The ANSS event ID is nn00916412 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/nn00916412/executive.
2026/04/25 12:11:01 39.336 -118.976 9.1 3.8 Nevada
USGS/SLU Moment Tensor Solution
ENS 2026/04/25 12:11:01.0 39.34 -118.98 9.1 3.8 Nevada
Stations used:
BK.BIGV BK.BUCR BK.EAGL BK.GCKB BK.GUMB BK.HATC BK.HELL
BK.LCOW BK.MNLT BK.OVRO BK.PATT BK.RAVE BK.SWNM BK.WELL
BK.YUBA CI.CWC CI.GRA CI.MPM CI.WRC2 IM.NV31 LB.BMN LB.TPH
NC.AFD NC.LDH NN.BEK NN.BFC NN.DIX NN.KVN NN.LHV NN.MPK
NN.PAH NN.PRN NN.Q09A NN.R11B NN.YER UO.ADEL UO.PRONG
US.ELK US.TPNV
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 0.07 n 3
Best Fitting Double Couple
Mo = 3.89e+21 dyne-cm
Mw = 3.66
Z = 8 km
Plane Strike Dip Rake
NP1 60 90 -10
NP2 150 80 -180
Principal Axes:
Axis Value Plunge Azimuth
T 3.89e+21 7 105
N 0.00e+00 80 240
P -3.89e+21 7 15
Moment Tensor: (dyne-cm)
Component Value
Mxx -3.32e+21
Mxy -1.92e+21
Mxz -5.85e+20
Myy 3.32e+21
Myz 3.38e+20
Mzz 5.91e+13
---------- P -
#------------- -----
####------------------------
######------------------------
########--------------------------
##########--------------------------
############---------------------#####
##############-----------------#########
###############-------------############
#################---------################
##################-----###################
##########################################
################----################## #
############--------################# T
#########------------################
#####----------------#################
----------------------##############
----------------------############
---------------------#########
----------------------######
---------------------#
--------------
Global CMT Convention Moment Tensor:
R T P
5.91e+13 -5.85e+20 -3.38e+20
-5.85e+20 -3.32e+21 1.92e+21
-3.38e+20 1.92e+21 3.32e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260425121101/index.html
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STK = 60
DIP = 90
RAKE = -10
MW = 3.66
HS = 8.0
The NDK file is 20260425121101.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 2026/04/25 12:11:01.0 39.34 -118.98 9.1 3.8 Nevada
Stations used:
BK.BIGV BK.BUCR BK.EAGL BK.GCKB BK.GUMB BK.HATC BK.HELL
BK.LCOW BK.MNLT BK.OVRO BK.PATT BK.RAVE BK.SWNM BK.WELL
BK.YUBA CI.CWC CI.GRA CI.MPM CI.WRC2 IM.NV31 LB.BMN LB.TPH
NC.AFD NC.LDH NN.BEK NN.BFC NN.DIX NN.KVN NN.LHV NN.MPK
NN.PAH NN.PRN NN.Q09A NN.R11B NN.YER UO.ADEL UO.PRONG
US.ELK US.TPNV
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 0.07 n 3
Best Fitting Double Couple
Mo = 3.89e+21 dyne-cm
Mw = 3.66
Z = 8 km
Plane Strike Dip Rake
NP1 60 90 -10
NP2 150 80 -180
Principal Axes:
Axis Value Plunge Azimuth
T 3.89e+21 7 105
N 0.00e+00 80 240
P -3.89e+21 7 15
Moment Tensor: (dyne-cm)
Component Value
Mxx -3.32e+21
Mxy -1.92e+21
Mxz -5.85e+20
Myy 3.32e+21
Myz 3.38e+20
Mzz 5.91e+13
---------- P -
#------------- -----
####------------------------
######------------------------
########--------------------------
##########--------------------------
############---------------------#####
##############-----------------#########
###############-------------############
#################---------################
##################-----###################
##########################################
################----################## #
############--------################# T
#########------------################
#####----------------#################
----------------------##############
----------------------############
---------------------#########
----------------------######
---------------------#
--------------
Global CMT Convention Moment Tensor:
R T P
5.91e+13 -5.85e+20 -3.38e+20
-5.85e+20 -3.32e+21 1.92e+21
-3.38e+20 1.92e+21 3.32e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20260425121101/index.html
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Regional Moment Tensor (Mwr) Moment 4.032e+14 N-m Magnitude 3.67 Mwr Depth 8.0 km Percent DC 98% Half Duration - Catalog US Data Source US Contributor US Nodal Planes Plane Strike Dip Rake NP1 149 87 -172 NP2 59 82 -3 Principal Axes Axis Value Plunge Azimuth T 4.047e+14 4 284 N -0.031e+14 82 167 P -4.016e+14 7 14 |
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: 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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 60 85 0 3.34 0.3808
WVFGRD96 2.0 60 80 5 3.46 0.5077
WVFGRD96 3.0 60 85 0 3.50 0.5620
WVFGRD96 4.0 60 85 -5 3.54 0.5974
WVFGRD96 5.0 60 85 -5 3.57 0.6211
WVFGRD96 6.0 60 85 -5 3.60 0.6367
WVFGRD96 7.0 60 85 -5 3.63 0.6470
WVFGRD96 8.0 60 90 -10 3.66 0.6534
WVFGRD96 9.0 240 80 10 3.68 0.6515
WVFGRD96 10.0 240 80 10 3.69 0.6468
WVFGRD96 11.0 240 80 10 3.71 0.6402
WVFGRD96 12.0 240 80 10 3.72 0.6316
WVFGRD96 13.0 240 75 10 3.73 0.6227
WVFGRD96 14.0 240 75 10 3.74 0.6133
WVFGRD96 15.0 240 75 10 3.75 0.6032
WVFGRD96 16.0 240 75 10 3.76 0.5929
WVFGRD96 17.0 240 75 10 3.77 0.5824
WVFGRD96 18.0 240 70 10 3.78 0.5718
WVFGRD96 19.0 240 70 10 3.79 0.5615
WVFGRD96 20.0 240 70 10 3.80 0.5514
WVFGRD96 21.0 240 70 10 3.80 0.5414
WVFGRD96 22.0 240 70 10 3.81 0.5311
WVFGRD96 23.0 240 70 10 3.81 0.5209
WVFGRD96 24.0 240 70 10 3.82 0.5110
WVFGRD96 25.0 240 70 10 3.82 0.5013
WVFGRD96 26.0 240 70 10 3.83 0.4919
WVFGRD96 27.0 240 70 10 3.83 0.4826
WVFGRD96 28.0 240 70 10 3.84 0.4731
WVFGRD96 29.0 240 70 10 3.84 0.4636
The best solution is
WVFGRD96 8.0 60 90 -10 3.66 0.6534
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.07 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 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