2016/09/03 01:34:12 42.7753 13.13 10.6 4.3 Perugia
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2016/09/03 01:34:12:1 42.78 13.13 10.6 4.3 Perugia Stations used: IV.AOI IV.ARCI IV.ARVD IV.ASQU IV.ASSB IV.ATFO IV.ATPC IV.ATTE IV.ATVO IV.CAFI IV.CASP IV.CERA IV.CERT IV.CING IV.CRE IV.CSNT IV.FDMO IV.FIAM IV.FNVD IV.FRES IV.FSSB IV.GIUL IV.GUAR IV.GUMA IV.LATE IV.LAV9 IV.LNSS IV.LPEL IV.MA9 IV.MGAB IV.MIDA IV.MODR IV.MTCE IV.MURB IV.OFFI IV.OSSC IV.PARC IV.PESA IV.PIGN IV.POFI IV.PTQR IV.RMP IV.RNI2 IV.SACS IV.SAMA IV.SGRT IV.SNTG IV.SSFR IV.TERO IV.TOLF IV.TRIV IV.VAGA IV.ZCCA Filtering commands used: cut o DIST/3.3 -20 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 = 2.19e+22 dyne-cm Mw = 4.16 Z = 2 km Plane Strike Dip Rake NP1 338 61 -99 NP2 175 30 -75 Principal Axes: Axis Value Plunge Azimuth T 2.19e+22 16 74 N 0.00e+00 7 342 P -2.19e+22 73 227 Moment Tensor: (dyne-cm) Component Value Mxx 6.31e+20 Mxy 4.38e+21 Mxz 5.81e+21 Myy 1.77e+22 Myz 1.01e+22 Mzz -1.83e+22 ---########### ####--################ #####-------################ ####-----------############### #####-------------################ #####----------------############### ######-----------------############### ######-------------------########### # ######--------------------########## T # ######----------------------######### ## ######----------------------############## ######---------- ----------############# #######--------- P -----------############ ######--------- -----------########### ######-----------------------########### ######----------------------########## ######----------------------######## ######---------------------####### #####-------------------###### ######-----------------##### ######--------------## #####--------- Global CMT Convention Moment Tensor: R T P -1.83e+22 5.81e+21 -1.01e+22 5.81e+21 6.31e+20 -4.38e+21 -1.01e+22 -4.38e+21 1.77e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160903013412/index.html |
STK = 175 DIP = 30 RAKE = -75 MW = 4.16 HS = 2.0
The NDK file is 20160903013412.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2016/09/03 01:34:12:1 42.78 13.13 10.6 4.3 Perugia Stations used: IV.AOI IV.ARCI IV.ARVD IV.ASQU IV.ASSB IV.ATFO IV.ATPC IV.ATTE IV.ATVO IV.CAFI IV.CASP IV.CERA IV.CERT IV.CING IV.CRE IV.CSNT IV.FDMO IV.FIAM IV.FNVD IV.FRES IV.FSSB IV.GIUL IV.GUAR IV.GUMA IV.LATE IV.LAV9 IV.LNSS IV.LPEL IV.MA9 IV.MGAB IV.MIDA IV.MODR IV.MTCE IV.MURB IV.OFFI IV.OSSC IV.PARC IV.PESA IV.PIGN IV.POFI IV.PTQR IV.RMP IV.RNI2 IV.SACS IV.SAMA IV.SGRT IV.SNTG IV.SSFR IV.TERO IV.TOLF IV.TRIV IV.VAGA IV.ZCCA Filtering commands used: cut o DIST/3.3 -20 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 = 2.19e+22 dyne-cm Mw = 4.16 Z = 2 km Plane Strike Dip Rake NP1 338 61 -99 NP2 175 30 -75 Principal Axes: Axis Value Plunge Azimuth T 2.19e+22 16 74 N 0.00e+00 7 342 P -2.19e+22 73 227 Moment Tensor: (dyne-cm) Component Value Mxx 6.31e+20 Mxy 4.38e+21 Mxz 5.81e+21 Myy 1.77e+22 Myz 1.01e+22 Mzz -1.83e+22 ---########### ####--################ #####-------################ ####-----------############### #####-------------################ #####----------------############### ######-----------------############### ######-------------------########### # ######--------------------########## T # ######----------------------######### ## ######----------------------############## ######---------- ----------############# #######--------- P -----------############ ######--------- -----------########### ######-----------------------########### ######----------------------########## ######----------------------######## ######---------------------####### #####-------------------###### ######-----------------##### ######--------------## #####--------- Global CMT Convention Moment Tensor: R T P -1.83e+22 5.81e+21 -1.01e+22 5.81e+21 6.31e+20 -4.38e+21 -1.01e+22 -4.38e+21 1.77e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160903013412/index.html |
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.
![]() |
|
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 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 180 30 -65 4.09 0.4957 WVFGRD96 2.0 175 30 -75 4.16 0.5323 WVFGRD96 3.0 170 30 -85 4.17 0.5081 WVFGRD96 4.0 40 55 25 4.08 0.4858 WVFGRD96 5.0 170 30 -80 4.24 0.4870 WVFGRD96 6.0 40 60 35 4.15 0.4726 WVFGRD96 7.0 40 60 30 4.15 0.4583 WVFGRD96 8.0 35 65 25 4.14 0.4530 WVFGRD96 9.0 35 65 20 4.15 0.4372 WVFGRD96 10.0 35 65 20 4.15 0.4210 WVFGRD96 11.0 35 65 20 4.16 0.4045 WVFGRD96 12.0 35 65 20 4.17 0.3881 WVFGRD96 13.0 35 65 20 4.18 0.3723 WVFGRD96 14.0 35 65 20 4.19 0.3583 WVFGRD96 15.0 35 65 20 4.20 0.3392 WVFGRD96 16.0 35 60 20 4.21 0.3264 WVFGRD96 17.0 35 60 20 4.22 0.3168 WVFGRD96 18.0 35 60 20 4.22 0.3092 WVFGRD96 19.0 35 60 20 4.23 0.3026 WVFGRD96 20.0 35 65 20 4.24 0.2967 WVFGRD96 21.0 35 65 20 4.25 0.2930 WVFGRD96 22.0 305 70 25 4.28 0.2965 WVFGRD96 23.0 305 70 25 4.30 0.2988 WVFGRD96 24.0 305 70 25 4.31 0.3004 WVFGRD96 25.0 305 70 25 4.32 0.3049 WVFGRD96 26.0 305 70 25 4.33 0.3077 WVFGRD96 27.0 305 70 25 4.35 0.3103 WVFGRD96 28.0 305 70 25 4.36 0.3110 WVFGRD96 29.0 305 75 25 4.38 0.3106
The best solution is
WVFGRD96 2.0 175 30 -75 4.16 0.5323
The mechanism correspond to the best fit is
![]() |
|
The best fit as a function of depth is given in the following figure:
![]() |
|
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 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3
![]() |
|
![]() |
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=Fri Sep 2 21:40:18 CDT 2016