2013/10/19 12:29:35 43.675 10.274 9.9 3.40 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2013/10/19 12:29:35:0 43.67 10.27 9.9 3.4 Italy Stations used: FR.TURF GU.ENR GU.FINB GU.GORR GU.MAIM GU.PCP GU.POPM GU.STV IV.ARVD IV.ASQU IV.BDI IV.CAFI IV.CASP IV.CELB IV.CING IV.CRE IV.CRMI IV.FDMO IV.FNVD IV.GROG IV.MAON IV.MGAB IV.MSSA IV.MTRZ IV.MURB IV.PESA IV.PIEI IV.PLMA IV.QLNO IV.SACS IV.SNTG MN.VLC Filtering commands used: cut a -10 a 80 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 2.16e+21 dyne-cm Mw = 3.49 Z = 6 km Plane Strike Dip Rake NP1 5 60 -50 NP2 126 48 -138 Principal Axes: Axis Value Plunge Azimuth T 2.16e+21 7 68 N 0.00e+00 34 162 P -2.16e+21 55 328 Moment Tensor: (dyne-cm) Component Value Mxx -1.98e+20 Mxy 1.06e+21 Mxz -7.65e+20 Myy 1.63e+21 Myz 7.65e+20 Mzz -1.43e+21 ----------#### ---------------####### -------------------######### ---------------------######### ------------------------########## #------------------------########### ##----------- ----------########## ###----------- P -----------######### T ####---------- -----------######### ######-----------------------############# #######----------------------############# ########---------------------############# #########-------------------############## ##########-----------------############# ###########----------------############# #############------------############# ###############--------############# #################-----############ ###################----------- #################----------- ############---------- #######------- Global CMT Convention Moment Tensor: R T P -1.43e+21 -7.65e+20 -7.65e+20 -7.65e+20 -1.98e+20 -1.06e+21 -7.65e+20 -1.06e+21 1.63e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20131019122935/index.html |
STK = 5 DIP = 60 RAKE = -50 MW = 3.49 HS = 6.0
The NDK file is 20131019122935.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2013/10/19 12:29:35:0 43.67 10.27 9.9 3.4 Italy Stations used: FR.TURF GU.ENR GU.FINB GU.GORR GU.MAIM GU.PCP GU.POPM GU.STV IV.ARVD IV.ASQU IV.BDI IV.CAFI IV.CASP IV.CELB IV.CING IV.CRE IV.CRMI IV.FDMO IV.FNVD IV.GROG IV.MAON IV.MGAB IV.MSSA IV.MTRZ IV.MURB IV.PESA IV.PIEI IV.PLMA IV.QLNO IV.SACS IV.SNTG MN.VLC Filtering commands used: cut a -10 a 80 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 2.16e+21 dyne-cm Mw = 3.49 Z = 6 km Plane Strike Dip Rake NP1 5 60 -50 NP2 126 48 -138 Principal Axes: Axis Value Plunge Azimuth T 2.16e+21 7 68 N 0.00e+00 34 162 P -2.16e+21 55 328 Moment Tensor: (dyne-cm) Component Value Mxx -1.98e+20 Mxy 1.06e+21 Mxz -7.65e+20 Myy 1.63e+21 Myz 7.65e+20 Mzz -1.43e+21 ----------#### ---------------####### -------------------######### ---------------------######### ------------------------########## #------------------------########### ##----------- ----------########## ###----------- P -----------######### T ####---------- -----------######### ######-----------------------############# #######----------------------############# ########---------------------############# #########-------------------############## ##########-----------------############# ###########----------------############# #############------------############# ###############--------############# #################-----############ ###################----------- #################----------- ############---------- #######------- Global CMT Convention Moment Tensor: R T P -1.43e+21 -7.65e+20 -7.65e+20 -7.65e+20 -1.98e+20 -1.06e+21 -7.65e+20 -1.06e+21 1.63e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20131019122935/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.
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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 80 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 1.0 290 75 10 3.17 0.2625 WVFGRD96 2.0 295 50 20 3.29 0.2854 WVFGRD96 3.0 5 60 -50 3.37 0.3510 WVFGRD96 4.0 0 55 -55 3.42 0.4049 WVFGRD96 5.0 -5 55 -65 3.51 0.4453 WVFGRD96 6.0 5 60 -50 3.49 0.4478 WVFGRD96 7.0 10 65 -40 3.48 0.4293 WVFGRD96 8.0 15 70 -35 3.46 0.4154 WVFGRD96 9.0 15 70 -30 3.47 0.4094 WVFGRD96 10.0 15 70 -30 3.48 0.4026 WVFGRD96 11.0 15 70 -30 3.49 0.3957 WVFGRD96 12.0 15 75 -30 3.50 0.3882 WVFGRD96 13.0 15 75 -30 3.51 0.3791 WVFGRD96 14.0 15 75 -25 3.52 0.3698 WVFGRD96 15.0 15 75 -30 3.54 0.3580 WVFGRD96 16.0 15 75 -30 3.55 0.3472 WVFGRD96 17.0 15 75 -30 3.56 0.3351 WVFGRD96 18.0 20 70 15 3.54 0.3206 WVFGRD96 19.0 20 70 15 3.55 0.3124 WVFGRD96 20.0 20 65 10 3.55 0.3050 WVFGRD96 21.0 20 65 10 3.56 0.2980 WVFGRD96 22.0 20 65 10 3.57 0.2922 WVFGRD96 23.0 25 60 20 3.57 0.2853 WVFGRD96 24.0 205 65 15 3.60 0.2840 WVFGRD96 25.0 205 65 10 3.60 0.2800 WVFGRD96 26.0 205 65 10 3.61 0.2764 WVFGRD96 27.0 200 70 10 3.63 0.2761 WVFGRD96 28.0 200 75 15 3.65 0.2740 WVFGRD96 29.0 200 80 15 3.68 0.2740
The best solution is
WVFGRD96 6.0 5 60 -50 3.49 0.4478
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 80 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 Oct 19 09:53:42 CDT 2013