Location

Location ANSS

The ANSS event ID is usb000szm7 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usb000szm7/executive.

2014/11/24 19:05:58 36.873 -98.335 5.3 3.7 Oklahoma

Focal Mechanism

USGS/SLU Moment Tensor Solution ENS 2014/11/24 19:05:58:0 36.87 -98.33 5.3 3.7 Oklahoma Stations used: GS.KAN01 GS.KAN10 GS.KAN12 GS.KAN14 GS.KS20 GS.OK025 GS.OK026 GS.OK027 GS.OK028 GS.OK030 GS.OK031 N4.R32B N4.T35B N4.Z35B OK.CROK OK.FNO OK.U32A OK.X37A TA.ABTX TA.TUL1 TA.WHTX US.CBKS US.KSU1 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 0.07 n 3 Best Fitting Double Couple Mo = 3.89e+21 dyne-cm Mw = 3.66 Z = 3 km Plane Strike Dip Rake NP1 239 54 -110 NP2 90 40 -65 Principal Axes: Axis Value Plunge Azimuth T 3.89e+21 7 342 N 0.00e+00 16 250 P -3.89e+21 72 97 Moment Tensor: (dyne-cm) Component Value Mxx 3.47e+21 Mxy -1.06e+21 Mxz 6.12e+20 Myy -9.24e+13 Myz -1.26e+21 Mzz -3.47e+21 ########### #### T ############### ####### ################## ############################## ########################------#### ##################------------------ ###############----------------------- #############--------------------------- ###########----------------------------- ##########-------------------------------- ########---------------- --------------- -######----------------- P --------------# --####------------------ -------------## --##----------------------------------## ---#--------------------------------#### --###----------------------------##### ########--------------------######## #############--------############# ############################## ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -3.47e+21 6.12e+20 1.26e+21 6.12e+20 3.47e+21 1.06e+21 1.26e+21 1.06e+21 -9.24e+13 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20141124190558/index.html

Preferred Solution

      STK = 90
      DIP = 40
     RAKE = -65
       MW = 3.66
       HS = 3.0

The NDK file is 20141124190558.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.

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 0.03 n 3 
lp c 0.07 n 3 

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   100    35   -45   3.50 0.4267
WVFGRD96    2.0    90    25   -60   3.66 0.5188
WVFGRD96    3.0    90    40   -65   3.66 0.5443
WVFGRD96    4.0    95    40   -60   3.66 0.4617
WVFGRD96    5.0   305    40   -15   3.63 0.3947
WVFGRD96    6.0   310    45   -10   3.62 0.3997
WVFGRD96    7.0   310    50    10   3.64 0.4042
WVFGRD96    8.0   310    40    -5   3.68 0.4067
WVFGRD96    9.0   310    40    -5   3.69 0.4111
WVFGRD96   10.0   310    40    -5   3.69 0.4159
WVFGRD96   11.0   315    40    10   3.70 0.4215
WVFGRD96   12.0   320    40    15   3.71 0.4255
WVFGRD96   13.0   320    40    15   3.71 0.4280
WVFGRD96   14.0   320    40    15   3.72 0.4285
WVFGRD96   15.0   320    40    15   3.73 0.4277
WVFGRD96   16.0   320    40    15   3.73 0.4257
WVFGRD96   17.0   320    40    15   3.74 0.4226
WVFGRD96   18.0   320    40    15   3.75 0.4187
WVFGRD96   19.0   320    40    10   3.75 0.4146
WVFGRD96   20.0   320    40    10   3.76 0.4099
WVFGRD96   21.0   160    45    30   3.78 0.4110
WVFGRD96   22.0   160    45    30   3.79 0.4107
WVFGRD96   23.0   165    45    35   3.80 0.4104
WVFGRD96   24.0   165    45    30   3.81 0.4094
WVFGRD96   25.0   170    45    35   3.81 0.4073
WVFGRD96   26.0   170    45    35   3.82 0.4047
WVFGRD96   27.0   170    45    35   3.83 0.4009
WVFGRD96   28.0   170    45    35   3.84 0.3967
WVFGRD96   29.0   170    45    35   3.84 0.3910

The best solution is

WVFGRD96    3.0    90    40   -65   3.66 0.5443

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 0.03 n 3 
lp c 0.07 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