The ANSS event ID is ak020804cj04 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak020804cj04/executive.
2020/06/22 21:56:16 64.689 -150.889 24.1 3.8 Alaska
USGS/SLU Moment Tensor Solution ENS 2020/06/22 21:56:16:0 64.69 -150.89 24.1 3.8 Alaska Stations used: AK.CAST AK.CCB AK.DHY AK.H21K AK.H22K AK.H23K AK.H24K AK.HDA AK.I21K AK.I23K AK.I26K AK.J17K AK.J19K AK.J20K AK.J25K AK.K20K AK.KLU AK.KNK AK.L18K AK.L19K AK.L22K AK.L26K AK.M20K AK.MCK AK.MLY AK.NEA2 AK.PAX AK.PPD AK.PPLA AK.RIDG AK.RND AK.TRF AK.WRH AT.MENT AT.PMR AV.STLK IM.IL31 IU.COLA TA.E21K TA.E23K TA.E24K TA.F19K TA.F20K TA.F21K TA.F24K TA.F25K TA.G18K TA.G19K TA.G21K TA.G23K TA.G24K TA.G26K TA.H17K TA.H18K TA.H19K TA.I20K TA.K17K 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 = 4.32e+21 dyne-cm Mw = 3.69 Z = 22 km Plane Strike Dip Rake NP1 180 70 -50 NP2 292 44 -150 Principal Axes: Axis Value Plunge Azimuth T 4.32e+21 15 242 N 0.00e+00 37 344 P -4.32e+21 49 133 Moment Tensor: (dyne-cm) Component Value Mxx -4.56e+14 Mxy 2.61e+21 Mxz 9.49e+20 Myy 2.12e+21 Myz -2.53e+21 Mzz -2.12e+21 ------######## ---------############# -----------################# ------------################## ------#######----################# --############---------############# ###############-------------########## ###############----------------######### ###############------------------####### ################--------------------###### ################---------------------##### ################----------------------#### ################-----------------------### ###############----------- ----------# ### #########----------- P ----------# ## T ##########---------- ---------- # ##########---------------------- #############--------------------- ############------------------ ###########----------------- #########------------- ######-------- Global CMT Convention Moment Tensor: R T P -2.12e+21 9.49e+20 2.53e+21 9.49e+20 -4.56e+14 -2.61e+21 2.53e+21 -2.61e+21 2.12e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20200622215616/index.html |
STK = 180 DIP = 70 RAKE = -50 MW = 3.69 HS = 22.0
The NDK file is 20200622215616.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: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated.
Right: residuals as a function of distance and azimuth.
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 1.0 335 45 90 3.14 0.2349 WVFGRD96 2.0 155 45 90 3.30 0.3211 WVFGRD96 3.0 145 45 80 3.32 0.2595 WVFGRD96 4.0 285 60 -10 3.25 0.2494 WVFGRD96 5.0 280 55 -15 3.28 0.2616 WVFGRD96 6.0 280 50 -10 3.30 0.2770 WVFGRD96 7.0 15 80 45 3.33 0.3066 WVFGRD96 8.0 20 80 45 3.40 0.3349 WVFGRD96 9.0 20 75 45 3.43 0.3660 WVFGRD96 10.0 20 75 45 3.46 0.3954 WVFGRD96 11.0 185 75 -45 3.48 0.4278 WVFGRD96 12.0 185 70 -45 3.51 0.4636 WVFGRD96 13.0 185 70 -45 3.54 0.4984 WVFGRD96 14.0 180 65 -45 3.56 0.5317 WVFGRD96 15.0 180 65 -45 3.58 0.5624 WVFGRD96 16.0 180 65 -45 3.60 0.5894 WVFGRD96 17.0 180 65 -45 3.62 0.6123 WVFGRD96 18.0 180 70 -45 3.64 0.6315 WVFGRD96 19.0 180 70 -45 3.65 0.6473 WVFGRD96 20.0 180 70 -45 3.67 0.6581 WVFGRD96 21.0 180 70 -50 3.68 0.6647 WVFGRD96 22.0 180 70 -50 3.69 0.6681 WVFGRD96 23.0 180 70 -50 3.70 0.6662 WVFGRD96 24.0 180 70 -50 3.71 0.6618 WVFGRD96 25.0 180 70 -50 3.72 0.6539 WVFGRD96 26.0 175 70 -55 3.73 0.6443 WVFGRD96 27.0 180 75 -55 3.73 0.6328 WVFGRD96 28.0 180 75 -55 3.74 0.6200 WVFGRD96 29.0 180 75 -55 3.74 0.6056 WVFGRD96 30.0 180 75 -55 3.75 0.5909 WVFGRD96 31.0 180 75 -55 3.75 0.5727 WVFGRD96 32.0 180 75 -55 3.75 0.5561 WVFGRD96 33.0 185 80 -55 3.75 0.5387 WVFGRD96 34.0 185 80 -55 3.76 0.5222 WVFGRD96 35.0 185 80 -55 3.76 0.5079 WVFGRD96 36.0 185 80 -55 3.76 0.4928 WVFGRD96 37.0 185 80 -55 3.76 0.4798 WVFGRD96 38.0 185 80 -55 3.76 0.4679 WVFGRD96 39.0 180 80 -50 3.77 0.4569 WVFGRD96 40.0 180 80 -60 3.87 0.4432 WVFGRD96 41.0 180 80 -60 3.87 0.4309 WVFGRD96 42.0 185 80 -55 3.87 0.4187 WVFGRD96 43.0 185 80 -55 3.87 0.4074 WVFGRD96 44.0 185 80 -50 3.87 0.3979 WVFGRD96 45.0 185 80 -50 3.87 0.3883 WVFGRD96 46.0 175 80 -50 3.88 0.3794 WVFGRD96 47.0 175 80 -50 3.88 0.3717 WVFGRD96 48.0 175 80 -50 3.88 0.3635 WVFGRD96 49.0 175 80 -50 3.89 0.3567 WVFGRD96 50.0 175 80 -45 3.89 0.3485 WVFGRD96 51.0 175 80 -45 3.89 0.3420 WVFGRD96 52.0 175 80 -45 3.89 0.3348 WVFGRD96 53.0 175 80 -45 3.89 0.3285 WVFGRD96 54.0 175 80 -45 3.90 0.3234 WVFGRD96 55.0 175 80 -45 3.90 0.3177 WVFGRD96 56.0 175 80 -45 3.90 0.3132 WVFGRD96 57.0 175 80 -45 3.90 0.3093 WVFGRD96 58.0 175 80 -45 3.90 0.3045 WVFGRD96 59.0 175 80 -45 3.91 0.3009
The best solution is
WVFGRD96 22.0 180 70 -50 3.69 0.6681
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 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