USGS/SLU Moment Tensor Solution ENS 2018/07/17 13:05:08:4 41.09 19.69 10.0 4.6 Albania Stations used: CL.MALA CL.MG05 CL.MG07 HL.EVR HL.JAN HL.KLV HL.KYMI HL.LIA HL.NEO HL.NVR HL.PLG HL.SMTH HL.THL HL.VLS HL.VLY HP.AMT HP.ANX HP.GUR HP.PVO HT.AGG HT.ALN HT.AOS2 HT.IGT HT.KAVA HT.KOKK HT.KRND HT.NEST HT.OUR HT.SIGR HT.SOH HT.THAS HU.KOVH HU.MORH ME.KOME RO.BZS RO.GZR SJ.FRGS Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 2.11e+22 dyne-cm Mw = 4.15 Z = 27 km Plane Strike Dip Rake NP1 152 73 132 NP2 260 45 25 Principal Axes: Axis Value Plunge Azimuth T 2.11e+22 45 104 N 0.00e+00 40 317 P -2.11e+22 17 212 Moment Tensor: (dyne-cm) Component Value Mxx -1.33e+22 Mxy -1.12e+22 Mxz 2.35e+21 Myy 4.36e+21 Myz 1.33e+22 Mzz 8.93e+21 -------------- #--------------------- ####------------------------ #####------------------------- ########-------------------------- #########---#################------- #########--#######################---- #######-----##########################-- #####--------########################### ####-----------########################### ###-------------########################## ##--------------############## ######### #----------------############# T ######### ------------------########### ######## -------------------##################### -------------------################### -------------------################# --------------------############## ---- ------------########### --- P --------------######## -----------------## -------------- Global CMT Convention Moment Tensor: R T P 8.93e+21 2.35e+21 -1.33e+22 2.35e+21 -1.33e+22 1.12e+22 -1.33e+22 1.12e+22 4.36e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180717130508/index.html |
STK = 260 DIP = 45 RAKE = 25 MW = 4.15 HS = 27.0
The NDK file is 20180717130508.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2018/07/17 13:05:08:4 41.09 19.69 10.0 4.6 Albania Stations used: CL.MALA CL.MG05 CL.MG07 HL.EVR HL.JAN HL.KLV HL.KYMI HL.LIA HL.NEO HL.NVR HL.PLG HL.SMTH HL.THL HL.VLS HL.VLY HP.AMT HP.ANX HP.GUR HP.PVO HT.AGG HT.ALN HT.AOS2 HT.IGT HT.KAVA HT.KOKK HT.KRND HT.NEST HT.OUR HT.SIGR HT.SOH HT.THAS HU.KOVH HU.MORH ME.KOME RO.BZS RO.GZR SJ.FRGS Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 Best Fitting Double Couple Mo = 2.11e+22 dyne-cm Mw = 4.15 Z = 27 km Plane Strike Dip Rake NP1 152 73 132 NP2 260 45 25 Principal Axes: Axis Value Plunge Azimuth T 2.11e+22 45 104 N 0.00e+00 40 317 P -2.11e+22 17 212 Moment Tensor: (dyne-cm) Component Value Mxx -1.33e+22 Mxy -1.12e+22 Mxz 2.35e+21 Myy 4.36e+21 Myz 1.33e+22 Mzz 8.93e+21 -------------- #--------------------- ####------------------------ #####------------------------- ########-------------------------- #########---#################------- #########--#######################---- #######-----##########################-- #####--------########################### ####-----------########################### ###-------------########################## ##--------------############## ######### #----------------############# T ######### ------------------########### ######## -------------------##################### -------------------################### -------------------################# --------------------############## ---- ------------########### --- P --------------######## -----------------## -------------- Global CMT Convention Moment Tensor: R T P 8.93e+21 2.35e+21 -1.33e+22 2.35e+21 -1.33e+22 1.12e+22 -1.33e+22 1.12e+22 4.36e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180717130508/index.html |
(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.
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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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 185 40 80 3.57 0.1284 WVFGRD96 2.0 190 45 -95 3.68 0.1660 WVFGRD96 3.0 200 40 -85 3.76 0.1882 WVFGRD96 4.0 10 50 -100 3.78 0.1779 WVFGRD96 5.0 320 60 -20 3.68 0.1771 WVFGRD96 6.0 320 65 -25 3.71 0.1868 WVFGRD96 7.0 320 65 -20 3.73 0.1965 WVFGRD96 8.0 315 60 -30 3.79 0.2046 WVFGRD96 9.0 295 55 -20 3.84 0.2129 WVFGRD96 10.0 255 40 15 3.87 0.2224 WVFGRD96 11.0 255 40 15 3.89 0.2342 WVFGRD96 12.0 255 45 20 3.90 0.2458 WVFGRD96 13.0 255 50 25 3.92 0.2591 WVFGRD96 14.0 255 50 25 3.94 0.2733 WVFGRD96 15.0 255 50 25 3.96 0.2869 WVFGRD96 16.0 255 55 25 3.97 0.2999 WVFGRD96 17.0 255 55 25 3.99 0.3118 WVFGRD96 18.0 255 55 25 4.01 0.3226 WVFGRD96 19.0 255 55 25 4.02 0.3326 WVFGRD96 20.0 255 55 25 4.04 0.3414 WVFGRD96 21.0 255 50 25 4.06 0.3485 WVFGRD96 22.0 255 50 25 4.08 0.3550 WVFGRD96 23.0 255 50 25 4.09 0.3598 WVFGRD96 24.0 255 50 25 4.10 0.3636 WVFGRD96 25.0 255 50 20 4.12 0.3663 WVFGRD96 26.0 260 45 25 4.14 0.3683 WVFGRD96 27.0 260 45 25 4.15 0.3692 WVFGRD96 28.0 260 45 25 4.16 0.3691 WVFGRD96 29.0 260 45 25 4.17 0.3682 WVFGRD96 30.0 260 40 20 4.19 0.3663 WVFGRD96 31.0 260 40 20 4.20 0.3647 WVFGRD96 32.0 260 40 20 4.20 0.3621 WVFGRD96 33.0 260 40 20 4.21 0.3597 WVFGRD96 34.0 260 40 20 4.22 0.3566 WVFGRD96 35.0 260 40 20 4.23 0.3531 WVFGRD96 36.0 260 40 20 4.24 0.3495 WVFGRD96 37.0 260 40 15 4.24 0.3454 WVFGRD96 38.0 260 40 15 4.25 0.3408 WVFGRD96 39.0 260 40 20 4.26 0.3353 WVFGRD96 40.0 295 15 65 4.42 0.3305 WVFGRD96 41.0 295 15 65 4.43 0.3256 WVFGRD96 42.0 285 20 55 4.43 0.3199 WVFGRD96 43.0 285 20 55 4.44 0.3138 WVFGRD96 44.0 285 20 55 4.45 0.3072 WVFGRD96 45.0 285 20 60 4.46 0.3006 WVFGRD96 46.0 285 20 60 4.47 0.2938 WVFGRD96 47.0 280 20 55 4.48 0.2867 WVFGRD96 48.0 280 20 55 4.49 0.2794 WVFGRD96 49.0 275 25 50 4.48 0.2719
The best solution is
WVFGRD96 27.0 260 45 25 4.15 0.3692
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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 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.
Thanks also to the many seismic network operators whose dedication make this effort possible: University of Nevada Reno, University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureas of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Iris stations and the Transportable Array of EarthScope.
The WUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
MODEL.01 Model after 8 iterations 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 1.9000 3.4065 2.0089 2.2150 0.302E-02 0.679E-02 0.00 0.00 1.00 1.00 6.1000 5.5445 3.2953 2.6089 0.349E-02 0.784E-02 0.00 0.00 1.00 1.00 13.0000 6.2708 3.7396 2.7812 0.212E-02 0.476E-02 0.00 0.00 1.00 1.00 19.0000 6.4075 3.7680 2.8223 0.111E-02 0.249E-02 0.00 0.00 1.00 1.00 0.0000 7.9000 4.6200 3.2760 0.164E-10 0.370E-10 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: