2012/10/01 20:28:28 39.901 16.013 8.1 3.6 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution
ENS 2012/10/01 20:28:28:0 39.90 16.01 8.1 3.6 Italy
Stations used:
IV.BULG IV.CAR1 IV.CDRU IV.CELI IV.CET2 IV.CMPR IV.MCEL
IV.MGR IV.MTSN IV.SALB IV.SIRI IV.SLCN MN.CUC MN.TIP
Filtering commands used:
hp c 0.02 n 3
lp c 0.06 n 3
Best Fitting Double Couple
Mo = 5.69e+21 dyne-cm
Mw = 3.77
Z = 5 km
Plane Strike Dip Rake
NP1 330 45 -90
NP2 150 45 -90
Principal Axes:
Axis Value Plunge Azimuth
T 5.69e+21 -0 60
N 0.00e+00 -0 330
P -5.69e+21 90 185
Moment Tensor: (dyne-cm)
Component Value
Mxx 1.42e+21
Mxy 2.46e+21
Mxz -2.77e+14
Myy 4.27e+21
Myz -1.27e+14
Mzz -5.69e+21
##############
------################
##-----------###############
###--------------#############
####------------------###########
#####-------------------########## T
######---------------------########
#######----------------------###########
#######-----------------------##########
########------------------------##########
#########------------------------#########
#########---------- -----------#########
##########--------- P ------------########
##########-------- ------------#######
###########----------------------#######
###########---------------------######
############-------------------#####
############------------------####
#############--------------###
###############-----------##
################------
##############
Global CMT Convention Moment Tensor:
R T P
-5.69e+21 -2.77e+14 1.27e+14
-2.77e+14 1.42e+21 -2.46e+21
1.27e+14 -2.46e+21 4.27e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20121001202828/index.html
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STK = 150
DIP = 45
RAKE = -90
MW = 3.77
HS = 5.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2012/10/01 20:28:28:0 39.90 16.01 8.1 3.6 Italy
Stations used:
IV.BULG IV.CAR1 IV.CDRU IV.CELI IV.CET2 IV.CMPR IV.MCEL
IV.MGR IV.MTSN IV.SALB IV.SIRI IV.SLCN MN.CUC MN.TIP
Filtering commands used:
hp c 0.02 n 3
lp c 0.06 n 3
Best Fitting Double Couple
Mo = 5.69e+21 dyne-cm
Mw = 3.77
Z = 5 km
Plane Strike Dip Rake
NP1 330 45 -90
NP2 150 45 -90
Principal Axes:
Axis Value Plunge Azimuth
T 5.69e+21 -0 60
N 0.00e+00 -0 330
P -5.69e+21 90 185
Moment Tensor: (dyne-cm)
Component Value
Mxx 1.42e+21
Mxy 2.46e+21
Mxz -2.77e+14
Myy 4.27e+21
Myz -1.27e+14
Mzz -5.69e+21
##############
------################
##-----------###############
###--------------#############
####------------------###########
#####-------------------########## T
######---------------------########
#######----------------------###########
#######-----------------------##########
########------------------------##########
#########------------------------#########
#########---------- -----------#########
##########--------- P ------------########
##########-------- ------------#######
###########----------------------#######
###########---------------------######
############-------------------#####
############------------------####
#############--------------###
###############-----------##
################------
##############
Global CMT Convention Moment Tensor:
R T P
-5.69e+21 -2.77e+14 1.27e+14
-2.77e+14 1.42e+21 -2.46e+21
1.27e+14 -2.46e+21 4.27e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20121001202828/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:
hp c 0.02 n 3 lp c 0.06 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT
WVFGRD96 1.0 170 45 -60 3.57 0.4547
WVFGRD96 2.0 165 45 -70 3.64 0.5277
WVFGRD96 3.0 155 45 -85 3.69 0.5708
WVFGRD96 4.0 335 45 -90 3.70 0.5633
WVFGRD96 5.0 150 45 -90 3.77 0.6062
WVFGRD96 6.0 335 45 -85 3.75 0.5322
WVFGRD96 7.0 340 40 -80 3.72 0.4523
WVFGRD96 8.0 15 75 -15 3.60 0.4518
WVFGRD96 9.0 15 75 -10 3.60 0.4490
WVFGRD96 10.0 15 75 -10 3.61 0.4449
WVFGRD96 11.0 15 75 -10 3.62 0.4406
WVFGRD96 12.0 15 70 -10 3.63 0.4374
WVFGRD96 13.0 15 70 -10 3.64 0.4349
WVFGRD96 14.0 20 65 10 3.64 0.4333
WVFGRD96 15.0 5 40 -40 3.72 0.4379
WVFGRD96 16.0 10 45 -35 3.71 0.4351
WVFGRD96 17.0 -5 55 -50 3.71 0.4333
WVFGRD96 18.0 -5 55 -50 3.72 0.4370
WVFGRD96 19.0 -5 55 -50 3.73 0.4398
WVFGRD96 20.0 -5 55 -50 3.73 0.4417
WVFGRD96 21.0 -5 55 -50 3.74 0.4423
WVFGRD96 22.0 0 55 -45 3.75 0.4422
WVFGRD96 23.0 0 55 -45 3.76 0.4419
WVFGRD96 24.0 0 55 -45 3.76 0.4394
WVFGRD96 25.0 0 55 -45 3.77 0.4360
WVFGRD96 26.0 10 75 -30 3.76 0.4323
WVFGRD96 27.0 10 75 -25 3.77 0.4291
WVFGRD96 28.0 10 75 -25 3.78 0.4244
WVFGRD96 29.0 20 75 15 3.78 0.4261
The best solution is
WVFGRD96 5.0 150 45 -90 3.77 0.6062
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
hp c 0.02 n 3 lp c 0.06 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=Tue Oct 2 08:01:31 CDT 2012