2013/11/30 20:13:38 42.638 13.217 11.4 3.90 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution
ENS 2013/11/30 20:13:38:0 42.64 13.22 11.4 3.9 Italy
Stations used:
IV.AOI IV.ARVD IV.ASQU IV.CAFI IV.CAMP IV.CERA IV.CESI
IV.CESX IV.CING IV.CRE IV.CSNT IV.FDMO IV.FIAM IV.FSSB
IV.GIUL IV.GUAR IV.INTR IV.LAV9 IV.LNSS IV.LPEL IV.MA9
IV.MAON IV.MGAB IV.MSAG IV.MTCE IV.MURB IV.NRCA IV.OSSC
IV.PARC IV.PIEI IV.POFI IV.PTQR IV.RNI2 IV.ROM9 IV.SACS
IV.SAMA IV.SNTG IV.SSFR IV.TERO IV.TOLF MN.AQU
Filtering commands used:
cut a -10 a 60
rtr
taper w 0.1
hp c 0.02 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 4.03e+21 dyne-cm
Mw = 3.67
Z = 7 km
Plane Strike Dip Rake
NP1 333 61 -99
NP2 170 30 -75
Principal Axes:
Axis Value Plunge Azimuth
T 4.03e+21 16 69
N 0.00e+00 7 337
P -4.03e+21 73 222
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.80e+20
Mxy 1.07e+21
Mxz 1.23e+21
Myy 3.09e+21
Myz 1.76e+21
Mzz -3.37e+21
--############
###-##################
####------##################
####----------################
#####------------#################
#####---------------################
#####-----------------############ #
######-------------------########## T ##
#####---------------------######### ##
######----------------------##############
######-----------------------#############
######----------- ---------#############
#######---------- P ----------############
######---------- -----------##########
#######-----------------------##########
######-----------------------#########
######-----------------------#######
#######---------------------######
######-------------------#####
#######-----------------####
######---------------#
######--------
Global CMT Convention Moment Tensor:
R T P
-3.37e+21 1.23e+21 -1.76e+21
1.23e+21 2.80e+20 -1.07e+21
-1.76e+21 -1.07e+21 3.09e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20131130201338/index.html
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STK = 170
DIP = 30
RAKE = -75
MW = 3.67
HS = 7.0
The NDK file is 20131130201338.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2013/11/30 20:13:38:0 42.64 13.22 11.4 3.9 Italy
Stations used:
IV.AOI IV.ARVD IV.ASQU IV.CAFI IV.CAMP IV.CERA IV.CESI
IV.CESX IV.CING IV.CRE IV.CSNT IV.FDMO IV.FIAM IV.FSSB
IV.GIUL IV.GUAR IV.INTR IV.LAV9 IV.LNSS IV.LPEL IV.MA9
IV.MAON IV.MGAB IV.MSAG IV.MTCE IV.MURB IV.NRCA IV.OSSC
IV.PARC IV.PIEI IV.POFI IV.PTQR IV.RNI2 IV.ROM9 IV.SACS
IV.SAMA IV.SNTG IV.SSFR IV.TERO IV.TOLF MN.AQU
Filtering commands used:
cut a -10 a 60
rtr
taper w 0.1
hp c 0.02 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 4.03e+21 dyne-cm
Mw = 3.67
Z = 7 km
Plane Strike Dip Rake
NP1 333 61 -99
NP2 170 30 -75
Principal Axes:
Axis Value Plunge Azimuth
T 4.03e+21 16 69
N 0.00e+00 7 337
P -4.03e+21 73 222
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.80e+20
Mxy 1.07e+21
Mxz 1.23e+21
Myy 3.09e+21
Myz 1.76e+21
Mzz -3.37e+21
--############
###-##################
####------##################
####----------################
#####------------#################
#####---------------################
#####-----------------############ #
######-------------------########## T ##
#####---------------------######### ##
######----------------------##############
######-----------------------#############
######----------- ---------#############
#######---------- P ----------############
######---------- -----------##########
#######-----------------------##########
######-----------------------#########
######-----------------------#######
#######---------------------######
######-------------------#####
#######-----------------####
######---------------#
######--------
Global CMT Convention Moment Tensor:
R T P
-3.37e+21 1.23e+21 -1.76e+21
1.23e+21 2.80e+20 -1.07e+21
-1.76e+21 -1.07e+21 3.09e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20131130201338/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 a -10 a 60 rtr taper w 0.1 hp c 0.02 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 1.0 160 50 -85 3.43 0.3328
WVFGRD96 2.0 5 45 -45 3.46 0.3413
WVFGRD96 3.0 195 30 -30 3.50 0.3727
WVFGRD96 4.0 175 25 -65 3.55 0.4326
WVFGRD96 5.0 170 25 -70 3.66 0.4935
WVFGRD96 6.0 165 25 -80 3.68 0.5333
WVFGRD96 7.0 170 30 -75 3.67 0.5477
WVFGRD96 8.0 170 30 -70 3.63 0.5310
WVFGRD96 9.0 180 35 -60 3.63 0.5193
WVFGRD96 10.0 190 35 -50 3.63 0.5043
WVFGRD96 11.0 190 35 -45 3.63 0.4870
WVFGRD96 12.0 215 55 15 3.63 0.4709
WVFGRD96 13.0 210 60 15 3.64 0.4599
WVFGRD96 14.0 210 60 15 3.65 0.4486
WVFGRD96 15.0 205 40 -25 3.69 0.4281
WVFGRD96 16.0 215 55 15 3.68 0.4150
WVFGRD96 17.0 215 55 15 3.68 0.3999
WVFGRD96 18.0 215 55 15 3.69 0.3853
WVFGRD96 19.0 215 55 15 3.69 0.3717
WVFGRD96 20.0 215 55 15 3.70 0.3586
WVFGRD96 21.0 220 55 15 3.71 0.3470
WVFGRD96 22.0 220 55 20 3.71 0.3366
WVFGRD96 23.0 220 55 20 3.72 0.3278
WVFGRD96 24.0 220 55 20 3.73 0.3202
WVFGRD96 25.0 220 55 20 3.74 0.3129
WVFGRD96 26.0 305 60 35 3.76 0.3128
WVFGRD96 27.0 305 60 35 3.77 0.3115
WVFGRD96 28.0 305 60 35 3.78 0.3080
WVFGRD96 29.0 210 60 20 3.78 0.3057
The best solution is
WVFGRD96 7.0 170 30 -75 3.67 0.5477
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 a -10 a 60 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.10 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 Nov 30 15:25:47 CST 2013