2013/06/29 09:00:47 44.150 10.174 5.3 3.3 Italy
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2013/06/29 09:00:47:0 44.15 10.17 5.3 3.3 Italy Stations used: GU.GORR GU.MAIM GU.PCP GU.POPM IV.ASQU IV.BDI IV.BOB IV.CAFI IV.CRE IV.CRMI IV.CSNT IV.MGAB IV.MSSA IV.PARC IV.PLMA IV.QLNO IV.ROVR MN.VLC Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.12e+21 dyne-cm Mw = 3.30 Z = 2 km Plane Strike Dip Rake NP1 252 50 -113 NP2 105 45 -65 Principal Axes: Axis Value Plunge Azimuth T 1.12e+21 3 358 N 0.00e+00 17 267 P -1.12e+21 72 96 Moment Tensor: (dyne-cm) Component Value Mxx 1.12e+21 Mxy -3.62e+19 Mxz 8.68e+19 Myy -9.95e+19 Myz -3.24e+20 Mzz -1.02e+21 ##### T ###### ######### ########## ############################ ############################## ################################## #################--------------##### #############-----------------------## ##########------------------------------ ########-------------------------------- --#####----------------------------------- ---##------------------- --------------- ------------------------ P --------------- ---##------------------- --------------- -#####---------------------------------- ########-------------------------------# ##########--------------------------## #############------------------##### ################################## ############################## ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -1.02e+21 8.68e+19 3.24e+20 8.68e+19 1.12e+21 3.62e+19 3.24e+20 3.62e+19 -9.95e+19 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130629090047/index.html |
STK = 105 DIP = 45 RAKE = -65 MW = 3.30 HS = 2.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2013/06/29 09:00:47:0 44.15 10.17 5.3 3.3 Italy Stations used: GU.GORR GU.MAIM GU.PCP GU.POPM IV.ASQU IV.BDI IV.BOB IV.CAFI IV.CRE IV.CRMI IV.CSNT IV.MGAB IV.MSSA IV.PARC IV.PLMA IV.QLNO IV.ROVR MN.VLC Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 1.12e+21 dyne-cm Mw = 3.30 Z = 2 km Plane Strike Dip Rake NP1 252 50 -113 NP2 105 45 -65 Principal Axes: Axis Value Plunge Azimuth T 1.12e+21 3 358 N 0.00e+00 17 267 P -1.12e+21 72 96 Moment Tensor: (dyne-cm) Component Value Mxx 1.12e+21 Mxy -3.62e+19 Mxz 8.68e+19 Myy -9.95e+19 Myz -3.24e+20 Mzz -1.02e+21 ##### T ###### ######### ########## ############################ ############################## ################################## #################--------------##### #############-----------------------## ##########------------------------------ ########-------------------------------- --#####----------------------------------- ---##------------------- --------------- ------------------------ P --------------- ---##------------------- --------------- -#####---------------------------------- ########-------------------------------# ##########--------------------------## #############------------------##### ################################## ############################## ############################ ###################### ############## Global CMT Convention Moment Tensor: R T P -1.02e+21 8.68e+19 3.24e+20 8.68e+19 1.12e+21 3.62e+19 3.24e+20 3.62e+19 -9.95e+19 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20130629090047/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:
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 1.0 105 45 -65 3.25 0.4582 WVFGRD96 2.0 105 45 -65 3.30 0.4830 WVFGRD96 3.0 110 45 -60 3.32 0.4553 WVFGRD96 4.0 315 70 5 3.23 0.4524 WVFGRD96 5.0 120 55 -45 3.34 0.4515 WVFGRD96 6.0 315 65 -5 3.30 0.4452 WVFGRD96 7.0 310 65 -15 3.31 0.4426 WVFGRD96 8.0 310 70 -10 3.30 0.4347 WVFGRD96 9.0 310 70 -10 3.31 0.4256 WVFGRD96 10.0 135 70 10 3.33 0.4207 WVFGRD96 11.0 140 65 15 3.35 0.4155 WVFGRD96 12.0 140 65 15 3.36 0.4111 WVFGRD96 13.0 140 65 15 3.37 0.4077 WVFGRD96 14.0 140 65 15 3.39 0.4036 WVFGRD96 15.0 140 60 20 3.40 0.3968 WVFGRD96 16.0 140 60 20 3.41 0.3918 WVFGRD96 17.0 140 60 20 3.42 0.3869 WVFGRD96 18.0 140 60 20 3.43 0.3816 WVFGRD96 19.0 140 60 25 3.44 0.3774 WVFGRD96 20.0 140 60 25 3.45 0.3736 WVFGRD96 21.0 140 60 25 3.45 0.3692 WVFGRD96 22.0 140 60 25 3.46 0.3638 WVFGRD96 23.0 140 60 25 3.47 0.3599 WVFGRD96 24.0 140 60 25 3.47 0.3560 WVFGRD96 25.0 140 65 25 3.48 0.3522 WVFGRD96 26.0 140 65 30 3.49 0.3494 WVFGRD96 27.0 140 65 25 3.50 0.3467 WVFGRD96 28.0 140 65 25 3.51 0.3426 WVFGRD96 29.0 140 70 25 3.53 0.3387
The best solution is
WVFGRD96 2.0 105 45 -65 3.30 0.4830
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=Tue Jul 2 09:19:40 CDT 2013