2017/11/19 12:37:43 44.66 10.07 32.0 4.4 Fornovp
USGS Felt map for this earthquake
SLU Moment Tensor Solution ENS 2017/11/19 12:37:43:0 44.66 10.07 32.0 4.4 Fornovp Stations used: CH.BERNI CH.MUGIO FR.ESCA FR.MON FR.SAOF FR.SPIF FR.TURF GU.RSP IV.BRMO IV.CASP IV.CELB IV.CRMI IV.CSNT IV.IMI IV.MSSA IV.OSSC IV.PARC IV.PLMA IV.QLNO IV.SALO MN.VLC 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 = 3.31e+22 dyne-cm Mw = 4.28 Z = 20 km Plane Strike Dip Rake NP1 337 58 116 NP2 115 40 55 Principal Axes: Axis Value Plunge Azimuth T 3.31e+22 66 297 N 0.00e+00 22 143 P -3.31e+22 10 49 Moment Tensor: (dyne-cm) Component Value Mxx -1.26e+22 Mxy -1.81e+22 Mxz 1.88e+21 Myy -1.41e+22 Myz -1.52e+22 Mzz 2.67e+22 -------------- #######--------------- ############---------------- ###############------------- ###################----------- P - ######################--------- -- ########################-------------- -#########################-------------- --########### ###########------------- ---########### T ############------------- ----########## ############------------- -----#########################------------ ------########################------------ ------########################---------- --------######################---------- ---------####################--------- -----------#################-------# --------------#############----### -------------------------##### -----------------------##### --------------------## -------------- Global CMT Convention Moment Tensor: R T P 2.67e+22 1.88e+21 1.52e+22 1.88e+21 -1.26e+22 1.81e+22 1.52e+22 1.81e+22 -1.41e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20171119123743/index.html |
STK = 115 DIP = 40 RAKE = 55 MW = 4.28 HS = 20.0
The NDK file is 20171119123743.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution ENS 2017/11/19 12:37:43:0 44.66 10.07 32.0 4.4 Fornovp Stations used: CH.BERNI CH.MUGIO FR.ESCA FR.MON FR.SAOF FR.SPIF FR.TURF GU.RSP IV.BRMO IV.CASP IV.CELB IV.CRMI IV.CSNT IV.IMI IV.MSSA IV.OSSC IV.PARC IV.PLMA IV.QLNO IV.SALO MN.VLC 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 = 3.31e+22 dyne-cm Mw = 4.28 Z = 20 km Plane Strike Dip Rake NP1 337 58 116 NP2 115 40 55 Principal Axes: Axis Value Plunge Azimuth T 3.31e+22 66 297 N 0.00e+00 22 143 P -3.31e+22 10 49 Moment Tensor: (dyne-cm) Component Value Mxx -1.26e+22 Mxy -1.81e+22 Mxz 1.88e+21 Myy -1.41e+22 Myz -1.52e+22 Mzz 2.67e+22 -------------- #######--------------- ############---------------- ###############------------- ###################----------- P - ######################--------- -- ########################-------------- -#########################-------------- --########### ###########------------- ---########### T ############------------- ----########## ############------------- -----#########################------------ ------########################------------ ------########################---------- --------######################---------- ---------####################--------- -----------#################-------# --------------#############----### -------------------------##### -----------------------##### --------------------## -------------- Global CMT Convention Moment Tensor: R T P 2.67e+22 1.88e+21 1.52e+22 1.88e+21 -1.26e+22 1.81e+22 1.52e+22 1.81e+22 -1.41e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20171119123743/index.html |
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(a) ML computed using the IASPEI formula for Horizontal components; (b) ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
(a) ML computed using the IASPEI formula for Vertical components (research); (b) ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
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 1.0 320 45 -90 3.92 0.3696 WVFGRD96 2.0 140 40 -90 3.99 0.3595 WVFGRD96 3.0 300 45 60 3.96 0.2700 WVFGRD96 4.0 90 60 -30 3.93 0.2819 WVFGRD96 5.0 80 45 -30 4.02 0.2965 WVFGRD96 6.0 80 35 -10 4.03 0.3286 WVFGRD96 7.0 90 30 10 4.06 0.3661 WVFGRD96 8.0 85 35 5 4.04 0.4032 WVFGRD96 9.0 95 35 20 4.07 0.4368 WVFGRD96 10.0 95 35 20 4.09 0.4681 WVFGRD96 11.0 100 40 30 4.11 0.4981 WVFGRD96 12.0 105 40 35 4.13 0.5257 WVFGRD96 13.0 105 45 40 4.15 0.5517 WVFGRD96 14.0 110 45 50 4.17 0.5780 WVFGRD96 15.0 115 45 55 4.21 0.6056 WVFGRD96 16.0 115 45 55 4.23 0.6300 WVFGRD96 17.0 115 40 55 4.24 0.6490 WVFGRD96 18.0 115 40 55 4.25 0.6645 WVFGRD96 19.0 115 40 55 4.27 0.6743 WVFGRD96 20.0 115 40 55 4.28 0.6784 WVFGRD96 21.0 115 40 55 4.29 0.6779 WVFGRD96 22.0 115 35 50 4.30 0.6744 WVFGRD96 23.0 115 35 50 4.31 0.6672 WVFGRD96 24.0 115 35 50 4.31 0.6545 WVFGRD96 25.0 110 35 45 4.32 0.6380 WVFGRD96 26.0 110 35 40 4.33 0.6201 WVFGRD96 27.0 110 35 40 4.34 0.6028 WVFGRD96 28.0 110 30 40 4.34 0.5883 WVFGRD96 29.0 110 30 40 4.35 0.5764
The best solution is
WVFGRD96 20.0 115 40 55 4.28 0.6784
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=Sun Nov 19 11:16:58 CST 2017