2016/10/15 01:30:54 42.8918 13.256 9.4 3.0 Ascoli
USGS Felt map for this earthquake
SLU Moment Tensor Solution
ENS 2016/10/15 01:30:54:5 42.89 13.26 9.4 3.0 Ascoli
Stations used:
IV.ASSB IV.FIAM IV.GUMA IV.NRCA IV.OFFI IV.SNTG IV.TERO
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 = 6.03e+20 dyne-cm
Mw = 3.12
Z = 3 km
Plane Strike Dip Rake
NP1 145 60 -55
NP2 271 45 -135
Principal Axes:
Axis Value Plunge Azimuth
T 6.03e+20 9 211
N 0.00e+00 30 306
P -6.03e+20 59 106
Moment Tensor: (dyne-cm)
Component Value
Mxx 4.22e+20
Mxy 3.03e+20
Mxz -4.49e+13
Myy 5.57e+18
Myz -3.01e+20
Mzz -4.27e+20
##############
######################
--##########################
---###########################
-----#############################
------####----------------##########
-------------------------------#######
-----####--------------------------#####
--#######----------------------------###
--#########-----------------------------##
-###########-----------------------------#
#############-------------- ------------
##############------------- P ------------
##############------------ -----------
###############-------------------------
################----------------------
#################-------------------
##################----------------
### ############------------
## T ################-------
####################
##############
Global CMT Convention Moment Tensor:
R T P
-4.27e+20 -4.49e+13 3.01e+20
-4.49e+13 4.22e+20 -3.03e+20
3.01e+20 -3.03e+20 5.57e+18
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20161015013054/index.html
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STK = 145
DIP = 60
RAKE = -55
MW = 3.12
HS = 3.0
The NDK file is 20161015013054.ndk The waveform inversion is preferred.
The following compares this source inversion to others
SLU Moment Tensor Solution
ENS 2016/10/15 01:30:54:5 42.89 13.26 9.4 3.0 Ascoli
Stations used:
IV.ASSB IV.FIAM IV.GUMA IV.NRCA IV.OFFI IV.SNTG IV.TERO
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 = 6.03e+20 dyne-cm
Mw = 3.12
Z = 3 km
Plane Strike Dip Rake
NP1 145 60 -55
NP2 271 45 -135
Principal Axes:
Axis Value Plunge Azimuth
T 6.03e+20 9 211
N 0.00e+00 30 306
P -6.03e+20 59 106
Moment Tensor: (dyne-cm)
Component Value
Mxx 4.22e+20
Mxy 3.03e+20
Mxz -4.49e+13
Myy 5.57e+18
Myz -3.01e+20
Mzz -4.27e+20
##############
######################
--##########################
---###########################
-----#############################
------####----------------##########
-------------------------------#######
-----####--------------------------#####
--#######----------------------------###
--#########-----------------------------##
-###########-----------------------------#
#############-------------- ------------
##############------------- P ------------
##############------------ -----------
###############-------------------------
################----------------------
#################-------------------
##################----------------
### ############------------
## T ################-------
####################
##############
Global CMT Convention Moment Tensor:
R T P
-4.27e+20 -4.49e+13 3.01e+20
-4.49e+13 4.22e+20 -3.03e+20
3.01e+20 -3.03e+20 5.57e+18
Details of the solution is found at
http://www.eas.slu.edu/eqc/eqc_mt/MECH.IT/20161015013054/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.
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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 +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 1.0 150 65 -55 3.00 0.4013
WVFGRD96 2.0 145 65 -60 3.11 0.4584
WVFGRD96 3.0 145 60 -55 3.12 0.4827
WVFGRD96 4.0 135 55 -70 3.15 0.4693
WVFGRD96 5.0 135 55 -70 3.23 0.4787
WVFGRD96 6.0 60 60 10 3.26 0.4414
WVFGRD96 7.0 60 60 10 3.27 0.4347
WVFGRD96 8.0 60 65 5 3.26 0.4209
WVFGRD96 9.0 60 70 5 3.28 0.4114
WVFGRD96 10.0 60 70 5 3.30 0.4006
WVFGRD96 11.0 60 70 5 3.30 0.3890
WVFGRD96 12.0 60 70 5 3.31 0.3766
WVFGRD96 13.0 60 70 5 3.32 0.3651
WVFGRD96 14.0 60 70 5 3.33 0.3526
WVFGRD96 15.0 60 65 10 3.34 0.3449
WVFGRD96 16.0 60 65 10 3.34 0.3352
WVFGRD96 17.0 65 60 15 3.32 0.3279
WVFGRD96 18.0 345 80 35 3.25 0.3297
WVFGRD96 19.0 345 80 35 3.27 0.3341
WVFGRD96 20.0 345 75 35 3.29 0.3386
WVFGRD96 21.0 345 75 35 3.30 0.3433
WVFGRD96 22.0 345 75 40 3.31 0.3474
WVFGRD96 23.0 345 75 40 3.32 0.3533
WVFGRD96 24.0 340 75 40 3.35 0.3582
WVFGRD96 25.0 340 75 40 3.36 0.3658
WVFGRD96 26.0 340 75 40 3.37 0.3699
WVFGRD96 27.0 340 75 40 3.38 0.3736
WVFGRD96 28.0 340 75 40 3.39 0.3756
WVFGRD96 29.0 340 75 40 3.40 0.3764
The best solution is
WVFGRD96 3.0 145 60 -55 3.12 0.4827
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 +40 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.10 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.
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=Mon Oct 17 07:41:28 CDT 2016