2012/11/25 08:28:39 39.921 16.027 7.5 3.7 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution
ENS 2012/11/25 08:28:39:0 39.92 16.03 7.5 3.7 Italy
Stations used:
IV.BULG IV.CAR1 IV.CDRU IV.CELI IV.CET2 IV.CMPR IV.MCEL
IV.MGR IV.MIGL IV.MRLC IV.MTSN IV.SALB IV.SERS IV.SIRI
IV.SLCN MN.CUC MN.TIP
Filtering commands used:
hp c 0.02 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 4.79e+21 dyne-cm
Mw = 3.72
Z = 5 km
Plane Strike Dip Rake
NP1 345 50 -90
NP2 165 40 -90
Principal Axes:
Axis Value Plunge Azimuth
T 4.79e+21 5 75
N 0.00e+00 -0 165
P -4.79e+21 85 255
Moment Tensor: (dyne-cm)
Component Value
Mxx 3.16e+20
Mxy 1.18e+21
Mxz 2.15e+20
Myy 4.40e+21
Myz 8.03e+20
Mzz -4.71e+21
#--###########
###--------###########
#####-----------############
#####--------------###########
######----------------############
######-------------------###########
#######--------------------###########
#######---------------------##########
#######----------------------######### T
########-----------------------########
########-------- ------------###########
#########------- P ------------###########
#########------- -------------##########
########-----------------------#########
#########----------------------#########
#########---------------------########
#########-------------------########
#########------------------#######
#########---------------######
##########------------######
#########---------####
##########---#
Global CMT Convention Moment Tensor:
R T P
-4.71e+21 2.15e+20 -8.03e+20
2.15e+20 3.16e+20 -1.18e+21
-8.03e+20 -1.18e+21 4.40e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20121125082839/index.html
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STK = 345
DIP = 50
RAKE = -90
MW = 3.72
HS = 5.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2012/11/25 08:28:39:0 39.92 16.03 7.5 3.7 Italy
Stations used:
IV.BULG IV.CAR1 IV.CDRU IV.CELI IV.CET2 IV.CMPR IV.MCEL
IV.MGR IV.MIGL IV.MRLC IV.MTSN IV.SALB IV.SERS IV.SIRI
IV.SLCN MN.CUC MN.TIP
Filtering commands used:
hp c 0.02 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 4.79e+21 dyne-cm
Mw = 3.72
Z = 5 km
Plane Strike Dip Rake
NP1 345 50 -90
NP2 165 40 -90
Principal Axes:
Axis Value Plunge Azimuth
T 4.79e+21 5 75
N 0.00e+00 -0 165
P -4.79e+21 85 255
Moment Tensor: (dyne-cm)
Component Value
Mxx 3.16e+20
Mxy 1.18e+21
Mxz 2.15e+20
Myy 4.40e+21
Myz 8.03e+20
Mzz -4.71e+21
#--###########
###--------###########
#####-----------############
#####--------------###########
######----------------############
######-------------------###########
#######--------------------###########
#######---------------------##########
#######----------------------######### T
########-----------------------########
########-------- ------------###########
#########------- P ------------###########
#########------- -------------##########
########-----------------------#########
#########----------------------#########
#########---------------------########
#########-------------------########
#########------------------#######
#########---------------######
##########------------######
#########---------####
##########---#
Global CMT Convention Moment Tensor:
R T P
-4.71e+21 2.15e+20 -8.03e+20
2.15e+20 3.16e+20 -1.18e+21
-8.03e+20 -1.18e+21 4.40e+21
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20121125082839/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 0.10 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 20 70 -55 3.45 0.3454
WVFGRD96 2.0 10 60 -60 3.54 0.4106
WVFGRD96 3.0 5 50 -65 3.58 0.4579
WVFGRD96 4.0 345 50 -90 3.64 0.4782
WVFGRD96 5.0 345 50 -90 3.72 0.5257
WVFGRD96 6.0 165 40 -90 3.71 0.4876
WVFGRD96 7.0 25 65 -30 3.62 0.4628
WVFGRD96 8.0 35 70 25 3.61 0.4601
WVFGRD96 9.0 35 75 25 3.61 0.4505
WVFGRD96 10.0 35 75 25 3.62 0.4402
WVFGRD96 11.0 35 80 25 3.62 0.4275
WVFGRD96 12.0 35 80 25 3.63 0.4170
WVFGRD96 13.0 35 80 25 3.64 0.4063
WVFGRD96 14.0 35 80 20 3.66 0.3957
WVFGRD96 15.0 35 85 25 3.67 0.3847
WVFGRD96 16.0 30 90 25 3.68 0.3741
WVFGRD96 17.0 210 85 -25 3.69 0.3662
WVFGRD96 18.0 210 85 -25 3.69 0.3592
WVFGRD96 19.0 210 85 -25 3.70 0.3528
WVFGRD96 20.0 210 85 -25 3.71 0.3468
WVFGRD96 21.0 210 85 -25 3.72 0.3419
WVFGRD96 22.0 30 70 -20 3.75 0.3361
WVFGRD96 23.0 30 70 -20 3.76 0.3335
WVFGRD96 24.0 30 75 -20 3.76 0.3328
WVFGRD96 25.0 30 75 -20 3.77 0.3314
WVFGRD96 26.0 30 80 -20 3.77 0.3301
WVFGRD96 27.0 210 85 20 3.78 0.3289
WVFGRD96 28.0 210 85 20 3.79 0.3269
WVFGRD96 29.0 210 90 15 3.81 0.3271
The best solution is
WVFGRD96 5.0 345 50 -90 3.72 0.5257
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 0.10 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=Mon Nov 26 13:58:00 CST 2012