2013/01/04 07:50:06 37.873 14.722 10.1 4.3 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2013/01/04 07:50:06:0 37.87 14.72 10.1 4.3 Italy Stations used: IV.ALJA IV.GALF IV.GIB IV.HAGA IV.HAVL IV.HCRL IV.HMDC IV.MILZ IV.MPAZ IV.MSCL IV.MSFR IV.MSRU IV.NOV IV.SOLUN MN.CEL Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.60e+22 dyne-cm Mw = 4.07 Z = 9 km Plane Strike Dip Rake NP1 88 56 -113 NP2 305 40 -60 Principal Axes: Axis Value Plunge Azimuth T 1.60e+22 9 194 N 0.00e+00 19 101 P -1.60e+22 69 307 Moment Tensor: (dyne-cm) Component Value Mxx 1.40e+22 Mxy 4.66e+21 Mxz -5.50e+21 Myy -3.44e+20 Myz 3.65e+21 Mzz -1.37e+22 ############## ###################### ############################ ##------------################ ---------------------############# -------------------------########### ----------------------------########## -------------------------------######### --------------- ---------------####### ---------------- P ----------------####### ---------------- -----------------###### -------------------------------------###-- ##---------------------------------------- ####-------------------------------##--- #######------------------------######--- ##############--------##############-- ###################################- ################################## ############################## ############################ ##### ############## # T ########## Global CMT Convention Moment Tensor: R T P -1.37e+22 -5.50e+21 -3.65e+21 -5.50e+21 1.40e+22 -4.66e+21 -3.65e+21 -4.66e+21 -3.44e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130104075006/index.html |
STK = 305 DIP = 40 RAKE = -60 MW = 4.07 HS = 9.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2013/01/04 07:50:06:0 37.87 14.72 10.1 4.3 Italy Stations used: IV.ALJA IV.GALF IV.GIB IV.HAGA IV.HAVL IV.HCRL IV.HMDC IV.MILZ IV.MPAZ IV.MSCL IV.MSFR IV.MSRU IV.NOV IV.SOLUN MN.CEL Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.60e+22 dyne-cm Mw = 4.07 Z = 9 km Plane Strike Dip Rake NP1 88 56 -113 NP2 305 40 -60 Principal Axes: Axis Value Plunge Azimuth T 1.60e+22 9 194 N 0.00e+00 19 101 P -1.60e+22 69 307 Moment Tensor: (dyne-cm) Component Value Mxx 1.40e+22 Mxy 4.66e+21 Mxz -5.50e+21 Myy -3.44e+20 Myz 3.65e+21 Mzz -1.37e+22 ############## ###################### ############################ ##------------################ ---------------------############# -------------------------########### ----------------------------########## -------------------------------######### --------------- ---------------####### ---------------- P ----------------####### ---------------- -----------------###### -------------------------------------###-- ##---------------------------------------- ####-------------------------------##--- #######------------------------######--- ##############--------##############-- ###################################- ################################## ############################## ############################ ##### ############## # T ########## Global CMT Convention Moment Tensor: R T P -1.37e+22 -5.50e+21 -3.65e+21 -5.50e+21 1.40e+22 -4.66e+21 -3.65e+21 -4.66e+21 -3.44e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130104075006/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 1.0 290 35 -85 3.88 0.3123 WVFGRD96 2.0 295 30 -75 3.95 0.3151 WVFGRD96 3.0 305 60 -35 3.94 0.3268 WVFGRD96 4.0 310 55 -30 3.96 0.3540 WVFGRD96 5.0 295 20 -75 4.09 0.3838 WVFGRD96 6.0 295 25 -75 4.10 0.4297 WVFGRD96 7.0 295 30 -75 4.10 0.4657 WVFGRD96 8.0 295 35 -75 4.08 0.4868 WVFGRD96 9.0 305 40 -60 4.07 0.4889 WVFGRD96 10.0 305 40 -60 4.07 0.4858 WVFGRD96 11.0 310 40 -55 4.07 0.4772 WVFGRD96 12.0 315 45 -45 4.06 0.4669 WVFGRD96 13.0 315 50 -35 4.06 0.4564 WVFGRD96 14.0 315 55 -30 4.07 0.4476 WVFGRD96 15.0 315 55 -30 4.09 0.4395 WVFGRD96 16.0 315 55 -30 4.10 0.4296 WVFGRD96 17.0 315 55 -30 4.10 0.4186 WVFGRD96 18.0 315 60 -25 4.11 0.4075 WVFGRD96 19.0 315 60 -25 4.11 0.3962 WVFGRD96 20.0 315 60 -25 4.12 0.3843 WVFGRD96 21.0 320 60 -20 4.12 0.3723 WVFGRD96 22.0 320 65 -25 4.12 0.3609 WVFGRD96 23.0 345 55 25 4.10 0.3552 WVFGRD96 24.0 345 55 25 4.11 0.3491 WVFGRD96 25.0 345 55 25 4.11 0.3435 WVFGRD96 26.0 345 55 25 4.12 0.3380 WVFGRD96 27.0 345 55 25 4.13 0.3331 WVFGRD96 28.0 340 60 25 4.14 0.3296 WVFGRD96 29.0 340 60 25 4.15 0.3264
The best solution is
WVFGRD96 9.0 305 40 -60 4.07 0.4889
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=Fri Jan 4 07:20:46 CST 2013