The ANSS event ID is ak01720vwz40 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/ak01720vwz40/executive.
2017/02/13 07:17:12 62.512 -142.748 8.9 5.3 Alaska
USGS/SLU Moment Tensor Solution
ENS 2017/02/13 07:17:12:0 62.51 -142.75 8.9 5.3 Alaska
Stations used:
AK.BARN AK.BCP AK.BWN AK.CCB AK.CUT AK.DHY AK.DIV AK.DOT
AK.EYAK AK.FIRE AK.GLB AK.HDA AK.KLU AK.MCAR AK.MDM AK.NEA2
AK.PAX AK.PIN AK.PPD AK.PWL AK.RC01 AK.RIDG AK.SCRK AK.SSN
AK.SSP AK.VRDI AK.WRH AT.MENT AT.PMR CN.DAWY CN.HYT IM.IL31
IU.COLA NY.MAYO TA.I23K TA.I26K TA.I29M TA.J26L TA.J29M
TA.L26K TA.L27K TA.M27K TA.M30M TA.M31M TA.N25K TA.N31M
TA.O22K TA.POKR TA.TCOL US.EGAK
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 = 8.22e+23 dyne-cm
Mw = 5.21
Z = 14 km
Plane Strike Dip Rake
NP1 50 90 -5
NP2 140 85 -180
Principal Axes:
Axis Value Plunge Azimuth
T 8.22e+23 4 95
N 0.00e+00 85 230
P -8.22e+23 4 5
Moment Tensor: (dyne-cm)
Component Value
Mxx -8.07e+23
Mxy -1.42e+23
Mxz -5.49e+22
Myy 8.07e+23
Myz 4.61e+22
Mzz 6.27e+15
------- P ----
----------- --------
#---------------------------
###---------------------------
######-------------------------###
########----------------------######
###########------------------#########
#############---------------############
###############-----------##############
#################-------##################
###################---##################
######################################## T
##################----##################
##############--------##################
############------------################
#########----------------#############
######-------------------###########
###-----------------------########
--------------------------####
---------------------------#
----------------------
--------------
Global CMT Convention Moment Tensor:
R T P
6.27e+15 -5.49e+22 -4.61e+22
-5.49e+22 -8.07e+23 1.42e+23
-4.61e+22 1.42e+23 8.07e+23
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170213071712/index.html
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STK = 50
DIP = 90
RAKE = -5
MW = 5.21
HS = 14.0
The NDK file is 20170213071712.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 2017/02/13 07:17:12:0 62.51 -142.75 8.9 5.3 Alaska
Stations used:
AK.BARN AK.BCP AK.BWN AK.CCB AK.CUT AK.DHY AK.DIV AK.DOT
AK.EYAK AK.FIRE AK.GLB AK.HDA AK.KLU AK.MCAR AK.MDM AK.NEA2
AK.PAX AK.PIN AK.PPD AK.PWL AK.RC01 AK.RIDG AK.SCRK AK.SSN
AK.SSP AK.VRDI AK.WRH AT.MENT AT.PMR CN.DAWY CN.HYT IM.IL31
IU.COLA NY.MAYO TA.I23K TA.I26K TA.I29M TA.J26L TA.J29M
TA.L26K TA.L27K TA.M27K TA.M30M TA.M31M TA.N25K TA.N31M
TA.O22K TA.POKR TA.TCOL US.EGAK
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 = 8.22e+23 dyne-cm
Mw = 5.21
Z = 14 km
Plane Strike Dip Rake
NP1 50 90 -5
NP2 140 85 -180
Principal Axes:
Axis Value Plunge Azimuth
T 8.22e+23 4 95
N 0.00e+00 85 230
P -8.22e+23 4 5
Moment Tensor: (dyne-cm)
Component Value
Mxx -8.07e+23
Mxy -1.42e+23
Mxz -5.49e+22
Myy 8.07e+23
Myz 4.61e+22
Mzz 6.27e+15
------- P ----
----------- --------
#---------------------------
###---------------------------
######-------------------------###
########----------------------######
###########------------------#########
#############---------------############
###############-----------##############
#################-------##################
###################---##################
######################################## T
##################----##################
##############--------##################
############------------################
#########----------------#############
######-------------------###########
###-----------------------########
--------------------------####
---------------------------#
----------------------
--------------
Global CMT Convention Moment Tensor:
R T P
6.27e+15 -5.49e+22 -4.61e+22
-5.49e+22 -8.07e+23 1.42e+23
-4.61e+22 1.42e+23 8.07e+23
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20170213071712/index.html
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Regional Moment Tensor (Mwr) Moment 9.622e+16 N-m Magnitude 5.3 Mwr Depth 14.0 km Percent DC 87 % Half Duration – Catalog US Data Source US3 Contributor US3 Nodal Planes Plane Strike Dip Rake NP1 51 87 -4 NP2 141 86 -177 Principal Axes Axis Value Plunge Azimuth T 9.936e+16 N-m 0 96 N -0.663e+16 N-m 85 189 P -9.273e+16 N-m 5 6 |
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 1.0 50 80 -10 4.75 0.3073
WVFGRD96 2.0 45 65 -25 4.92 0.4297
WVFGRD96 3.0 50 75 -10 4.94 0.4843
WVFGRD96 4.0 50 90 15 4.97 0.5350
WVFGRD96 5.0 50 90 15 5.01 0.5799
WVFGRD96 6.0 50 85 15 5.04 0.6210
WVFGRD96 7.0 50 80 10 5.07 0.6611
WVFGRD96 8.0 50 80 -10 5.11 0.6971
WVFGRD96 9.0 50 80 15 5.13 0.7231
WVFGRD96 10.0 50 85 -10 5.15 0.7430
WVFGRD96 11.0 230 90 10 5.17 0.7564
WVFGRD96 12.0 50 85 -10 5.19 0.7658
WVFGRD96 13.0 50 90 -10 5.20 0.7698
WVFGRD96 14.0 50 90 -5 5.21 0.7707
WVFGRD96 15.0 50 90 -5 5.22 0.7691
WVFGRD96 16.0 50 90 -5 5.23 0.7650
WVFGRD96 17.0 50 90 -5 5.24 0.7592
WVFGRD96 18.0 50 90 -5 5.25 0.7523
WVFGRD96 19.0 50 90 -5 5.26 0.7443
WVFGRD96 20.0 50 90 -5 5.26 0.7350
WVFGRD96 21.0 230 90 5 5.27 0.7251
WVFGRD96 22.0 50 90 -5 5.28 0.7146
WVFGRD96 23.0 50 90 -5 5.28 0.7031
WVFGRD96 24.0 230 90 5 5.29 0.6914
WVFGRD96 25.0 50 90 0 5.29 0.6798
WVFGRD96 26.0 50 90 0 5.30 0.6683
WVFGRD96 27.0 50 90 0 5.30 0.6571
WVFGRD96 28.0 230 85 -5 5.31 0.6460
WVFGRD96 29.0 50 85 0 5.32 0.6354
The best solution is
WVFGRD96 14.0 50 90 -5 5.21 0.7707
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