Location

SLU Location

Location ANSS

The ANSS event ID is usp000hkyn and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000hkyn/executive.

2010/09/19 22:01:47 35.611 -97.246 5.0 3.5 Oklahoma

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2010/09/19 22:01:47:0 35.61 -97.25 5.0 3.5 Oklahoma Stations used: AG.HHAR TA.S35A TA.T30A TA.T34A TA.TUL1 TA.U33A TA.U34A TA.V33A TA.V34A TA.V35A TA.W33A TA.W35A TA.W36A TA.W37A TA.W38A TA.X34A TA.X35A TA.X36A TA.X37A TA.X38A TA.Y34A TA.Y35A TA.Y37A TA.Y39A TA.Z35A Filtering commands used: hp c 0.02 n 4 lp c 0.08 n 4 Best Fitting Double Couple Mo = 2.02e+21 dyne-cm Mw = 3.47 Z = 3 km Plane Strike Dip Rake NP1 15 90 -160 NP2 285 70 0 Principal Axes: Axis Value Plunge Azimuth T 2.02e+21 14 148 N 0.00e+00 70 15 P -2.02e+21 14 242 Moment Tensor: (dyne-cm) Component Value Mxx 9.48e+20 Mxy -1.64e+21 Mxz -1.79e+20 Myy -9.48e+20 Myz 6.67e+20 Mzz 0.00e+00 ############-- ################------ ##################---------- ###################----------- ####################-------------- #####################--------------- #####################----------------- ####---------#########------------------ ---------------------#------------------ ----------------------#######------------- ---------------------############--------- ---------------------###############------ --------------------##################---- -------------------####################- --- ------------###################### -- P ------------##################### - -----------##################### --------------#################### -----------############ #### ----------############ T ### ------############# --############ Global CMT Convention Moment Tensor: R T P 0.00e+00 -1.79e+20 -6.67e+20 -1.79e+20 9.48e+20 1.64e+21 -6.67e+20 1.64e+21 -9.48e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20100919220147/index.html

Preferred Solution

      STK = 285
      DIP = 70
     RAKE = 0
       MW = 3.47
       HS = 3.0

The NDK file is 20100919220147.ndk The waveform inversion is preferred.

Moment Tensor Comparison

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.

SLU

SLUFM

USGS/SLU Moment Tensor Solution ENS 2010/09/19 22:01:47:0 35.61 -97.25 5.0 3.5 Oklahoma Stations used: AG.HHAR TA.S35A TA.T30A TA.T34A TA.TUL1 TA.U33A TA.U34A TA.V33A TA.V34A TA.V35A TA.W33A TA.W35A TA.W36A TA.W37A TA.W38A TA.X34A TA.X35A TA.X36A TA.X37A TA.X38A TA.Y34A TA.Y35A TA.Y37A TA.Y39A TA.Z35A Filtering commands used: hp c 0.02 n 4 lp c 0.08 n 4 Best Fitting Double Couple Mo = 2.02e+21 dyne-cm Mw = 3.47 Z = 3 km Plane Strike Dip Rake NP1 15 90 -160 NP2 285 70 0 Principal Axes: Axis Value Plunge Azimuth T 2.02e+21 14 148 N 0.00e+00 70 15 P -2.02e+21 14 242 Moment Tensor: (dyne-cm) Component Value Mxx 9.48e+20 Mxy -1.64e+21 Mxz -1.79e+20 Myy -9.48e+20 Myz 6.67e+20 Mzz 0.00e+00 ############-- ################------ ##################---------- ###################----------- ####################-------------- #####################--------------- #####################----------------- ####---------#########------------------ ---------------------#------------------ ----------------------#######------------- ---------------------############--------- ---------------------###############------ --------------------##################---- -------------------####################- --- ------------###################### -- P ------------##################### - -----------##################### --------------#################### -----------############ #### ----------############ T ### ------############# --############ Global CMT Convention Moment Tensor: R T P 0.00e+00 -1.79e+20 -6.67e+20 -1.79e+20 9.48e+20 1.64e+21 -6.67e+20 1.64e+21 -9.48e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20100919220147/index.html

First motions plot using the waveform inversion nodal planes and the elcoate takeoff angles and azimuths. Symbols: o strong compression, + weak compression, Delta strong dilatation, - weak dilatation, X undetermined polarity.

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

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:

hp c 0.02 n 4
lp c 0.08 n 4

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    0.5   285    50     5   3.42 0.3902
WVFGRD96    1.0   285    65     5   3.39 0.4050
WVFGRD96    2.0   285    55     0   3.47 0.4386
WVFGRD96    3.0   285    70     0   3.47 0.4502
WVFGRD96    4.0   285    70     0   3.49 0.4498
WVFGRD96    5.0   285    75    10   3.50 0.4441
WVFGRD96    6.0   285    80    15   3.52 0.4377
WVFGRD96    7.0   285    80    15   3.53 0.4315
WVFGRD96    8.0   285    80    20   3.56 0.4247
WVFGRD96    9.0   105    60     5   3.59 0.4185
WVFGRD96   10.0   105    65    10   3.59 0.4160
WVFGRD96   11.0   105    65    10   3.61 0.4136
WVFGRD96   12.0   105    65    10   3.62 0.4110
WVFGRD96   13.0   105    65    10   3.63 0.4075
WVFGRD96   14.0   105    65    10   3.64 0.4042
WVFGRD96   15.0   105    65     5   3.65 0.4001
WVFGRD96   16.0   105    65    10   3.66 0.3955
WVFGRD96   17.0   105    65    10   3.67 0.3903
WVFGRD96   18.0   105    65    10   3.68 0.3847
WVFGRD96   19.0   105    65    10   3.69 0.3787
WVFGRD96   20.0   105    70    10   3.69 0.3724
WVFGRD96   21.0   110    60    25   3.71 0.3669
WVFGRD96   22.0   110    60    25   3.72 0.3616
WVFGRD96   23.0   110    60    25   3.73 0.3561
WVFGRD96   24.0   110    60    25   3.74 0.3503
WVFGRD96   25.0   110    60    25   3.75 0.3441
WVFGRD96   26.0   110    60    25   3.76 0.3376
WVFGRD96   27.0   110    60    25   3.77 0.3306
WVFGRD96   28.0   110    60    30   3.78 0.3234
WVFGRD96   29.0   110    65    30   3.78 0.3163

The best solution is

WVFGRD96    3.0   285    70     0   3.47 0.4502

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

hp c 0.02 n 4
lp c 0.08 n 4

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)

 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