2016/10/29 22:08:08 42.8257 13.1005 9.9 3.2 Perugia
USGS Felt map for this earthquake
SLU Moment Tensor Solution
ENS 2016/10/29 22:08:08:5 42.83 13.10 9.9 3.2 Perugia
Stations used:
IV.ARVD IV.ATTE IV.FDMO IV.GUMA IV.OFFI IV.SNTG
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +40
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.12 n 3
Best Fitting Double Couple
Mo = 8.22e+20 dyne-cm
Mw = 3.21
Z = 5 km
Plane Strike Dip Rake
NP1 353 61 -96
NP2 185 30 -80
Principal Axes:
Axis Value Plunge Azimuth
T 8.22e+20 15 88
N 0.00e+00 5 356
P -8.22e+20 74 249
Moment Tensor: (dyne-cm)
Component Value
Mxx -7.07e+18
Mxy 9.42e+18
Mxz 8.79e+19
Myy 7.08e+20
Myz 4.14e+20
Mzz -7.01e+20
#####-########
######------##########
######----------############
#####-------------############
######---------------#############
######-----------------#############
######-------------------#############
######--------------------##############
######---------------------#############
#######---------------------######### ##
######----------- --------######### T ##
######----------- P ---------######## ##
######----------- ---------#############
######----------------------############
######----------------------############
######--------------------############
#####--------------------###########
#####-------------------##########
####-----------------#########
#####--------------#########
####------------######
###-------####
Global CMT Convention Moment Tensor:
R T P
-7.01e+20 8.79e+19 -4.14e+20
8.79e+19 -7.07e+18 -9.42e+18
-4.14e+20 -9.42e+18 7.08e+20
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20161029220808/index.html
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STK = 185
DIP = 30
RAKE = -80
MW = 3.21
HS = 5.0
The NDK file is 20161029220808.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2016/10/29 22:08:08:5 42.83 13.10 9.9 3.2 Perugia
Stations used:
IV.ARVD IV.ATTE IV.FDMO IV.GUMA IV.OFFI IV.SNTG
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +40
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.12 n 3
Best Fitting Double Couple
Mo = 8.22e+20 dyne-cm
Mw = 3.21
Z = 5 km
Plane Strike Dip Rake
NP1 353 61 -96
NP2 185 30 -80
Principal Axes:
Axis Value Plunge Azimuth
T 8.22e+20 15 88
N 0.00e+00 5 356
P -8.22e+20 74 249
Moment Tensor: (dyne-cm)
Component Value
Mxx -7.07e+18
Mxy 9.42e+18
Mxz 8.79e+19
Myy 7.08e+20
Myz 4.14e+20
Mzz -7.01e+20
#####-########
######------##########
######----------############
#####-------------############
######---------------#############
######-----------------#############
######-------------------#############
######--------------------##############
######---------------------#############
#######---------------------######### ##
######----------- --------######### T ##
######----------- P ---------######## ##
######----------- ---------#############
######----------------------############
######----------------------############
######--------------------############
#####--------------------###########
#####-------------------##########
####-----------------#########
#####--------------#########
####------------######
###-------####
Global CMT Convention Moment Tensor:
R T P
-7.01e+20 8.79e+19 -4.14e+20
8.79e+19 -7.07e+18 -9.42e+18
-4.14e+20 -9.42e+18 7.08e+20
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20161029220808/index.html
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The focal mechanism was determined using broadband seismic waveforms. The location of the event and the and stations used for 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 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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.12 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 200 30 -50 2.95 0.3220
WVFGRD96 2.0 190 20 -65 3.07 0.3797
WVFGRD96 3.0 190 25 -70 3.08 0.4411
WVFGRD96 4.0 185 30 -80 3.11 0.4623
WVFGRD96 5.0 185 30 -80 3.21 0.4778
WVFGRD96 6.0 190 35 -80 3.21 0.4499
WVFGRD96 7.0 190 35 -80 3.19 0.4058
WVFGRD96 8.0 40 55 -30 3.11 0.3633
WVFGRD96 9.0 40 55 -30 3.12 0.3505
WVFGRD96 10.0 40 55 -30 3.13 0.3364
WVFGRD96 11.0 45 60 -25 3.13 0.3241
WVFGRD96 12.0 125 55 45 3.17 0.3131
WVFGRD96 13.0 130 55 50 3.19 0.3081
WVFGRD96 14.0 125 60 40 3.19 0.3025
WVFGRD96 15.0 125 60 45 3.23 0.3052
WVFGRD96 16.0 130 60 50 3.24 0.2989
WVFGRD96 17.0 150 70 60 3.25 0.3009
WVFGRD96 18.0 150 70 60 3.26 0.3014
WVFGRD96 19.0 150 75 60 3.27 0.3028
WVFGRD96 20.0 150 75 60 3.29 0.3066
WVFGRD96 21.0 150 75 60 3.30 0.3072
WVFGRD96 22.0 150 75 60 3.32 0.3101
WVFGRD96 23.0 145 80 55 3.31 0.3099
WVFGRD96 24.0 150 80 55 3.32 0.3111
WVFGRD96 25.0 145 85 50 3.31 0.3089
WVFGRD96 26.0 145 85 50 3.32 0.3080
WVFGRD96 27.0 110 70 0 3.31 0.3028
WVFGRD96 28.0 320 85 -45 3.30 0.3078
WVFGRD96 29.0 320 80 -40 3.30 0.3111
The best solution is
WVFGRD96 5.0 185 30 -80 3.21 0.4778
The mechanism correspond 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 and because the velocity model used in the predictions may not be perfect. 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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.12 n 3
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| Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to thewavefroms. 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 nnCIA used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
MODEL.01
C.It. A. Di Luzio et al Earth Plan Lettrs 280 (2009) 1-12 Fig 5. 7-8 MODEL/SURF3
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
1.5000 3.7497 2.1436 2.2753 0.500E-02 0.100E-01 0.00 0.00 1.00 1.00
3.0000 4.9399 2.8210 2.4858 0.500E-02 0.100E-01 0.00 0.00 1.00 1.00
3.0000 6.0129 3.4336 2.7058 0.500E-02 0.100E-01 0.00 0.00 1.00 1.00
7.0000 5.5516 3.1475 2.6093 0.167E-02 0.333E-02 0.00 0.00 1.00 1.00
15.0000 5.8805 3.3583 2.6770 0.167E-02 0.333E-02 0.00 0.00 1.00 1.00
6.0000 7.1059 4.0081 3.0002 0.167E-02 0.333E-02 0.00 0.00 1.00 1.00
8.0000 7.1000 3.9864 3.0120 0.167E-02 0.333E-02 0.00 0.00 1.00 1.00
0.0000 7.9000 4.4036 3.2760 0.167E-02 0.333E-02 0.00 0.00 1.00 1.00
Here we tabulate the reasons for not using certain digital data sets
The following stations did not have a valid response files:
DATE=Sat Oct 29 20:32:17 CDT 2016