The ANSS event ID is nm60617031 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/nm60617031/executive.
2026/01/20 07:27:40 39.375 -89.247 8.8 3.5 Illinois
USGS/SLU Moment Tensor Solution
ENS 2026/01/20 07:27:40.0 39.38 -89.25 8.8 3.5 Illinois
Stations used:
AG.LCAR GS.DEC04 GS.DEC05 GS.DEC08 GS.DEC09 IU.CCM IU.WCI
N4.K43A N4.L40A N4.M44A N4.N38B N4.N41A N4.N47A N4.P38B
N4.P40B N4.P46A N4.P48A N4.Q44B N4.R40B N4.R49A N4.S44A
N4.SFIN N4.T45B N4.T47A N4.U49A NM.BLO NM.FVM NM.GLAT
NM.HALT NM.HENM NM.OLIL NM.PARM NM.PEBM NM.PENM NM.SLM
NW.L44A US.HDIL US.SCIA
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +30
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 6.31e+21 dyne-cm
Mw = 3.80
Z = 8 km
Plane Strike Dip Rake
NP1 120 90 -10
NP2 210 80 -180
Principal Axes:
Axis Value Plunge Azimuth
T 6.31e+21 7 165
N 0.00e+00 80 300
P -6.31e+21 7 75
Moment Tensor: (dyne-cm)
Component Value
Mxx 5.38e+21
Mxy -3.11e+21
Mxz -9.49e+20
Myy -5.38e+21
Myz -5.48e+20
Mzz 9.58e+13
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---------############----------------
------------########----------------- P
----------------####------------------ -
------------------------------------------
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-############# #####
########## T #
Global CMT Convention Moment Tensor:
R T P
9.58e+13 -9.49e+20 5.48e+20
-9.49e+20 5.38e+21 3.11e+21
5.48e+20 3.11e+21 -5.38e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260120072740/index.html
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STK = 120
DIP = 90
RAKE = -10
MW = 3.80
HS = 8.0
The NDK file is 20260120072740.ndk The waveform inversion is preferred.
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.
USGS/SLU Moment Tensor Solution
ENS 2026/01/20 07:27:40.0 39.38 -89.25 8.8 3.5 Illinois
Stations used:
AG.LCAR GS.DEC04 GS.DEC05 GS.DEC08 GS.DEC09 IU.CCM IU.WCI
N4.K43A N4.L40A N4.M44A N4.N38B N4.N41A N4.N47A N4.P38B
N4.P40B N4.P46A N4.P48A N4.Q44B N4.R40B N4.R49A N4.S44A
N4.SFIN N4.T45B N4.T47A N4.U49A NM.BLO NM.FVM NM.GLAT
NM.HALT NM.HENM NM.OLIL NM.PARM NM.PEBM NM.PENM NM.SLM
NW.L44A US.HDIL US.SCIA
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +30
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 6.31e+21 dyne-cm
Mw = 3.80
Z = 8 km
Plane Strike Dip Rake
NP1 120 90 -10
NP2 210 80 -180
Principal Axes:
Axis Value Plunge Azimuth
T 6.31e+21 7 165
N 0.00e+00 80 300
P -6.31e+21 7 75
Moment Tensor: (dyne-cm)
Component Value
Mxx 5.38e+21
Mxy -3.11e+21
Mxz -9.49e+20
Myy -5.38e+21
Myz -5.48e+20
Mzz 9.58e+13
##############
#####################-
######################------
#####################---------
######################------------
######################--------------
-----################-----------------
---------############----------------
------------########----------------- P
----------------####------------------ -
------------------------------------------
------------------#####-------------------
-----------------#########----------------
---------------#############------------
--------------#################---------
------------#####################-----
----------##########################
--------##########################
------########################
----########################
-############# #####
########## T #
Global CMT Convention Moment Tensor:
R T P
9.58e+13 -9.49e+20 5.48e+20
-9.49e+20 5.38e+21 3.11e+21
5.48e+20 3.11e+21 -5.38e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260120072740/index.html
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Regional Moment Tensor (Mwr) Moment 5.933e+14 N-m Magnitude 3.78 Mwr Depth 7.0 km Percent DC 94% Half Duration - Catalog US Data Source US Contributor US Nodal Planes Plane Strike Dip Rake NP1 300 86 9 NP2 209 81 176 Principal Axes Axis Value Plunge Azimuth T 5.843e+14 9 165 N 0.175e+14 80 322 P -6.018e+14 4 74 |
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 +30 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 125 70 25 3.74 0.6156
WVFGRD96 2.0 300 85 15 3.73 0.6360
WVFGRD96 3.0 300 85 10 3.74 0.6536
WVFGRD96 4.0 300 85 10 3.76 0.6674
WVFGRD96 5.0 300 85 10 3.77 0.6776
WVFGRD96 6.0 300 85 10 3.78 0.6847
WVFGRD96 7.0 300 85 10 3.79 0.6891
WVFGRD96 8.0 120 90 -10 3.80 0.6910
WVFGRD96 9.0 120 90 -5 3.81 0.6908
WVFGRD96 10.0 120 90 -10 3.83 0.6891
WVFGRD96 11.0 120 90 -10 3.84 0.6845
WVFGRD96 12.0 300 85 10 3.85 0.6784
WVFGRD96 13.0 300 85 10 3.85 0.6708
WVFGRD96 14.0 300 85 10 3.86 0.6618
WVFGRD96 15.0 300 80 10 3.87 0.6521
WVFGRD96 16.0 300 80 10 3.87 0.6423
WVFGRD96 17.0 300 80 10 3.88 0.6315
WVFGRD96 18.0 300 80 10 3.88 0.6215
WVFGRD96 19.0 300 80 10 3.89 0.6119
WVFGRD96 20.0 300 80 10 3.90 0.6022
WVFGRD96 21.0 300 80 10 3.90 0.5951
WVFGRD96 22.0 300 80 10 3.91 0.5883
WVFGRD96 23.0 300 80 10 3.91 0.5827
WVFGRD96 24.0 300 80 10 3.92 0.5778
WVFGRD96 25.0 300 80 10 3.92 0.5736
WVFGRD96 26.0 300 75 10 3.93 0.5717
WVFGRD96 27.0 300 80 10 3.93 0.5715
WVFGRD96 28.0 300 75 10 3.94 0.5718
WVFGRD96 29.0 300 80 10 3.94 0.5711
The best solution is
WVFGRD96 8.0 120 90 -10 3.80 0.6910
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 +30 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 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