The ANSS event ID is usb000rt1u and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usb000rt1u/executive.
2014/07/15 07:19:17 35.524 -97.154 6.5 3.5 Oklahoma
USGS/SLU Moment Tensor Solution
ENS 2014/07/15 07:19:17:0 35.52 -97.15 6.5 3.5 Oklahoma
Stations used:
AG.CCAR AG.FCAR AG.LCAR AG.WHAR AG.WLAR GS.KAN10 GS.KAN12
GS.KAN13 GS.OK026 GS.OK027 GS.OK029 IU.CCM N4.237B N4.N33B
N4.P38B N4.R32B N4.S39B N4.T42B N4.U38B N4.Z35B N4.Z38B
NM.MGMO OK.BCOK OK.FNO OK.U32A OK.X37A TA.435B TA.ABTX
TA.MSTX TA.TUL1 TA.U40A TA.W41B TA.WHTX TA.X40A US.CBKS
US.KSU1 US.MIAR US.WMOK
Filtering commands used:
cut o DIST/3.3 -30 o DIST/3.3 +60
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.07 n 3
Best Fitting Double Couple
Mo = 4.47e+21 dyne-cm
Mw = 3.70
Z = 4 km
Plane Strike Dip Rake
NP1 19 85 170
NP2 110 80 5
Principal Axes:
Axis Value Plunge Azimuth
T 4.47e+21 11 334
N 0.00e+00 79 173
P -4.47e+21 4 65
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.70e+21
Mxy -3.40e+21
Mxz 6.08e+20
Myy -2.83e+21
Myz -6.01e+20
Mzz 1.33e+20
##############
# T #############-----
#### #############--------
#####################---------
######################------------
#######################------------
#######################------------- P
-######################--------------
----###################-----------------
--------###############-------------------
------------###########-------------------
----------------######--------------------
------------------------------------------
--------------------######--------------
-------------------###############------
-----------------#####################
----------------####################
--------------####################
-----------###################
---------###################
-----#################
##############
Global CMT Convention Moment Tensor:
R T P
1.33e+20 6.08e+20 6.01e+20
6.08e+20 2.70e+21 3.40e+21
6.01e+20 3.40e+21 -2.83e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20140715071917/index.html
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STK = 110
DIP = 80
RAKE = 5
MW = 3.70
HS = 4.0
The NDK file is 20140715071917.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 2014/07/15 07:19:17:0 35.52 -97.15 6.5 3.5 Oklahoma
Stations used:
AG.CCAR AG.FCAR AG.LCAR AG.WHAR AG.WLAR GS.KAN10 GS.KAN12
GS.KAN13 GS.OK026 GS.OK027 GS.OK029 IU.CCM N4.237B N4.N33B
N4.P38B N4.R32B N4.S39B N4.T42B N4.U38B N4.Z35B N4.Z38B
NM.MGMO OK.BCOK OK.FNO OK.U32A OK.X37A TA.435B TA.ABTX
TA.MSTX TA.TUL1 TA.U40A TA.W41B TA.WHTX TA.X40A US.CBKS
US.KSU1 US.MIAR US.WMOK
Filtering commands used:
cut o DIST/3.3 -30 o DIST/3.3 +60
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.07 n 3
Best Fitting Double Couple
Mo = 4.47e+21 dyne-cm
Mw = 3.70
Z = 4 km
Plane Strike Dip Rake
NP1 19 85 170
NP2 110 80 5
Principal Axes:
Axis Value Plunge Azimuth
T 4.47e+21 11 334
N 0.00e+00 79 173
P -4.47e+21 4 65
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.70e+21
Mxy -3.40e+21
Mxz 6.08e+20
Myy -2.83e+21
Myz -6.01e+20
Mzz 1.33e+20
##############
# T #############-----
#### #############--------
#####################---------
######################------------
#######################------------
#######################------------- P
-######################--------------
----###################-----------------
--------###############-------------------
------------###########-------------------
----------------######--------------------
------------------------------------------
--------------------######--------------
-------------------###############------
-----------------#####################
----------------####################
--------------####################
-----------###################
---------###################
-----#################
##############
Global CMT Convention Moment Tensor:
R T P
1.33e+20 6.08e+20 6.01e+20
6.08e+20 2.70e+21 3.40e+21
6.01e+20 3.40e+21 -2.83e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20140715071917/index.html
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Moment
2.47e+14 N-m
Magnitude
3.5
Percent DC
56%
Depth
2.0 km
Updated
2014-07-15 13:03:43 UTC
Author
us
Catalog
us
Contributor
us
Code
us_b000rt1u_mwr
Principal Axes
Axis Value Plunge Azimuth
T 2.713 12 161
N -0.594 72 295
P -2.119 12 68
Nodal Planes
Plane Strike Dip Rake
NP1 115 90 -18
NP2 205 72 -180
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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 +60 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 1.0 290 85 5 3.50 0.3711
WVFGRD96 2.0 110 80 -5 3.61 0.4578
WVFGRD96 3.0 110 80 5 3.67 0.5035
WVFGRD96 4.0 110 80 5 3.70 0.5167
WVFGRD96 5.0 110 80 10 3.74 0.5127
WVFGRD96 6.0 110 75 5 3.76 0.5019
WVFGRD96 7.0 110 80 10 3.78 0.4903
WVFGRD96 8.0 110 75 10 3.81 0.4805
WVFGRD96 9.0 110 75 10 3.82 0.4603
WVFGRD96 10.0 110 75 10 3.83 0.4413
WVFGRD96 11.0 110 75 10 3.85 0.4266
WVFGRD96 12.0 110 75 10 3.85 0.4112
WVFGRD96 13.0 110 75 5 3.86 0.3972
WVFGRD96 14.0 110 80 10 3.87 0.3831
WVFGRD96 15.0 110 80 10 3.87 0.3698
WVFGRD96 16.0 110 80 10 3.88 0.3565
WVFGRD96 17.0 110 80 5 3.88 0.3452
WVFGRD96 18.0 110 80 5 3.88 0.3355
WVFGRD96 19.0 110 80 5 3.89 0.3270
WVFGRD96 20.0 110 80 5 3.90 0.3193
WVFGRD96 21.0 110 80 5 3.90 0.3150
WVFGRD96 22.0 110 80 5 3.91 0.3110
WVFGRD96 23.0 110 80 5 3.92 0.3079
WVFGRD96 24.0 110 80 10 3.93 0.3071
WVFGRD96 25.0 110 80 10 3.94 0.3072
WVFGRD96 26.0 110 80 10 3.95 0.3071
WVFGRD96 27.0 115 85 10 3.95 0.3076
WVFGRD96 28.0 115 85 10 3.96 0.3093
WVFGRD96 29.0 110 85 10 3.97 0.3106
The best solution is
WVFGRD96 4.0 110 80 5 3.70 0.5167
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 +60 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