Location

Location ANSS

The ANSS event ID is us70003mzp and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us70003mzp/executive.

2019/05/18 09:55:36 36.704 -97.663 5.0 3.3 Oklahoma

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2019/05/18 09:55:36:0 36.70 -97.66 5.0 3.3 Oklahoma Stations used: GS.KAN08 GS.KAN13 N4.R32B N4.T35B N4.U38B O2.CHAN O2.DRUM O2.MRSH O2.PERK O2.PERY O2.SMNL OK.CROK OK.FNO US.CBKS US.KSU1 US.MIAR Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.05 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 9.44e+20 dyne-cm Mw = 3.25 Z = 3 km Plane Strike Dip Rake NP1 345 90 -5 NP2 75 85 -180 Principal Axes: Axis Value Plunge Azimuth T 9.44e+20 4 30 N 0.00e+00 85 165 P -9.44e+20 4 300 Moment Tensor: (dyne-cm) Component Value Mxx 4.70e+20 Mxy 8.14e+20 Mxz 2.13e+19 Myy -4.70e+20 Myz 7.95e+19 Mzz 7.19e+12 --############ ------############# T ----------############ ### -----------################### -------------#################### P -------------##################### --------------##################### ------------------###################### -------------------###################-- --------------------###############------- ---------------------########------------- ---------------------#-------------------- ---------------#######-------------------- -----################------------------- ######################------------------ #####################----------------- #####################--------------- ####################-------------- ###################----------- ##################---------- ################------ ############-- Global CMT Convention Moment Tensor: R T P 7.19e+12 2.13e+19 -7.95e+19 2.13e+19 4.70e+20 -8.14e+20 -7.95e+19 -8.14e+20 -4.70e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20190518095536/index.html

Preferred Solution

      STK = 345
      DIP = 90
     RAKE = -5
       MW = 3.25
       HS = 3.0

The NDK file is 20190518095536.ndk The waveform inversion is preferred.

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:

cut o DIST/3.3 -30 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.05 n 3 
lp c 0.10 n 3 

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   340    80   -35   3.12 0.4234
WVFGRD96    2.0   340    75   -20   3.22 0.4678
WVFGRD96    3.0   345    90    -5   3.25 0.4737
WVFGRD96    4.0   345    90   -15   3.29 0.4619
WVFGRD96    5.0   165    80    20   3.33 0.4574
WVFGRD96    6.0   345    90   -20   3.36 0.4507
WVFGRD96    7.0   165    85    25   3.40 0.4480
WVFGRD96    8.0   165    80    35   3.45 0.4410
WVFGRD96    9.0   165    85    30   3.47 0.4325
WVFGRD96   10.0   340    90   -30   3.48 0.4232
WVFGRD96   11.0   165    85    30   3.51 0.4140
WVFGRD96   12.0   340    85   -30   3.52 0.4033
WVFGRD96   13.0   165    85    25   3.54 0.3919
WVFGRD96   14.0   340    85   -30   3.55 0.3790
WVFGRD96   15.0   340    85   -30   3.57 0.3662
WVFGRD96   16.0   160    85    20   3.56 0.3555
WVFGRD96   17.0   345    90    25   3.58 0.3436
WVFGRD96   18.0   165    90   -25   3.59 0.3365
WVFGRD96   19.0   160    90   -25   3.59 0.3309
WVFGRD96   20.0   160    80   -15   3.59 0.3270
WVFGRD96   21.0   160    80   -15   3.59 0.3244
WVFGRD96   22.0   160    80   -20   3.61 0.3227
WVFGRD96   23.0   160    80   -20   3.61 0.3204
WVFGRD96   24.0   160    85   -20   3.62 0.3204
WVFGRD96   25.0   250    85    10   3.61 0.3195
WVFGRD96   26.0   250    85    10   3.62 0.3215
WVFGRD96   27.0    70    90   -10   3.62 0.3243
WVFGRD96   28.0   250    90    10   3.63 0.3253
WVFGRD96   29.0   250    90    10   3.63 0.3311

The best solution is

WVFGRD96    3.0   345    90    -5   3.25 0.4737

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

cut o DIST/3.3 -30 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.05 n 3 
lp c 0.10 n 3 

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