFGRD96 198.0 5 80 75 4.58 0.6536 WVFGRD96 200.0 5 80 75 4.59 0.6548 WVFGRD96 202.0 5 80 75 4.59 0.6565 WVFGRD96 204.0 5 80 75 4.59 0.6561 WVFGRD96 206.0 5 80 75 4.59 0.6558 WVFGRD96 208.0 5 80 75 4.59 0.6540
The best solution is
WVFGRD96 202.0 5 80 75 4.59 0.6565
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/3.7 -60 o DIST/3.7 +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 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