2016/08/27 10:40:14 42.8382 13.2462 6.8 3.6 Ascoli
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2016/08/27 10:40:14:0 42.84 13.25 6.8 3.6 Ascoli Stations used: IV.AOI IV.ARCI IV.ARVD IV.ASQU IV.ASSB IV.ATFO IV.ATPC IV.ATTE IV.ATVO IV.CAFI IV.CASP IV.CELB IV.CERA IV.CERT IV.CESX IV.CING IV.CRE IV.CRMI IV.CSNT IV.FDMO IV.FIAM IV.GUAR IV.GUMA IV.LATE IV.LAV9 IV.LNSS IV.LPEL IV.MA9 IV.MGAB IV.MODR IV.MTCE IV.MURB IV.NRCA IV.OFFI IV.OSSC IV.PARC IV.PESA IV.PIEI IV.PIGN IV.POFI IV.PTQR IV.RMP IV.RNI2 IV.SACR IV.SACS IV.SNTG IV.TERO IV.TOLF Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 2.48e+21 dyne-cm Mw = 3.53 Z = 2 km Plane Strike Dip Rake NP1 175 65 -60 NP2 301 38 -137 Principal Axes: Axis Value Plunge Azimuth T 2.48e+21 15 244 N 0.00e+00 27 341 P -2.48e+21 59 128 Moment Tensor: (dyne-cm) Component Value Mxx 2.08e+20 Mxy 1.25e+21 Mxz 4.02e+20 Myy 1.44e+21 Myz -1.42e+21 Mzz -1.65e+21 ----########## -------############### ---------################### ----######-----############### -##########-----------############ ############--------------########## #############----------------######### ##############------------------######## ##############--------------------###### ##############----------------------###### ###############----------------------##### ###############-----------------------#### ###############----------- ---------#### ##############----------- P ----------## ## ##########---------- ----------## # T ##########-----------------------# ###########---------------------- #############--------------------- ############------------------ ############---------------- ##########------------ ########------ Global CMT Convention Moment Tensor: R T P -1.65e+21 4.02e+20 1.42e+21 4.02e+20 2.08e+20 -1.25e+21 1.42e+21 -1.25e+21 1.44e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160827104014/index.html |
STK = 175 DIP = 65 RAKE = -60 MW = 3.53 HS = 2.0
The NDK file is 20160827104014.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2016/08/27 10:40:14:0 42.84 13.25 6.8 3.6 Ascoli Stations used: IV.AOI IV.ARCI IV.ARVD IV.ASQU IV.ASSB IV.ATFO IV.ATPC IV.ATTE IV.ATVO IV.CAFI IV.CASP IV.CELB IV.CERA IV.CERT IV.CESX IV.CING IV.CRE IV.CRMI IV.CSNT IV.FDMO IV.FIAM IV.GUAR IV.GUMA IV.LATE IV.LAV9 IV.LNSS IV.LPEL IV.MA9 IV.MGAB IV.MODR IV.MTCE IV.MURB IV.NRCA IV.OFFI IV.OSSC IV.PARC IV.PESA IV.PIEI IV.PIGN IV.POFI IV.PTQR IV.RMP IV.RNI2 IV.SACR IV.SACS IV.SNTG IV.TERO IV.TOLF Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3 Best Fitting Double Couple Mo = 2.48e+21 dyne-cm Mw = 3.53 Z = 2 km Plane Strike Dip Rake NP1 175 65 -60 NP2 301 38 -137 Principal Axes: Axis Value Plunge Azimuth T 2.48e+21 15 244 N 0.00e+00 27 341 P -2.48e+21 59 128 Moment Tensor: (dyne-cm) Component Value Mxx 2.08e+20 Mxy 1.25e+21 Mxz 4.02e+20 Myy 1.44e+21 Myz -1.42e+21 Mzz -1.65e+21 ----########## -------############### ---------################### ----######-----############### -##########-----------############ ############--------------########## #############----------------######### ##############------------------######## ##############--------------------###### ##############----------------------###### ###############----------------------##### ###############-----------------------#### ###############----------- ---------#### ##############----------- P ----------## ## ##########---------- ----------## # T ##########-----------------------# ###########---------------------- #############--------------------- ############------------------ ############---------------- ##########------------ ########------ Global CMT Convention Moment Tensor: R T P -1.65e+21 4.02e+20 1.42e+21 4.02e+20 2.08e+20 -1.25e+21 1.42e+21 -1.25e+21 1.44e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160827104014/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 o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 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 1.0 180 65 -55 3.47 0.5053 WVFGRD96 2.0 175 65 -60 3.53 0.5203 WVFGRD96 3.0 170 65 -65 3.55 0.5037 WVFGRD96 4.0 20 70 30 3.50 0.4791 WVFGRD96 5.0 160 60 -75 3.64 0.4840 WVFGRD96 6.0 20 65 30 3.56 0.4658 WVFGRD96 7.0 20 65 30 3.57 0.4557 WVFGRD96 8.0 20 65 25 3.57 0.4487 WVFGRD96 9.0 20 65 25 3.58 0.4324 WVFGRD96 10.0 15 70 20 3.58 0.4151 WVFGRD96 11.0 15 70 20 3.59 0.3972 WVFGRD96 12.0 15 65 20 3.60 0.3791 WVFGRD96 13.0 15 65 25 3.61 0.3616 WVFGRD96 14.0 15 65 25 3.61 0.3454 WVFGRD96 15.0 15 65 25 3.63 0.3233 WVFGRD96 16.0 15 65 30 3.63 0.3078 WVFGRD96 17.0 15 65 30 3.64 0.2966 WVFGRD96 18.0 15 65 30 3.64 0.2861 WVFGRD96 19.0 15 65 30 3.65 0.2765 WVFGRD96 20.0 15 65 30 3.65 0.2679 WVFGRD96 21.0 110 60 30 3.70 0.2734 WVFGRD96 22.0 110 60 25 3.71 0.2796 WVFGRD96 23.0 110 55 25 3.73 0.2849 WVFGRD96 24.0 110 60 25 3.74 0.2904 WVFGRD96 25.0 110 60 25 3.75 0.2944 WVFGRD96 26.0 110 60 25 3.77 0.2977 WVFGRD96 27.0 105 65 20 3.78 0.2991 WVFGRD96 28.0 105 65 20 3.79 0.2998 WVFGRD96 29.0 105 65 20 3.81 0.2977
The best solution is
WVFGRD96 2.0 175 65 -60 3.53 0.5203
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 o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 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 Aug 27 07:20:07 CDT 2016