The ANSS event ID is ak0196r9o3rq and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak0196r9o3rq/executive.
2019/05/27 09:52:21 58.856 -152.358 64.0 5.8 Alaska
USGS/SLU Moment Tensor Solution ENS 2019/05/27 09:52:21:0 58.86 -152.36 64.0 5.8 Alaska Stations used: AK.BRLK AK.CNP AK.FID AK.GHO AK.GLI AK.HIN AK.HOM AK.KNK AK.PWL AK.SLK AK.SWD AT.OHAK AV.ACH AV.ILSW AV.RED II.KDAK TA.L18K TA.M17K TA.N17K TA.N18K TA.N19K TA.O16K TA.O18K TA.O19K TA.O22K TA.P18K TA.P23K TA.Q19K TA.R16K Filtering commands used: cut o DIST/3.3 -50 o DIST/3.3 +60 rtr taper w 0.1 hp c 0.01 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 7.76e+24 dyne-cm Mw = 5.86 Z = 70 km Plane Strike Dip Rake NP1 327 69 148 NP2 70 60 25 Principal Axes: Axis Value Plunge Azimuth T 7.76e+24 38 286 N 0.00e+00 52 117 P -7.76e+24 5 20 Moment Tensor: (dyne-cm) Component Value Mxx -6.42e+24 Mxy -3.75e+24 Mxz 3.38e+23 Myy 3.58e+24 Myz -3.87e+24 Mzz 2.84e+24 ------------ P ---------------- --- ######---------------------- ##########-------------------- ##############-------------------- #################------------------- ####################------------------ ######################-----------------# ###### ##############---------------## ####### T ################------------#### ####### #################---------###### ############################-------####### #############################---########## ############################-########### ########################-----########### --################-----------######### -----------------------------####### ----------------------------###### --------------------------#### -------------------------### ---------------------- -------------- Global CMT Convention Moment Tensor: R T P 2.84e+24 3.38e+23 3.87e+24 3.38e+23 -6.42e+24 3.75e+24 3.87e+24 3.75e+24 3.58e+24 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20190527095221/index.html |
STK = 70 DIP = 60 RAKE = 25 MW = 5.86 HS = 70.0
The NDK file is 20190527095221.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 -50 o DIST/3.3 +60 rtr taper w 0.1 hp c 0.01 n 3 lp c 0.05 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 30.0 215 55 -25 5.47 0.3040 WVFGRD96 32.0 55 65 -20 5.50 0.3128 WVFGRD96 34.0 55 65 -15 5.52 0.3256 WVFGRD96 36.0 60 70 -15 5.56 0.3409 WVFGRD96 38.0 60 70 -15 5.58 0.3599 WVFGRD96 40.0 65 60 15 5.66 0.3868 WVFGRD96 42.0 65 60 15 5.68 0.4050 WVFGRD96 44.0 65 55 20 5.69 0.4233 WVFGRD96 46.0 65 55 20 5.71 0.4409 WVFGRD96 48.0 65 60 20 5.73 0.4582 WVFGRD96 50.0 70 55 25 5.75 0.4755 WVFGRD96 52.0 70 55 25 5.77 0.4919 WVFGRD96 54.0 70 55 25 5.78 0.5068 WVFGRD96 56.0 70 55 30 5.79 0.5200 WVFGRD96 58.0 70 55 30 5.81 0.5319 WVFGRD96 60.0 70 55 30 5.82 0.5416 WVFGRD96 62.0 70 55 30 5.83 0.5493 WVFGRD96 64.0 70 60 25 5.84 0.5550 WVFGRD96 66.0 70 60 25 5.85 0.5593 WVFGRD96 68.0 70 60 25 5.85 0.5621 WVFGRD96 70.0 70 60 25 5.86 0.5630 WVFGRD96 72.0 70 60 30 5.86 0.5622 WVFGRD96 74.0 70 60 30 5.87 0.5602 WVFGRD96 76.0 70 60 30 5.87 0.5569 WVFGRD96 78.0 70 60 30 5.87 0.5523 WVFGRD96 80.0 70 60 25 5.87 0.5466 WVFGRD96 82.0 65 65 20 5.88 0.5411 WVFGRD96 84.0 65 65 20 5.88 0.5355 WVFGRD96 86.0 65 65 20 5.88 0.5294 WVFGRD96 88.0 65 65 20 5.88 0.5227 WVFGRD96 90.0 65 70 20 5.89 0.5164 WVFGRD96 92.0 65 70 20 5.89 0.5103 WVFGRD96 94.0 65 70 20 5.89 0.5040 WVFGRD96 96.0 65 70 15 5.89 0.4976 WVFGRD96 98.0 65 70 15 5.89 0.4911
The best solution is
WVFGRD96 70.0 70 60 25 5.86 0.5630
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 -50 o DIST/3.3 +60 rtr taper w 0.1 hp c 0.01 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