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.
The ANSS event ID is us20002yvl and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us20002yvl/executive.
2015/07/21 11:16:14 36.837 -98.245 5.0 3.1 Oklahoma
USGS/SLU Moment Tensor Solution
ENS 2015/07/21 11:16:14:0 36.84 -98.25 5.0 3.1 Oklahoma
Stations used:
GS.KAN08 GS.KAN10 GS.KAN11 GS.KAN12 GS.KAN13 GS.KAN17
GS.KS20 GS.KS21 GS.OK029 N4.T35B OK.CROK OK.U32A
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +40
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.08 n 3
Best Fitting Double Couple
Mo = 6.03e+20 dyne-cm
Mw = 3.12
Z = 5 km
Plane Strike Dip Rake
NP1 265 55 -70
NP2 53 40 -116
Principal Axes:
Axis Value Plunge Azimuth
T 6.03e+20 8 341
N 0.00e+00 16 73
P -6.03e+20 72 226
Moment Tensor: (dyne-cm)
Component Value
Mxx 4.99e+20
Mxy -2.12e+20
Mxz 2.03e+20
Myy 3.34e+19
Myz 1.01e+20
Mzz -5.32e+20
############
### T ################
###### ###################
##############################
##################################
###################################-
###############-------------########--
##########------------------------###---
######-------------------------------#--
####---------------------------------####-
##-----------------------------------#####
#--------------- -----------------######
---------------- P ----------------#######
--------------- ---------------#######
-------------------------------#########
----------------------------##########
-------------------------###########
---------------------#############
#--------------###############
############################
######################
##############
Global CMT Convention Moment Tensor:
R T P
-5.32e+20 2.03e+20 -1.01e+20
2.03e+20 4.99e+20 2.12e+20
-1.01e+20 2.12e+20 3.34e+19
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20150721111614/index.html
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STK = 265
DIP = 55
RAKE = -70
MW = 3.12
HS = 5.0
The NDK file is 20150721111614.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 -20 o DIST/3.3 +40 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 1.0 180 80 15 2.81 0.2993
WVFGRD96 2.0 110 25 -20 3.14 0.3289
WVFGRD96 3.0 95 45 -40 3.11 0.4313
WVFGRD96 4.0 265 55 -65 3.13 0.5180
WVFGRD96 5.0 265 55 -70 3.12 0.5233
WVFGRD96 6.0 265 55 -75 3.11 0.4914
WVFGRD96 7.0 265 55 -75 3.10 0.4524
WVFGRD96 8.0 265 55 -75 3.17 0.4454
WVFGRD96 9.0 335 60 -55 3.14 0.3998
WVFGRD96 10.0 335 60 -55 3.15 0.3962
WVFGRD96 11.0 335 60 -50 3.15 0.3847
WVFGRD96 12.0 340 65 -45 3.15 0.3699
WVFGRD96 13.0 340 65 -45 3.16 0.3542
WVFGRD96 14.0 335 60 -45 3.16 0.3385
WVFGRD96 15.0 335 60 -45 3.16 0.3242
WVFGRD96 16.0 45 75 -55 3.18 0.3100
WVFGRD96 17.0 45 75 -55 3.19 0.3093
WVFGRD96 18.0 255 80 60 3.16 0.3078
WVFGRD96 19.0 255 80 60 3.17 0.3103
WVFGRD96 20.0 255 80 60 3.17 0.3106
WVFGRD96 21.0 255 80 55 3.20 0.3100
WVFGRD96 22.0 255 80 55 3.21 0.3081
WVFGRD96 23.0 255 75 55 3.22 0.3062
WVFGRD96 24.0 250 85 60 3.22 0.3066
WVFGRD96 25.0 255 85 60 3.22 0.3071
WVFGRD96 26.0 260 85 65 3.22 0.3079
WVFGRD96 27.0 260 85 60 3.23 0.3091
WVFGRD96 28.0 260 85 60 3.24 0.3094
WVFGRD96 29.0 260 85 60 3.25 0.3075
The best solution is
WVFGRD96 5.0 265 55 -70 3.12 0.5233
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 -20 o DIST/3.3 +40 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 CUS.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 CUS Model with Q from simple gamma values 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 1.0000 5.0000 2.8900 2.5000 0.172E-02 0.387E-02 0.00 0.00 1.00 1.00 9.0000 6.1000 3.5200 2.7300 0.160E-02 0.363E-02 0.00 0.00 1.00 1.00 10.0000 6.4000 3.7000 2.8200 0.149E-02 0.336E-02 0.00 0.00 1.00 1.00 20.0000 6.7000 3.8700 2.9020 0.000E-04 0.000E-04 0.00 0.00 1.00 1.00 0.0000 8.1500 4.7000 3.3640 0.194E-02 0.431E-02 0.00 0.00 1.00 1.00