USGS/SLU Moment Tensor Solution ENS 2018/07/04 11:24:20:7 41.51 19.53 10.0 4.3 Albania Stations used: CL.AGRP CL.MALA CL.ROD3 CL.TRIZ HU.KOVH HU.MORH KO.GADA RO.BAIL RO.BANR RO.BZS RO.COPA RO.DEV RO.GZR RO.HERR RO.LOT RO.MDVR RO.PUNG RO.SIRR RO.VLAD SJ.BBLS Filtering commands used: cut o DIST/3.3 -30 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 = 5.56e+22 dyne-cm Mw = 4.43 Z = 25 km Plane Strike Dip Rake NP1 131 62 112 NP2 270 35 55 Principal Axes: Axis Value Plunge Azimuth T 5.56e+22 66 80 N 0.00e+00 19 300 P -5.56e+22 14 205 Moment Tensor: (dyne-cm) Component Value Mxx -4.28e+22 Mxy -1.83e+22 Mxz 1.56e+22 Myy -4.36e+14 Myz 2.61e+22 Mzz 4.28e+22 -------------- ---------------------- ---------------------------- ------------------------------ #-------##################-------- ###---########################------ ##################################---- ###---###############################--- ##-----###############################-- #--------################ #############- #---------############### T #############- ------------############# ############## --------------############################ --------------########################## -----------------####################### ------------------#################### --------------------################ -----------------------########### ------ --------------------- ----- P -------------------- -- ----------------- -------------- Global CMT Convention Moment Tensor: R T P 4.28e+22 1.56e+22 -2.61e+22 1.56e+22 -4.28e+22 1.83e+22 -2.61e+22 1.83e+22 -4.36e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180704112420/index.html |
STK = 270 DIP = 35 RAKE = 55 MW = 4.43 HS = 25.0
The NDK file is 20180704112420.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2018/07/04 11:24:20:7 41.51 19.53 10.0 4.3 Albania Stations used: CL.AGRP CL.MALA CL.ROD3 CL.TRIZ HU.KOVH HU.MORH KO.GADA RO.BAIL RO.BANR RO.BZS RO.COPA RO.DEV RO.GZR RO.HERR RO.LOT RO.MDVR RO.PUNG RO.SIRR RO.VLAD SJ.BBLS Filtering commands used: cut o DIST/3.3 -30 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 = 5.56e+22 dyne-cm Mw = 4.43 Z = 25 km Plane Strike Dip Rake NP1 131 62 112 NP2 270 35 55 Principal Axes: Axis Value Plunge Azimuth T 5.56e+22 66 80 N 0.00e+00 19 300 P -5.56e+22 14 205 Moment Tensor: (dyne-cm) Component Value Mxx -4.28e+22 Mxy -1.83e+22 Mxz 1.56e+22 Myy -4.36e+14 Myz 2.61e+22 Mzz 4.28e+22 -------------- ---------------------- ---------------------------- ------------------------------ #-------##################-------- ###---########################------ ##################################---- ###---###############################--- ##-----###############################-- #--------################ #############- #---------############### T #############- ------------############# ############## --------------############################ --------------########################## -----------------####################### ------------------#################### --------------------################ -----------------------########### ------ --------------------- ----- P -------------------- -- ----------------- -------------- Global CMT Convention Moment Tensor: R T P 4.28e+22 1.56e+22 -2.61e+22 1.56e+22 -4.28e+22 1.83e+22 -2.61e+22 1.83e+22 -4.36e+14 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20180704112420/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 -30 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 1.0 115 40 -90 4.10 0.4347 WVFGRD96 2.0 115 35 -90 4.18 0.4843 WVFGRD96 3.0 285 50 -90 4.26 0.5128 WVFGRD96 4.0 285 50 -85 4.30 0.4595 WVFGRD96 5.0 305 70 -55 4.29 0.3824 WVFGRD96 6.0 305 80 -50 4.28 0.3784 WVFGRD96 7.0 135 90 50 4.27 0.3940 WVFGRD96 8.0 310 85 -60 4.33 0.4141 WVFGRD96 9.0 135 90 60 4.33 0.4361 WVFGRD96 10.0 310 90 -60 4.32 0.4572 WVFGRD96 11.0 135 85 55 4.34 0.4771 WVFGRD96 12.0 135 80 55 4.35 0.4962 WVFGRD96 13.0 140 75 55 4.36 0.5133 WVFGRD96 14.0 145 70 60 4.38 0.5305 WVFGRD96 15.0 150 65 65 4.40 0.5466 WVFGRD96 16.0 150 65 70 4.41 0.5617 WVFGRD96 17.0 150 65 70 4.41 0.5746 WVFGRD96 18.0 150 65 70 4.42 0.5849 WVFGRD96 19.0 150 60 70 4.43 0.5933 WVFGRD96 20.0 155 60 75 4.44 0.5999 WVFGRD96 21.0 275 35 60 4.41 0.6066 WVFGRD96 22.0 275 35 60 4.41 0.6138 WVFGRD96 23.0 275 35 60 4.42 0.6181 WVFGRD96 24.0 275 35 60 4.42 0.6199 WVFGRD96 25.0 270 35 55 4.43 0.6201 WVFGRD96 26.0 260 40 50 4.44 0.6194 WVFGRD96 27.0 260 40 45 4.45 0.6178 WVFGRD96 28.0 260 40 45 4.45 0.6153 WVFGRD96 29.0 260 40 45 4.46 0.6115
The best solution is
WVFGRD96 25.0 270 35 55 4.43 0.6201
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 0.02 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:
Here we tabulate the reasons for not using certain digital data sets
The following stations did not have a valid response files: