2018/08/16 20:22:34 41.88 14.88 9.0 4.4 Gropparella
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2018/08/16 20:22:34:0 41.88 14.88 9.0 4.4 Gropparella Stations used: IV.AMUR IV.ARVD IV.BSSO IV.CERA IV.CERT IV.CESX IV.CMPR IV.GATE IV.LPEL IV.MA9 IV.MCRV IV.MELA IV.MIDA IV.MSAG IV.MTCE IV.NOCI IV.PIGN IV.POFI IV.RNI2 IV.SACR IV.SNAL IV.TERO IV.TOLF IV.TRIV IV.VAGA Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 5.96e+22 dyne-cm Mw = 4.45 Z = 14 km Plane Strike Dip Rake NP1 244 85 170 NP2 335 80 5 Principal Axes: Axis Value Plunge Azimuth T 5.96e+22 11 199 N 0.00e+00 79 38 P -5.96e+22 4 290 Moment Tensor: (dyne-cm) Component Value Mxx 4.44e+22 Mxy 3.69e+22 Mxz -1.14e+22 Myy -4.62e+22 Myz -6.66e+19 Mzz 1.78e+21 ############## ---################### --------#################### ----------#################### -------------##################### ----------------#################### ----------------#################--- P -----------------###########--------- ------------------######------------- -----------------------#------------------ --------------------###------------------- ----------------########------------------ -------------############----------------- --------#################--------------- -----#####################-------------- -########################------------- #########################----------- ########################---------- #######################------- ###### #############------ ### T ##############-- ############ Global CMT Convention Moment Tensor: R T P 1.78e+21 -1.14e+22 6.66e+19 -1.14e+22 4.44e+22 -3.69e+22 6.66e+19 -3.69e+22 -4.62e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20180816202234/index.html |
STK = 335 DIP = 80 RAKE = 5 MW = 4.45 HS = 14.0
The NDK file is 20180816202234.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2018/08/16 20:22:34:0 41.88 14.88 9.0 4.4 Gropparella Stations used: IV.AMUR IV.ARVD IV.BSSO IV.CERA IV.CERT IV.CESX IV.CMPR IV.GATE IV.LPEL IV.MA9 IV.MCRV IV.MELA IV.MIDA IV.MSAG IV.MTCE IV.NOCI IV.PIGN IV.POFI IV.RNI2 IV.SACR IV.SNAL IV.TERO IV.TOLF IV.TRIV IV.VAGA Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3 Best Fitting Double Couple Mo = 5.96e+22 dyne-cm Mw = 4.45 Z = 14 km Plane Strike Dip Rake NP1 244 85 170 NP2 335 80 5 Principal Axes: Axis Value Plunge Azimuth T 5.96e+22 11 199 N 0.00e+00 79 38 P -5.96e+22 4 290 Moment Tensor: (dyne-cm) Component Value Mxx 4.44e+22 Mxy 3.69e+22 Mxz -1.14e+22 Myy -4.62e+22 Myz -6.66e+19 Mzz 1.78e+21 ############## ---################### --------#################### ----------#################### -------------##################### ----------------#################### ----------------#################--- P -----------------###########--------- ------------------######------------- -----------------------#------------------ --------------------###------------------- ----------------########------------------ -------------############----------------- --------#################--------------- -----#####################-------------- -########################------------- #########################----------- ########################---------- #######################------- ###### #############------ ### T ##############-- ############ Global CMT Convention Moment Tensor: R T P 1.78e+21 -1.14e+22 6.66e+19 -1.14e+22 4.44e+22 -3.69e+22 6.66e+19 -3.69e+22 -4.62e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20180816202234/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:
cut o DIST/3.3 -20 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.05 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 335 80 -15 4.19 0.3038 WVFGRD96 2.0 335 80 -15 4.24 0.3415 WVFGRD96 3.0 335 80 -10 4.28 0.3709 WVFGRD96 4.0 335 80 -5 4.31 0.3969 WVFGRD96 5.0 335 75 -10 4.35 0.4194 WVFGRD96 6.0 335 75 -5 4.37 0.4299 WVFGRD96 7.0 335 75 -5 4.38 0.4344 WVFGRD96 8.0 335 80 5 4.39 0.4369 WVFGRD96 9.0 335 75 5 4.41 0.4389 WVFGRD96 10.0 335 75 5 4.42 0.4397 WVFGRD96 11.0 335 75 5 4.43 0.4398 WVFGRD96 12.0 335 75 5 4.44 0.4400 WVFGRD96 13.0 335 80 5 4.44 0.4397 WVFGRD96 14.0 335 80 5 4.45 0.4402 WVFGRD96 15.0 335 80 5 4.46 0.4391 WVFGRD96 16.0 335 80 5 4.47 0.4361 WVFGRD96 17.0 335 80 5 4.48 0.4332 WVFGRD96 18.0 335 80 5 4.49 0.4297 WVFGRD96 19.0 335 85 5 4.49 0.4262 WVFGRD96 20.0 335 85 5 4.50 0.4226 WVFGRD96 21.0 335 85 5 4.51 0.4196 WVFGRD96 22.0 250 85 -5 4.51 0.4160 WVFGRD96 23.0 70 90 0 4.51 0.4152 WVFGRD96 24.0 70 90 0 4.53 0.4173 WVFGRD96 25.0 70 90 0 4.54 0.4191 WVFGRD96 26.0 250 85 0 4.56 0.4237 WVFGRD96 27.0 70 90 0 4.57 0.4233 WVFGRD96 28.0 70 90 0 4.59 0.4265 WVFGRD96 29.0 70 90 0 4.61 0.4297
The best solution is
WVFGRD96 14.0 335 80 5 4.45 0.4402
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 0.02 n 3 lp c 0.05 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=Thu Aug 16 17:00:04 CDT 2018