Location

Location ANSS

The ANSS event ID is ak018em0mbpl and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak018em0mbpl/executive.

2018/11/14 06:25:02 64.774 -150.917 18.0 3.8 Alaska

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2018/11/14 06:25:02:0 64.77 -150.92 18.0 3.8 Alaska Stations used: AK.BPAW AK.BWN AK.CAST AK.CCB AK.DHY AK.GHO AK.HDA AK.KTH AK.MCK AK.MLY AK.NEA2 AK.RND AK.SCRK AK.SKN AK.TRF AK.WRH AT.MENT IM.IL31 IU.COLA TA.E19K TA.E21K TA.E22K TA.E23K TA.E24K TA.F19K TA.F20K TA.F21K TA.F24K TA.F26K TA.G18K TA.G19K TA.G21K TA.G23K TA.G24K TA.H17K TA.H18K TA.H19K TA.H21K TA.H23K TA.H24K TA.I21K TA.I23K TA.J18K TA.J19K TA.J20K TA.J25K TA.J26L TA.K17K TA.K20K TA.K27K TA.L18K TA.L19K TA.M19K TA.M20K TA.M24K TA.POKR TA.TOLK Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 4.47e+21 dyne-cm Mw = 3.70 Z = 12 km Plane Strike Dip Rake NP1 35 80 15 NP2 302 75 170 Principal Axes: Axis Value Plunge Azimuth T 4.47e+21 18 259 N 0.00e+00 72 68 P -4.47e+21 3 168 Moment Tensor: (dyne-cm) Component Value Mxx -4.12e+21 Mxy 1.64e+21 Mxz 9.39e+18 Myy 3.73e+21 Myz -1.32e+21 Mzz 3.95e+20 -------------- ---------------------- --------------------------## --------------------------#### ---------------------------####### #####----------------------######### ###########----------------########### ################-----------############# ####################------############## ########################--################ #########################-################ ## ##################------############# ## T #################---------########### # ################------------######## ##################----------------###### ################-------------------### #############----------------------# ###########----------------------- #######----------------------- ####------------------------ -------------- ----- ---------- P - Global CMT Convention Moment Tensor: R T P 3.95e+20 9.39e+18 1.32e+21 9.39e+18 -4.12e+21 -1.64e+21 1.32e+21 -1.64e+21 3.73e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20181114062502/index.html

Preferred Solution

The preferred solution from an analysis of the surface-wave spectral amplitude radiation pattern, waveform inversion or first motion observations is

      STK = 35
      DIP = 80
     RAKE = 15
       MW = 3.70
       HS = 12.0

The NDK file is 20181114062502.ndk The waveform inversion is preferred.

Magnitudes

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 M_L by application of the respective IASPEI formulae. As a research study, the linear distance term of the IASPEI formula for M_L is adjusted to remove a linear distance trend in residuals to give a regionally defined M_L. The defined M_L 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.

mLg Magnitude

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.

ML Magnitude

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.

Context

The left panel of the next figure presents the focal mechanism for this earthquake (red) in the context of other nearby events (blue) in the SLU Moment Tensor Catalog. The right panel shows the inferred direction of maximum compressive stress and the type of faulting (green is strike-slip, red is normal, blue is thrust; oblique is shown by a combination of colors). Thus context plot is useful for assessing the appropriateness of the moment tensor of this event.

Waveform Inversion using wvfgrd96

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.

Location of broadband stations used for waveform inversion

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 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.10 n 3 
br c 0.12 0.25 n 4 p 2

The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0    35    90     0   3.24 0.3343
WVFGRD96    2.0    35    90     5   3.43 0.5723
WVFGRD96    3.0   215    90    -5   3.49 0.6548
WVFGRD96    4.0   215    90   -10   3.53 0.6963
WVFGRD96    5.0   215    90   -25   3.57 0.7218
WVFGRD96    6.0    35    85    25   3.59 0.7479
WVFGRD96    7.0    35    80    20   3.61 0.7692
WVFGRD96    8.0    35    80    25   3.65 0.7856
WVFGRD96    9.0    35    80    20   3.66 0.7971
WVFGRD96   10.0    35    80    20   3.68 0.8064
WVFGRD96   11.0    35    80    20   3.69 0.8130
WVFGRD96   12.0    35    80    15   3.70 0.8182
WVFGRD96   13.0   215    90   -15   3.71 0.8154
WVFGRD96   14.0   215    90   -15   3.72 0.8172
WVFGRD96   15.0   215    90   -15   3.74 0.8164
WVFGRD96   16.0   215    90   -10   3.75 0.8151
WVFGRD96   17.0   215    90   -10   3.76 0.8113
WVFGRD96   18.0   215    90   -10   3.77 0.8062
WVFGRD96   19.0    35    85    10   3.78 0.8017
WVFGRD96   20.0    35    85    15   3.79 0.7933
WVFGRD96   21.0    35    85    15   3.80 0.7835
WVFGRD96   22.0   215    90   -10   3.81 0.7709
WVFGRD96   23.0    35    85    15   3.81 0.7599
WVFGRD96   24.0    35    85    15   3.82 0.7467
WVFGRD96   25.0    35    85    15   3.83 0.7321
WVFGRD96   26.0    35    85    15   3.83 0.7173
WVFGRD96   27.0   215    90   -15   3.84 0.7023
WVFGRD96   28.0   215    90   -15   3.84 0.6874
WVFGRD96   29.0    35    90    15   3.85 0.6735

The best solution is

WVFGRD96   12.0    35    80    15   3.70 0.8182

The mechanism corresponding to the best fit is

Figure 1. Waveform inversion focal mechanism

The best fit as a function of depth is given in the following figure:

Figure 2. Depth sensitivity for waveform mechanism

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 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.10 n 3 
br c 0.12 0.25 n 4 p 2

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.

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:

The origin time and epicentral distance are incorrect
The velocity model used for the inversion is incorrect
The velocity model used to define the P-arrival time is not the same as the velocity model used for the waveform inversion (assuming that the initial trace alignment is based on the P arrival time)

Assuming only a mislocation, the time shifts are fit to a functional form:

 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.

Velocity Model

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

Last Changed Fri Apr 26 03:41:34 AM CDT 2024