Location

Location ANSS

The ANSS event ID is us7000krer and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us7000krer/executive.

2023/08/28 02:43:26 41.731 -80.972 5.0 3.6 Ohio

Focal Mechanism

 USGS/SLU Moment Tensor Solution
 ENS  2023/08/28 02:43:26:0  41.73  -80.97   5.0 3.6 Ohio
 
 Stations used:
   CN.CHRO CN.EFO CN.GAC CN.KGNO CN.SADO IU.SSPA IU.WCI LD.FOR 
   LD.GCMD LD.GEDE LD.KSCT LD.KSPA LD.MMNY LD.SDMD LD.WVNY 
   LM.NHBP MU.EARS MU.MUG1 N4.E46A N4.I45A N4.I49A N4.J47A 
   N4.J55A N4.J57A N4.J59A N4.K50A N4.K57A N4.L46A N4.L56A 
   N4.L59A N4.M44A N4.M50A N4.M57A N4.N47A N4.N49A N4.N51A 
   N4.N53A N4.N58A N4.N62A N4.O48B N4.O49A N4.O52A N4.O54A 
   N4.P46A N4.P48A N4.P53A N4.Q51A N4.Q52A N4.Q54A N4.R49A 
   N4.R50A N4.R55A N4.S51A N4.S54A N4.SFIN N4.T50A N4.T57A 
   N4.T59A N4.V55A NE.TRY NE.WSPT NM.BLO NW.L44A OH.CPOH 
   OH.KLOH OH.MFOH US.AAM US.ACSO US.BINY US.CBN US.ERPA 
   US.GLMI US.LONY US.MCWV US.TZTN WU.BASO 
 
 Filtering commands used:
   cut o DIST/3.3 -40 o DIST/3.3 +50
   rtr
   taper w 0.1
   hp c 0.03 n 3 
   lp c 0.10 n 3 
 
 Best Fitting Double Couple
  Mo = 3.76e+21 dyne-cm
  Mw = 3.65 
  Z  = 4 km
  Plane   Strike  Dip  Rake
   NP1        5    90   -150
   NP2      275    60     0
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   3.76e+21     21     136
    N   0.00e+00     60       5
    P  -3.76e+21     21     234

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     5.65e+20
       Mxy    -3.21e+21
       Mxz    -1.64e+20
       Myy    -5.65e+20
       Myz     1.87e+21
       Mzz     0.00e+00
                                                     
                                                     
                                                     
                                                     
                     #########-----                  
                 #############---------              
              ###############-------------           
             ################--------------          
           ##################----------------        
          ###################-----------------       
         ####################------------------      
        ########-------------######-------------     
        ###-----------------############--------     
       #--------------------################-----    
       ---------------------##################---    
       ---------------------####################-    
       ---------------------#####################    
        --------------------####################     
        -------------------#####################     
         ----   -----------####################      
          --- P -----------###########   #####       
           --   -----------########### T ####        
             --------------###########   ##          
              -------------###############           
                 ---------#############              
                     -----#########                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
  0.00e+00  -1.64e+20  -1.87e+21 
 -1.64e+20   5.65e+20   3.21e+21 
 -1.87e+21   3.21e+21  -5.65e+20 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230828024326/index.html
        

Preferred Solution

The preferred solution from an analysis of the surface-wave spectral amplitude radiation pattern, waveform inversion or first motion observations is

      STK = 275
      DIP = 60
     RAKE = 0
       MW = 3.65
       HS = 4.0

The NDK file is 20230828024326.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
USGSMWR
 USGS/SLU Moment Tensor Solution
 ENS  2023/08/28 02:43:26:0  41.73  -80.97   5.0 3.6 Ohio
 
 Stations used:
   CN.CHRO CN.EFO CN.GAC CN.KGNO CN.SADO IU.SSPA IU.WCI LD.FOR 
   LD.GCMD LD.GEDE LD.KSCT LD.KSPA LD.MMNY LD.SDMD LD.WVNY 
   LM.NHBP MU.EARS MU.MUG1 N4.E46A N4.I45A N4.I49A N4.J47A 
   N4.J55A N4.J57A N4.J59A N4.K50A N4.K57A N4.L46A N4.L56A 
   N4.L59A N4.M44A N4.M50A N4.M57A N4.N47A N4.N49A N4.N51A 
   N4.N53A N4.N58A N4.N62A N4.O48B N4.O49A N4.O52A N4.O54A 
   N4.P46A N4.P48A N4.P53A N4.Q51A N4.Q52A N4.Q54A N4.R49A 
   N4.R50A N4.R55A N4.S51A N4.S54A N4.SFIN N4.T50A N4.T57A 
   N4.T59A N4.V55A NE.TRY NE.WSPT NM.BLO NW.L44A OH.CPOH 
   OH.KLOH OH.MFOH US.AAM US.ACSO US.BINY US.CBN US.ERPA 
   US.GLMI US.LONY US.MCWV US.TZTN WU.BASO 
 
 Filtering commands used:
   cut o DIST/3.3 -40 o DIST/3.3 +50
   rtr
   taper w 0.1
   hp c 0.03 n 3 
   lp c 0.10 n 3 
 
 Best Fitting Double Couple
  Mo = 3.76e+21 dyne-cm
  Mw = 3.65 
  Z  = 4 km
  Plane   Strike  Dip  Rake
   NP1        5    90   -150
   NP2      275    60     0
  Principal Axes:
   Axis    Value   Plunge  Azimuth
    T   3.76e+21     21     136
    N   0.00e+00     60       5
    P  -3.76e+21     21     234

 Moment Tensor: (dyne-cm)
    Component   Value
       Mxx     5.65e+20
       Mxy    -3.21e+21
       Mxz    -1.64e+20
       Myy    -5.65e+20
       Myz     1.87e+21
       Mzz     0.00e+00
                                                     
                                                     
                                                     
                                                     
                     #########-----                  
                 #############---------              
              ###############-------------           
             ################--------------          
           ##################----------------        
          ###################-----------------       
         ####################------------------      
        ########-------------######-------------     
        ###-----------------############--------     
       #--------------------################-----    
       ---------------------##################---    
       ---------------------####################-    
       ---------------------#####################    
        --------------------####################     
        -------------------#####################     
         ----   -----------####################      
          --- P -----------###########   #####       
           --   -----------########### T ####        
             --------------###########   ##          
              -------------###############           
                 ---------#############              
                     -----#########                  
                                                     
                                                     
                                                     
 Global CMT Convention Moment Tensor:
      R          T          P
  0.00e+00  -1.64e+20  -1.87e+21 
 -1.64e+20   5.65e+20   3.21e+21 
 -1.87e+21   3.21e+21  -5.65e+20 


Details of the solution is found at

http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20230828024326/index.html
	
egional Moment Tensor (Mwr)
Moment 3.229e+14 N-m
Magnitude 3.61 Mwr
Depth 3.0 km
Percent DC 61%
Half Duration -
Catalog US
Data Source US 1
Contributor US 1

Nodal Planes
Plane Strike Dip Rake
NP1 278 49 13
NP2 180 81 138

Principal Axes
Axis Value Plunge Azimuth
T 3.519e+14 N-m 35 130
N -0.691e+14 N-m 48 349
P -2.828e+14 N-m 20

        

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 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.

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

The left panel of the next figure presents the focal mechanism for this earthquake (red) in the context of other nearby events (blue) in the SLU Moment Tensor Catalog. The right panel shows the inferred direction of maximum compressive stress and the type of faulting (green is strike-slip, red is normal, blue is thrust; oblique is shown by a combination of colors). Thus context plot is useful for assessing the appropriateness of the moment tensor of this event.

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 -40 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 n 3 
lp c 0.10 n 3 
The results of this grid search are as follow:

           DEPTH  STK   DIP  RAKE   MW    FIT
WVFGRD96    1.0   275    55     0   3.60 0.4410
WVFGRD96    2.0   275    50     0   3.65 0.4569
WVFGRD96    3.0   275    55     0   3.65 0.4660
WVFGRD96    4.0   275    60     0   3.65 0.4680
WVFGRD96    5.0   275    60     0   3.66 0.4660
WVFGRD96    6.0   275    65    -5   3.66 0.4601
WVFGRD96    7.0   275    65    -5   3.67 0.4518
WVFGRD96    8.0   275    65     0   3.67 0.4408
WVFGRD96    9.0   275    70    -5   3.68 0.4278
WVFGRD96   10.0   275    65    -5   3.69 0.4132
WVFGRD96   11.0   275    70    -5   3.70 0.3980
WVFGRD96   12.0   275    70    -5   3.71 0.3820
WVFGRD96   13.0   275    70    -5   3.71 0.3657
WVFGRD96   14.0    90    65   -15   3.71 0.3513
WVFGRD96   15.0    95    65    -5   3.72 0.3370
WVFGRD96   16.0    95    65    -5   3.73 0.3229
WVFGRD96   17.0    95    65    -5   3.74 0.3089
WVFGRD96   18.0    95    60    -5   3.74 0.2949
WVFGRD96   19.0    95    60    -5   3.74 0.2813
WVFGRD96   20.0    95    55    -5   3.76 0.2680
WVFGRD96   21.0    95    55     0   3.76 0.2559
WVFGRD96   22.0    95    55     0   3.76 0.2442
WVFGRD96   23.0   270    70   -15   3.75 0.2348
WVFGRD96   24.0   270    70   -15   3.76 0.2279
WVFGRD96   25.0   270    70   -15   3.76 0.2212
WVFGRD96   26.0   270    70   -20   3.77 0.2149
WVFGRD96   27.0   270    70   -20   3.77 0.2089
WVFGRD96   28.0   270    65   -15   3.78 0.2040
WVFGRD96   29.0   270    65   -20   3.79 0.2006

The best solution is

WVFGRD96    4.0   275    60     0   3.65 0.4680

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 -40 o DIST/3.3 +50
rtr
taper w 0.1
hp c 0.03 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:

Assuming only a mislocation, the time shifts are fit to a functional form:

 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 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 
Last Changed Tue Apr 23 03:22:23 AM CDT 2024