The ANSS event ID is usp000hhj8 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/usp000hhj8/executive.
2010/08/05 00:04:17 43.596 -110.391 5.0 4.8 Wyoming
USGS/SLU Moment Tensor Solution
ENS 2010/08/05 00:04:17:0 43.60 -110.39 5.0 4.8 Wyoming
Stations used:
IU.RSSD IW.DLMT IW.FLWY IW.FXWY IW.IMW IW.MFID IW.MOOW
IW.PHWY IW.REDW IW.TPAW TA.E21A TA.E22A TA.F20A TA.F21A
TA.F22A TA.G20A TA.G21A TA.H17A TA.H19A TA.H20A TA.H22A
TA.I19A TA.I20A TA.I21A TA.J19A TA.J20A TA.K24A TA.K25A
TA.N23A US.AHID US.BOZ US.DUG US.HWUT US.LAO US.LKWY US.MSO
US.RLMT UU.BGU UU.HVU UU.MPU UU.NLU UU.NOQ UU.SPU UU.TCU
WY.YHB WY.YUF XV.BH1A XV.BH1B XV.BH1F XV.BH2A XV.BH2B
XV.BH2F XV.BH3A XV.BH3F XV.BH4A XV.BHM2 XV.BHM5 XV.BHM6
XV.BHM7 YX.C19 YX.D01 YX.D02 Z2.CFWY Z2.CSR Z2.HPWY Z2.IPID
Z2.RRWY Z2.SNFF Z2.WYMT
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 0.06 n 3
Best Fitting Double Couple
Mo = 2.54e+23 dyne-cm
Mw = 4.87
Z = 9 km
Plane Strike Dip Rake
NP1 45 75 -25
NP2 142 66 -164
Principal Axes:
Axis Value Plunge Azimuth
T 2.54e+23 6 95
N 0.00e+00 61 196
P -2.54e+23 28 2
Moment Tensor: (dyne-cm)
Component Value
Mxx -1.96e+23
Mxy -2.68e+22
Mxz -1.08e+23
Myy 2.49e+23
Myz 2.36e+22
Mzz -5.37e+22
--------------
---------- ---------
#------------ P ------------
##------------ ------------#
####---------------------------###
######-------------------------#####
#######------------------------#######
#########---------------------##########
##########-------------------###########
############-----------------#############
#############--------------############
##############-----------############## T
###############---------###############
################-----###################
#################--#####################
###############---####################
############-------#################
########-------------#############
###------------------#########
------------------------####
----------------------
--------------
Global CMT Convention Moment Tensor:
R T P
-5.37e+22 -1.08e+23 -2.36e+22
-1.08e+23 -1.96e+23 2.68e+22
-2.36e+22 2.68e+22 2.49e+23
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20100805000417/index.html
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STK = 45
DIP = 75
RAKE = -25
MW = 4.87
HS = 9.0
The NDK file is 20100805000417.ndk The waveform inversion is preferred.
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 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 225 90 0 4.55 0.4602
WVFGRD96 2.0 225 80 5 4.65 0.5833
WVFGRD96 3.0 225 80 5 4.70 0.6382
WVFGRD96 4.0 225 85 10 4.73 0.6734
WVFGRD96 5.0 45 80 -20 4.77 0.7069
WVFGRD96 6.0 45 80 -20 4.80 0.7329
WVFGRD96 7.0 45 80 -20 4.82 0.7534
WVFGRD96 8.0 40 70 -30 4.87 0.7680
WVFGRD96 9.0 45 75 -25 4.87 0.7733
WVFGRD96 10.0 45 75 -20 4.88 0.7725
WVFGRD96 11.0 45 75 -20 4.89 0.7686
WVFGRD96 12.0 45 75 -20 4.90 0.7620
WVFGRD96 13.0 45 75 -20 4.91 0.7535
WVFGRD96 14.0 45 75 -20 4.92 0.7475
WVFGRD96 15.0 45 75 -15 4.93 0.7418
WVFGRD96 16.0 45 75 -15 4.94 0.7343
WVFGRD96 17.0 45 75 -15 4.94 0.7251
WVFGRD96 18.0 45 75 -15 4.95 0.7148
WVFGRD96 19.0 45 75 -15 4.96 0.7041
WVFGRD96 20.0 45 75 -15 4.96 0.6933
WVFGRD96 21.0 45 75 -15 4.97 0.6816
WVFGRD96 22.0 45 75 -15 4.98 0.6698
WVFGRD96 23.0 45 75 -15 4.98 0.6582
WVFGRD96 24.0 45 80 -15 4.98 0.6464
WVFGRD96 25.0 45 75 -10 4.99 0.6341
WVFGRD96 26.0 45 75 -10 5.00 0.6227
WVFGRD96 27.0 45 75 -10 5.00 0.6106
WVFGRD96 28.0 45 80 -10 5.01 0.5987
WVFGRD96 29.0 45 80 -10 5.01 0.5876
The best solution is
WVFGRD96 9.0 45 75 -25 4.87 0.7733
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 -30 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 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