The ANSS event ID is us20003l6t and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us20003l6t/executive.
2015/09/18 12:35:17 35.993 -96.800 0.2 4.1 Oklahoma
USGS/SLU Moment Tensor Solution
ENS 2015/09/18 12:35:17:0 35.99 -96.80 0.2 4.1 Oklahoma
Stations used:
AG.HHAR GS.KAN05 GS.KAN10 GS.KAN12 GS.KAN13 GS.KAN14
GS.KAN16 GS.KAN17 GS.KS20 GS.KS21 GS.OK025 GS.OK029
GS.OK032 N4.R32B N4.T35B N4.U38B N4.Z35B OK.BCOK OK.BLOK
OK.CCOK OK.CHOK OK.CROK OK.FNO OK.LOOK OK.OKCFA OK.QUOK
OK.U32A OK.X34A OK.X37A TA.W39A US.KSU1 US.MIAR US.WMOK
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 0.08 n 3
Best Fitting Double Couple
Mo = 1.22e+22 dyne-cm
Mw = 3.99
Z = 4 km
Plane Strike Dip Rake
NP1 240 90 -175
NP2 150 85 0
Principal Axes:
Axis Value Plunge Azimuth
T 1.22e+22 4 15
N 0.00e+00 85 240
P -1.22e+22 4 105
Moment Tensor: (dyne-cm)
Component Value
Mxx 1.05e+22
Mxy 6.06e+21
Mxz 9.18e+20
Myy -1.05e+22
Myz -5.30e+20
Mzz 0.00e+00
########### T
-############## ####
-----#######################
------########################
---------#########################
-----------#########################
-------------####################-----
---------------################---------
----------------############------------
------------------########----------------
-------------------####-------------------
-------------------#----------------------
----------------#####------------------
------------#########----------------- P
---------#############----------------
-----##################---------------
#######################-------------
#######################-----------
######################--------
#######################-----
#####################-
##############
Global CMT Convention Moment Tensor:
R T P
0.00e+00 9.18e+20 5.30e+20
9.18e+20 1.05e+22 -6.06e+21
5.30e+20 -6.06e+21 -1.05e+22
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150918123517/index.html
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STK = 150
DIP = 85
RAKE = 0
MW = 3.99
HS = 4.0
The NDK file is 20150918123517.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 2015/09/18 12:35:17:0 35.99 -96.80 0.2 4.1 Oklahoma
Stations used:
AG.HHAR GS.KAN05 GS.KAN10 GS.KAN12 GS.KAN13 GS.KAN14
GS.KAN16 GS.KAN17 GS.KS20 GS.KS21 GS.OK025 GS.OK029
GS.OK032 N4.R32B N4.T35B N4.U38B N4.Z35B OK.BCOK OK.BLOK
OK.CCOK OK.CHOK OK.CROK OK.FNO OK.LOOK OK.OKCFA OK.QUOK
OK.U32A OK.X34A OK.X37A TA.W39A US.KSU1 US.MIAR US.WMOK
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 0.08 n 3
Best Fitting Double Couple
Mo = 1.22e+22 dyne-cm
Mw = 3.99
Z = 4 km
Plane Strike Dip Rake
NP1 240 90 -175
NP2 150 85 0
Principal Axes:
Axis Value Plunge Azimuth
T 1.22e+22 4 15
N 0.00e+00 85 240
P -1.22e+22 4 105
Moment Tensor: (dyne-cm)
Component Value
Mxx 1.05e+22
Mxy 6.06e+21
Mxz 9.18e+20
Myy -1.05e+22
Myz -5.30e+20
Mzz 0.00e+00
########### T
-############## ####
-----#######################
------########################
---------#########################
-----------#########################
-------------####################-----
---------------################---------
----------------############------------
------------------########----------------
-------------------####-------------------
-------------------#----------------------
----------------#####------------------
------------#########----------------- P
---------#############----------------
-----##################---------------
#######################-------------
#######################-----------
######################--------
#######################-----
#####################-
##############
Global CMT Convention Moment Tensor:
R T P
0.00e+00 9.18e+20 5.30e+20
9.18e+20 1.05e+22 -6.06e+21
5.30e+20 -6.06e+21 -1.05e+22
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150918123517/index.html
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egional Moment Tensor (Mwr) Moment 1.795e+15 N-m Magnitude 4.10 Depth 5.0 km Percent DC 86% Half Duration – Catalog US (us20003l6t) Data Source US1 Contributor US1 Nodal Planes Plane Strike Dip Rake NP1 149 70 -3 NP2 240 87 -160 Principal Axes Axis Value Plunge Azimuth T 1.858 12 13 N -0.133 70 247 P -1.725 16 106 |
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 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 330 75 0 3.79 0.3764
WVFGRD96 2.0 145 75 -15 3.91 0.4700
WVFGRD96 3.0 330 90 0 3.96 0.4973
WVFGRD96 4.0 150 85 0 3.99 0.5005
WVFGRD96 5.0 150 85 5 4.02 0.4918
WVFGRD96 6.0 150 80 5 4.05 0.4811
WVFGRD96 7.0 150 80 10 4.07 0.4717
WVFGRD96 8.0 330 70 10 4.10 0.4649
WVFGRD96 9.0 325 75 10 4.10 0.4547
WVFGRD96 10.0 325 75 10 4.12 0.4448
WVFGRD96 11.0 325 75 10 4.13 0.4344
WVFGRD96 12.0 325 75 10 4.14 0.4238
WVFGRD96 13.0 325 75 10 4.15 0.4134
WVFGRD96 14.0 325 80 10 4.16 0.4033
WVFGRD96 15.0 325 80 10 4.17 0.3932
WVFGRD96 16.0 325 80 10 4.18 0.3836
WVFGRD96 17.0 330 80 10 4.19 0.3751
WVFGRD96 18.0 330 80 10 4.20 0.3668
WVFGRD96 19.0 330 80 10 4.21 0.3590
WVFGRD96 20.0 330 80 10 4.22 0.3517
WVFGRD96 21.0 330 80 10 4.22 0.3447
WVFGRD96 22.0 330 80 10 4.23 0.3383
WVFGRD96 23.0 330 75 10 4.24 0.3320
WVFGRD96 24.0 330 75 10 4.24 0.3266
WVFGRD96 25.0 330 75 10 4.25 0.3214
WVFGRD96 26.0 330 75 10 4.26 0.3168
WVFGRD96 27.0 330 75 10 4.26 0.3124
WVFGRD96 28.0 330 75 10 4.27 0.3086
WVFGRD96 29.0 330 75 10 4.27 0.3047
The best solution is
WVFGRD96 4.0 150 85 0 3.99 0.5005
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 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 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