2013/07/12 03:34:06 44.206 10.108 10.8 3.5 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2013/07/12 03:34:06:0 44.21 10.11 10.8 3.5 Italy Stations used: GU.BHB GU.ENR GU.FINB GU.GORR GU.MAIM GU.PCP GU.PZZ GU.STV IV.ARVD IV.ASQU IV.BDI IV.BOB IV.CASP IV.CRMI IV.CSNT IV.DOI IV.GROG IV.MGAB IV.MSSA IV.OSSC IV.PLMA IV.QLNO IV.SSFR MN.VLC Filtering commands used: cut a -10 a 70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.53e+21 dyne-cm Mw = 3.39 Z = 7 km Plane Strike Dip Rake NP1 291 55 -87 NP2 105 35 -95 Principal Axes: Axis Value Plunge Azimuth T 1.53e+21 10 19 N 0.00e+00 3 109 P -1.53e+21 80 215 Moment Tensor: (dyne-cm) Component Value Mxx 1.30e+21 Mxy 4.25e+20 Mxz 4.76e+20 Myy 1.34e+20 Myz 2.41e+20 Mzz -1.43e+21 ############ ################ T ### ################### ###### ############################## ################################## ######--------###################### #---------------------################ ---------------------------############# ------------------------------########## #--------------------------------######### ##---------------------------------####### ###--------------- ----------------##### ####-------------- P -----------------#### ####------------- ------------------## #####----------------------------------- ######-------------------------------# ########-------------------------### ##########-------------------##### ################----########## ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -1.43e+21 4.76e+20 -2.41e+20 4.76e+20 1.30e+21 -4.25e+20 -2.41e+20 -4.25e+20 1.34e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130712033406/index.html |
STK = 105 DIP = 35 RAKE = -95 MW = 3.39 HS = 7.0
The NDK file is 20130712033406.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2013/07/12 03:34:06:0 44.21 10.11 10.8 3.5 Italy Stations used: GU.BHB GU.ENR GU.FINB GU.GORR GU.MAIM GU.PCP GU.PZZ GU.STV IV.ARVD IV.ASQU IV.BDI IV.BOB IV.CASP IV.CRMI IV.CSNT IV.DOI IV.GROG IV.MGAB IV.MSSA IV.OSSC IV.PLMA IV.QLNO IV.SSFR MN.VLC Filtering commands used: cut a -10 a 70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.53e+21 dyne-cm Mw = 3.39 Z = 7 km Plane Strike Dip Rake NP1 291 55 -87 NP2 105 35 -95 Principal Axes: Axis Value Plunge Azimuth T 1.53e+21 10 19 N 0.00e+00 3 109 P -1.53e+21 80 215 Moment Tensor: (dyne-cm) Component Value Mxx 1.30e+21 Mxy 4.25e+20 Mxz 4.76e+20 Myy 1.34e+20 Myz 2.41e+20 Mzz -1.43e+21 ############ ################ T ### ################### ###### ############################## ################################## ######--------###################### #---------------------################ ---------------------------############# ------------------------------########## #--------------------------------######### ##---------------------------------####### ###--------------- ----------------##### ####-------------- P -----------------#### ####------------- ------------------## #####----------------------------------- ######-------------------------------# ########-------------------------### ##########-------------------##### ################----########## ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -1.43e+21 4.76e+20 -2.41e+20 4.76e+20 1.30e+21 -4.25e+20 -2.41e+20 -4.25e+20 1.34e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130712033406/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 70 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 1.0 340 90 -35 3.05 0.3477 WVFGRD96 2.0 160 90 60 3.18 0.3742 WVFGRD96 3.0 325 65 -50 3.22 0.4635 WVFGRD96 4.0 310 55 -65 3.27 0.5304 WVFGRD96 5.0 310 55 -70 3.37 0.5726 WVFGRD96 6.0 105 40 -100 3.40 0.6409 WVFGRD96 7.0 105 35 -95 3.39 0.6499 WVFGRD96 8.0 290 55 -85 3.35 0.6175 WVFGRD96 9.0 290 55 -85 3.34 0.5841 WVFGRD96 10.0 290 55 -85 3.33 0.5487 WVFGRD96 11.0 295 60 -80 3.33 0.5193 WVFGRD96 12.0 295 60 -80 3.33 0.4940 WVFGRD96 13.0 295 60 -80 3.34 0.4698 WVFGRD96 14.0 295 65 -80 3.34 0.4482 WVFGRD96 15.0 295 65 -80 3.38 0.4328 WVFGRD96 16.0 295 65 -85 3.39 0.4129 WVFGRD96 17.0 300 70 -80 3.39 0.3971 WVFGRD96 18.0 300 70 -80 3.40 0.3816 WVFGRD96 19.0 300 70 -80 3.41 0.3629 WVFGRD96 20.0 305 75 -80 3.41 0.3445 WVFGRD96 21.0 305 75 -80 3.42 0.3289 WVFGRD96 22.0 325 80 -60 3.37 0.3114 WVFGRD96 23.0 325 80 -65 3.38 0.3000 WVFGRD96 24.0 240 35 30 3.42 0.2901 WVFGRD96 25.0 240 35 30 3.43 0.2861 WVFGRD96 26.0 240 35 30 3.44 0.2819 WVFGRD96 27.0 245 35 35 3.45 0.2771 WVFGRD96 28.0 250 45 25 3.46 0.2721 WVFGRD96 29.0 250 45 25 3.47 0.2725
The best solution is
WVFGRD96 7.0 105 35 -95 3.39 0.6499
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 70 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=Fri Jul 12 08:17:45 CDT 2013