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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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: