USGS/SLU Moment Tensor Solution ENS 2018/07/04 09:01:08:7 41.49 19.53 10.0 4.9 Albania Stations used: BS.ELND CL.AGRP CL.MALA CL.MG05 CL.ROD3 CL.TRIZ HA.AXAR HA.KALE HA.LOUT HA.MAKR HA.VILL HL.EVR HL.JAN HL.KLV HL.KYMI HL.LIA HL.LKR HL.NEO HL.NVR HL.PENT HL.PLG HL.RDO HL.RLS HL.SKY HL.SMTH HL.VLS HP.AMT HP.ANX HP.GUR HP.LTHK HT.AGG HT.ALN HT.EVGI HT.FNA HT.HORT HT.IGT HT.KAVA HT.KOKK HT.KPRO HT.LKD2 HT.LRSO HT.NEST HT.NYDR HT.OUR HT.PSDA HT.SOH HT.SRS HT.THAS HT.THE HU.KOVH HU.MORH ME.KOME MN.BZS MN.PDG RO.BAIL RO.BANR RO.COPA RO.DEV RO.GZR RO.HERR RO.HUMR RO.LOT RO.MDVR RO.SIRR RO.VLAD SJ.BBLS SJ.FRGS Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 6.03e+23 dyne-cm Mw = 5.12 Z = 25 km Plane Strike Dip Rake NP1 155 75 90 NP2 335 15 90 Principal Axes: Axis Value Plunge Azimuth T 6.03e+23 60 65 N 0.00e+00 -0 155 P -6.03e+23 30 245 Moment Tensor: (dyne-cm) Component Value Mxx -5.38e+22 Mxy -1.15e+23 Mxz 2.21e+23 Myy -2.47e+23 Myz 4.73e+23 Mzz 3.01e+23 -#######------ --###############----- -----###################---- -------####################--- ---------#####################---- ----------#######################--- ------------#######################--- -------------########################--- --------------########### #########--- ----------------########## T ##########--- ----------------########## ##########--- -----------------######################--- ------------------#####################--- ----- ----------####################-- ----- P -----------###################-- ---- ------------#################-- -------------------###############-- --------------------############-- -------------------##########- -------------------########- ------------------#### -------------- Global CMT Convention Moment Tensor: R T P 3.01e+23 2.21e+23 -4.73e+23 2.21e+23 -5.38e+22 1.15e+23 -4.73e+23 1.15e+23 -2.47e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180704090108/index.html |
STK = 155 DIP = 75 RAKE = 90 MW = 5.12 HS = 25.0
The NDK file is 20180704090108.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2018/07/04 09:01:08:7 41.49 19.53 10.0 4.9 Albania Stations used: BS.ELND CL.AGRP CL.MALA CL.MG05 CL.ROD3 CL.TRIZ HA.AXAR HA.KALE HA.LOUT HA.MAKR HA.VILL HL.EVR HL.JAN HL.KLV HL.KYMI HL.LIA HL.LKR HL.NEO HL.NVR HL.PENT HL.PLG HL.RDO HL.RLS HL.SKY HL.SMTH HL.VLS HP.AMT HP.ANX HP.GUR HP.LTHK HT.AGG HT.ALN HT.EVGI HT.FNA HT.HORT HT.IGT HT.KAVA HT.KOKK HT.KPRO HT.LKD2 HT.LRSO HT.NEST HT.NYDR HT.OUR HT.PSDA HT.SOH HT.SRS HT.THAS HT.THE HU.KOVH HU.MORH ME.KOME MN.BZS MN.PDG RO.BAIL RO.BANR RO.COPA RO.DEV RO.GZR RO.HERR RO.HUMR RO.LOT RO.MDVR RO.SIRR RO.VLAD SJ.BBLS SJ.FRGS Filtering commands used: cut o DIST/3.3 -20 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 6.03e+23 dyne-cm Mw = 5.12 Z = 25 km Plane Strike Dip Rake NP1 155 75 90 NP2 335 15 90 Principal Axes: Axis Value Plunge Azimuth T 6.03e+23 60 65 N 0.00e+00 -0 155 P -6.03e+23 30 245 Moment Tensor: (dyne-cm) Component Value Mxx -5.38e+22 Mxy -1.15e+23 Mxz 2.21e+23 Myy -2.47e+23 Myz 4.73e+23 Mzz 3.01e+23 -#######------ --###############----- -----###################---- -------####################--- ---------#####################---- ----------#######################--- ------------#######################--- -------------########################--- --------------########### #########--- ----------------########## T ##########--- ----------------########## ##########--- -----------------######################--- ------------------#####################--- ----- ----------####################-- ----- P -----------###################-- ---- ------------#################-- -------------------###############-- --------------------############-- -------------------##########- -------------------########- ------------------#### -------------- Global CMT Convention Moment Tensor: R T P 3.01e+23 2.21e+23 -4.73e+23 2.21e+23 -5.38e+22 1.15e+23 -4.73e+23 1.15e+23 -2.47e+23 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180704090108/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 -20 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.06 n 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 170 45 -90 4.74 0.2440 WVFGRD96 2.0 170 45 -90 4.83 0.2917 WVFGRD96 3.0 170 45 -90 4.86 0.2635 WVFGRD96 4.0 295 55 -35 4.76 0.2291 WVFGRD96 5.0 295 55 -30 4.78 0.2340 WVFGRD96 6.0 295 60 -25 4.79 0.2393 WVFGRD96 7.0 155 80 85 4.88 0.2644 WVFGRD96 8.0 155 80 85 4.96 0.2869 WVFGRD96 9.0 155 80 85 4.97 0.3202 WVFGRD96 10.0 155 75 85 4.99 0.3488 WVFGRD96 11.0 155 75 85 5.00 0.3755 WVFGRD96 12.0 350 15 105 5.00 0.3983 WVFGRD96 13.0 155 75 85 5.01 0.4183 WVFGRD96 14.0 155 75 85 5.02 0.4354 WVFGRD96 15.0 155 70 85 5.03 0.4509 WVFGRD96 16.0 155 70 85 5.04 0.4643 WVFGRD96 17.0 155 70 85 5.05 0.4756 WVFGRD96 18.0 155 70 85 5.05 0.4850 WVFGRD96 19.0 155 70 85 5.06 0.4926 WVFGRD96 20.0 155 70 85 5.07 0.4987 WVFGRD96 21.0 155 70 85 5.08 0.5042 WVFGRD96 22.0 155 70 85 5.09 0.5074 WVFGRD96 23.0 155 70 85 5.10 0.5095 WVFGRD96 24.0 155 75 90 5.11 0.5112 WVFGRD96 25.0 155 75 90 5.12 0.5121 WVFGRD96 26.0 155 75 90 5.12 0.5119 WVFGRD96 27.0 155 75 90 5.13 0.5108 WVFGRD96 28.0 150 75 85 5.14 0.5088 WVFGRD96 29.0 150 75 85 5.14 0.5059
The best solution is
WVFGRD96 25.0 155 75 90 5.12 0.5121
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 +70 rtr taper w 0.1 hp c 0.02 n 3 lp c 0.06 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 .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: