2016/09/15 17:27:54 42.7632 13.0868 10.5 3.1
SLU Moment Tensor Solution
ENS 2016/09/15 17:27:54:0 42.76 13.09 10.5 3.1
Stations used:
IV.ATFO IV.ATTE IV.CAMP IV.CESI IV.CESX IV.CING IV.FDMO
IV.GIGS IV.GUMA IV.MGAB IV.MURB IV.PTQR IV.SNTG IV.SRES
IV.T1241 IV.T1242 IV.T1243 IV.TERO MN.AQU
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +40
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 5.07e+20 dyne-cm
Mw = 3.07
Z = 7 km
Plane Strike Dip Rake
NP1 43 76 -104
NP2 270 20 -45
Principal Axes:
Axis Value Plunge Azimuth
T 5.07e+20 30 145
N 0.00e+00 14 47
P -5.07e+20 57 294
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.30e+20
Mxy -1.23e+20
Mxz -2.75e+20
Myy -2.92e+12
Myz 3.37e+20
Mzz -2.30e+20
##############
######################
#######--------------#######
####----------------------###-
###---------------------------#---
##----------------------------####--
##----------------------------######--
##----------------------------########--
#---------- ---------------##########-
#----------- P -------------#############-
------------ ------------###############
-------------------------#################
-----------------------###################
--------------------####################
-------------------#####################
---------------#######################
------------############# ########
---------############### T #######
----################## #####
############################
######################
##############
Global CMT Convention Moment Tensor:
R T P
-2.30e+20 -2.75e+20 -3.37e+20
-2.75e+20 2.30e+20 1.23e+20
-3.37e+20 1.23e+20 -2.92e+12
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160915172754/index.html
|
STK = 270
DIP = 20
RAKE = -45
MW = 3.07
HS = 7.0
The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2016/09/15 17:27:54:0 42.76 13.09 10.5 3.1
Stations used:
IV.ATFO IV.ATTE IV.CAMP IV.CESI IV.CESX IV.CING IV.FDMO
IV.GIGS IV.GUMA IV.MGAB IV.MURB IV.PTQR IV.SNTG IV.SRES
IV.T1241 IV.T1242 IV.T1243 IV.TERO MN.AQU
Filtering commands used:
cut o DIST/3.3 -20 o DIST/3.3 +40
rtr
taper w 0.1
hp c 0.03 n 3
lp c 0.10 n 3
Best Fitting Double Couple
Mo = 5.07e+20 dyne-cm
Mw = 3.07
Z = 7 km
Plane Strike Dip Rake
NP1 43 76 -104
NP2 270 20 -45
Principal Axes:
Axis Value Plunge Azimuth
T 5.07e+20 30 145
N 0.00e+00 14 47
P -5.07e+20 57 294
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.30e+20
Mxy -1.23e+20
Mxz -2.75e+20
Myy -2.92e+12
Myz 3.37e+20
Mzz -2.30e+20
##############
######################
#######--------------#######
####----------------------###-
###---------------------------#---
##----------------------------####--
##----------------------------######--
##----------------------------########--
#---------- ---------------##########-
#----------- P -------------#############-
------------ ------------###############
-------------------------#################
-----------------------###################
--------------------####################
-------------------#####################
---------------#######################
------------############# ########
---------############### T #######
----################## #####
############################
######################
##############
Global CMT Convention Moment Tensor:
R T P
-2.30e+20 -2.75e+20 -3.37e+20
-2.75e+20 2.30e+20 1.23e+20
-3.37e+20 1.23e+20 -2.92e+12
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20160915172754/index.html
|
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.
|
|
|
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 +40 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 65 35 -80 2.85 0.4268
WVFGRD96 2.0 280 15 -35 3.00 0.4611
WVFGRD96 3.0 280 15 -35 2.98 0.5844
WVFGRD96 4.0 280 20 -40 2.97 0.6483
WVFGRD96 5.0 265 15 -50 3.07 0.6877
WVFGRD96 6.0 270 20 -50 3.07 0.7112
WVFGRD96 7.0 270 20 -45 3.07 0.7126
WVFGRD96 8.0 275 25 -45 3.03 0.7001
WVFGRD96 9.0 275 25 -45 3.03 0.6827
WVFGRD96 10.0 275 25 -45 3.04 0.6602
WVFGRD96 11.0 280 25 -40 3.04 0.6352
WVFGRD96 12.0 285 25 -35 3.04 0.6091
WVFGRD96 13.0 290 25 -30 3.04 0.5828
WVFGRD96 14.0 320 30 20 3.06 0.5618
WVFGRD96 15.0 320 25 15 3.10 0.5398
The best solution is
WVFGRD96 7.0 270 20 -45 3.07 0.7126
The mechanism correspond to the best fit is
|
|
|
The best fit as a function of depth is given in the following figure:
|
|
|
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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 n 3
|
|
|
|
| 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=Fri Sep 16 07:28:57 CDT 2016