Location of the earthquake (yellow star) and great circle path from the epicenter to each station (red) [created using GMT (Wessel, P., and W. H. F. Smith, New version of Generic Mapping Tools released, EOS Trans. AGU, 76 329, 1995.)]
2006/10/15 17:07:49 19.88 -155.93 39
The following compares this source inversion to the USGS Rapid Moment Tensor Solution and to the Harvard CMT solutions, if they are available.
SLU Moment Tensor Solution
2006/10/15 17:07:49
Best Fitting Double Couple
Mo = 7.85e+25 dyne-cm
Mw = 6.53
Z = 5 km
Plane Strike Dip Rake
NP1 350 90 40
NP2 260 50 180
Principal Axes:
Axis Value Plunge Azimuth
T 7.85e+25 27 223
N 0.00e+00 50 350
P -7.85e+25 27 117
Moment Tensor: (dyne-cm)
Component Value
Mxx 2.06e+25
Mxy 5.65e+25
Mxz -8.76e+24
Myy -2.06e+25
Myz -4.97e+25
Mzz 1.23e+18
----##########
--------##############
-----------#################
-------------#################
---------------###################
----------------##-------###########
------------######---------------#####
---------##########------------------###
------#############--------------------#
-----################---------------------
---##################---------------------
--###################---------------------
-####################---------------------
#####################----------- -----
#####################----------- P -----
####################----------- ----
####### ##########----------------
###### T ##########---------------
#### ##########-------------
#################-----------
##############--------
##########----
Harvard Convention
Moment Tensor:
R T F
1.23e+18 -8.76e+24 4.97e+25
-8.76e+24 2.06e+25 -5.65e+25
4.97e+25 -5.65e+25 -2.06e+25
|
06/10/15 17:07:48.37
HAWAII REGION, HAWAII
Epicenter: 19.842 -156.059
MW 6.6
USGS MOMENT TENSOR SOLUTION
Depth 27 No. of sta: 76
Moment Tensor; Scale 10**19 Nm
Mrr=-0.32 Mtt= 0.10
Mpp= 0.22 Mrt=-0.16
Mrp=-0.46 Mtp=-1.01
Principal axes:
T Val= 1.21 Plg= 9 Azm= 49
N -0.11 59 153
P -1.10 30 313
Best Double Couple:Mo=1.2*10**19
NP1:Strike= 95 Dip=63 Slip=-164
NP2: 358 76 -28
---####
---------########
-----------##########
--------------########
----- --------######## T ##
------ P --------######## ###
------ ---------#############
-------------------##############
-------------------##############
#------------------##############
####---------------##############
#########----------##########----
##################-------------
##################-------------
#################------------
###############----------
############---------
##########-------
####---
|
October 15, 2006, HAWAII REGION, HAWAII, MW=6.7
Meredith Nettles
CENTROID, MOMENT TENSOR SOLUTION
HARVARD EVENT-FILE NAME C101506A
DATA USED: GSN
L.P. BODY WAVES: 73S,206C, T= 50
MANTLE WAVES: 69S,165C, T=125
CENTROID LOCATION:
ORIGIN TIME 17:07:54.2 0.1
LAT 19.85N 0.01;LON 155.81W 0.01
DEP 33.7 0.6;HALF-DURATION 5.5
MOMENT TENSOR; SCALE 10**26 D-CM
MRR=-0.63 0.01; MTT= 0.72 0.01
MPP=-0.09 0.01; MRT= 0.11 0.01
MRP=-0.85 0.02; MTP=-0.73 0.01
PRINCIPAL AXES:
1.(T) VAL= 1.31;PLG=17;AZM= 37
2.(N) 0.00; 36; 140
3.(P) -1.31; 49; 286
BEST DOUBLE COUPLE:M0=1.3*10**26
NP1:STRIKE= 87;DIP=42;SLIP=-151
NP2:STRIKE=334;DIP=71;SLIP= -52
###########
----############
--------########## T ##
------------######## ####
--------------###############
----------------###############
------ --------##############
------- P ---------##############
------- ----------#############
---------------------###########-
#---------------------#########--
##-------------------#######---
####------------------####-----
#######----------------------
#####################------
###################----
#################--
###########
|
The following broadband stations passed the QC and were used for the source inversion. AAM ACSO AGMN AHID ANMO BBSR BILL BINY BLA BRAL BW06 CBKS CBN CCM CMB COLA COR CTAO DGMT DUG DWPF ECSD EGAK EGMT ERM EYMN GUMO HAWA HDIL HKT HLID HNR HRV HUMO HWUT INCN ISCO JCT JFWS KBS KEV KSU1 KVTX LAO LOHW LONY LVC MA2 MAJO MBWA MCWV MIAR MNTX MOOW MSO MVCO NATX NCB NEW NLWA NNA OTAV OXF PAYG PET PFO PKME RAO RPN RRI2 RSSD SAO SCIA SDV SFJD SJG SNOW SNZO SSPA TATO TAU TEIG TPAW TUC TZTN WMOK WRAK WUAZ WVOR WVT YAK YSS
All observed and Greens function waveforms are corrected to instrument response to ground velocity in meters/sec for the passband of 0.004 - 5 Hz. The traces were then lowpass filtered at 0.25 Hz and interpolated to a sample rate of 1 second.
For the deviatoric moment tensor inversion, the observed traces and Green's functions are read in an cut using the following commands
#####
# Driver script for the teleseismic waveform inversion
#
# The depth HS must be of the form 0010 for a depth of 1.0 km
# of 6700 for a depth of 670.0 km
#
# The Filter_Band is an integer with the following meansing
#
# FILTER_BAND 1/FH 1/FL
# 1 60 12 for Mw < 6.4
# 2 100 20 6.4 =< Mw < 6.8
# 3 120 40 6.8 =< Mw < 7.2
# 4 143 80 7.2 =< Mw < 9.3
#####
# Source duration - halfwidth of triangular function
# this filters only the Green functions
#
# halfwidth = 1.05 * 10-8 * M0^1/3 (M0 is dyne-cm)
#
# MW half-width (sec)
# 5.0 0.75
# 6.0 2.45
# 7.0 7.7
# 8.0 24.5
# 9.0 74.3
# 0.5*(MW - 9)
# or half-width=74.3*10
# or echo 6.62 | awk '{print 74.3*exp(0.5*log(10.0)*(0050 - 9.0)) }'
#####
# Processing window for P (use SAC variable A for P arrival
# Start A - 30
# End A + 2*HALFWIDTH + 0.03*HS + 30 + 1/FH
# Processing window for SH (use SAC variable T0 for SH arrival
# Start T0 - 60
# End T0 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
# Processing window for SV (use SAC variable T1 for SV arrival
# Start T1 - 60
# End T1 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
#
# The term involving HS serves to include the depth phases and
# to exclude the PP or SS at most distanace
#####
The cut windows attempt to include the P, pP, sP, pS, S and sS arrivals. However, oen must be very careful about the fact that PP may be included in some distance ranges.
The waveforms are then bandpass filtered by the application of the following high- and low-pass stages (an optional microseism filter):
hp c 0.0100 2 lp c 0.0500 2 int br c 0.12 0.25 n 4 p 2The traces were next integrated to ground displacment in meters. Finally the observed data are interpolated to ahve the same sampling at the Green's functions.
The source inversion is a multipass operation since a lower frequency filter band is used for larger earthquakes and since a search is made over depth. Up to three passed of the outer loop are made, after which the moment magnitude is determined and filter settings readjusted. The inner loop over depth samples all depths from 0 to 800 km with 5 km increments in depth to 50 km, followed by 10 km depth sampling for the remaining range.
The following filter ranges are used according to the moment magnitude Mw:
FILTER_BAND 1/FH(s) 1/FL(s)
1 60 12 Mw < 6.4
2 100 20 6.4 < Mw <= 6.9
3 120 40 Mw > 6.9
The map displays the distribution of stations used for this source inversion.
|
Location of the earthquake (yellow star) and great circle path from the epicenter to each station (red) [created using GMT (Wessel, P., and W. H. F. Smith, New version of Generic Mapping Tools released, EOS Trans. AGU, 76 329, 1995.)] |
For this data set the favored solution is
WVFMTD96 5.0 170. 89. 81. 6.70 0.372 0.766E-05 0.365 0.630 0.349E-05 13.5
The following figures show the sensitivity of the goodness of fit parameter so source depth, the waveform comparison as a function of epicentral distance in degrees and the source to station azimuth
|
| Goodness of fit as a function of source depth. The measure is 1 - SUM (o -p)2 / SUM o2. A value of 1.0 is the best fit. The best double couple mechanism for the solution depth is plotted above goodness of fit value to indicate how the mefhanism may change with depth. |
| P-wave Z component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
| SH-wave T component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
| SV-wave R component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
All observed and Greens function waveforms are corrected to instrument response to ground velocity in meters/sec for the passband of 0.004 - 5 Hz. The traces were then lowpass filtered at 0.25 Hz and interpolated to a sample rate of 1 second.
For the deviatoric moment tensor inversion, the observed traces and Green's functions are read in an cut using the following commands
#####
# Driver script for the teleseismic waveform inversion
#
# The depth HS must be of the form 0010 for a depth of 1.0 km
# of 6700 for a depth of 670.0 km
#
# The Filter_Band is an integer with the following meansing
#
# FILTER_BAND 1/FH 1/FL
# 1 60 12 for Mw < 6.4
# 2 100 20 6.4 =< Mw < 6.8
# 3 120 40 6.8 =< Mw < 7.2
# 4 143 80 7.2 =< Mw < 9.3
#####
# Source duration - halfwidth of triangular function
# this filters only the Green functions
#
# halfwidth = 1.05 * 10-8 * M0^1/3 (M0 is dyne-cm)
#
# MW half-width (sec)
# 5.0 0.75
# 6.0 2.45
# 7.0 7.7
# 8.0 24.5
# 9.0 74.3
# 0.5*(MW - 9)
# or half-width=74.3*10
# or echo 6.47 | awk '{print 74.3*exp(0.5*log(10.0)*(0300 - 9.0)) }'
#####
# Processing window for P (use SAC variable A for P arrival
# Start A - 30
# End A + 2*HALFWIDTH + 0.03*HS + 30 + 1/FH
# Processing window for SH (use SAC variable T0 for SH arrival
# Start T0 - 60
# End T0 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
# Processing window for SV (use SAC variable T1 for SV arrival
# Start T1 - 60
# End T1 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
#
# The term involving HS serves to include the depth phases and
# to exclude the PP or SS at most distanace
#####
The cut windows attempt to include the P, pP, sP, pS, S and sS arrivals. However, oen must be very careful about the fact that PP may be included in some distance ranges.
The waveforms are then bandpass filtered by the application of the following high- and low-pass stages (an optional microseism filter):
hp c 0.0100 2 lp c 0.0500 2 int br c 0.12 0.25 n 4 p 2The traces were next integrated to ground displacment in meters. Finally the observed data are interpolated to ahve the same sampling at the Green's functions.
The source inversion is a multipass operation since a lower frequency filter band is used for larger earthquakes and since a search is made over depth. Up to three passed of the outer loop are made, after which the moment magnitude is determined and filter settings readjusted. The inner loop over depth samples all depths from 0 to 800 km with 5 km increments in depth to 50 km, followed by 10 km depth sampling for the remaining range.
The following filter ranges are used according to the moment magnitude Mw:
FILTER_BAND 1/FH(s) 1/FL(s)
1 60 12 Mw < 6.4
2 100 20 6.4 < Mw <= 6.9
3 120 40 Mw > 6.9
The map displays the distribution of stations used for this source inversion.
Location of the earthquake (yellow star) and great circle path from the epicenter to each station (red) [created using GMT (Wessel, P., and W. H. F. Smith, New version of Generic Mapping Tools released, EOS Trans. AGU, 76 329, 1995.)] |
For this data set the favored solution is
WVFMTD96 30.0 343. 68. -47. 6.47 0.498 0.990E-06 0.500 0.705 0.945E-06 28.1
The following figures show the sensitivity of the goodness of fit parameter so source depth, the waveform comparison as a function of epicentral distance in degrees and the source to station azimuth
|
|
| Goodness of fit as a function of source depth. The measure is 1 - SUM (o -p)2 / SUM o2. A value of 1.0 is the best fit. The best double couple mechanism for the solution depth is plotted above goodness of fit value to indicate how the mefhanism may change with depth. |
| P-wave Z component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
All observed and Greens function waveforms are corrected to instrument response to ground velocity in meters/sec for the passband of 0.004 - 5 Hz. The traces were then lowpass filtered at 0.25 Hz and interpolated to a sample rate of 1 second.
For the grid search, the observed traces and Green's functions are read in an cut using the following commands
#####
# Driver script for the teleseismic waveform inversion
#
# The depth HS must be of the form 0010 for a depth of 1.0 km
# of 6700 for a depth of 670.0 km
#
# The Filter_Band is an integer with the following meansing
#
# FILTER_BAND 1/FH 1/FL
# 1 60 12 for Mw < 6.4
# 2 100 20 6.4 =< Mw < 6.8
# 3 120 40 6.8 =< Mw < 7.2
# 4 143 80 7.2 =< Mw < 9.3
#####
# Source duration - halfwidth of triangular function
# this filters only the Green functions
#
# halfwidth = 1.05 * 10-8 * M0^1/3 (M0 is dyne-cm)
#
# MW half-width (sec)
# 5.0 0.75
# 6.0 2.45
# 7.0 7.7
# 8.0 24.5
# 9.0 74.3
# 0.5*(MW - 9)
# or half-width=74.3*10
# or echo 6.53 | awk '{print 74.3*exp(0.5*log(10.0)*(0050 - 9.0)) }'
#####
# Processing window for P (use SAC variable A for P arrival
# Start A - 30
# End A + 2*HALFWIDTH + 0.03*HS + 30 + 1/FH
# Processing window for SH (use SAC variable T0 for SH arrival
# Start T0 - 60
# End T0 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
# Processing window for SV (use SAC variable T1 for SV arrival
# Start T1 - 60
# End T1 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
#
# The term involving HS serves to include the depth phases and
# to exclude the PP or SS at most distanace
#####
The cut windows attempt to include the P, pP, sP, pS, S and sS arrivals. However, oen must be very careful about the fact that PP may be included in some distance ranges.
The waveforms are then bandpass filtered by the application of the following high- and low-pass stages (an optional microseism filter):
hp c 0.0100 2 lp c 0.0500 2 int br c 0.12 0.25 n 4 p 2The traces were next integrated to ground displacment in meters. Finally the observed data are interpolated to ahve the same sampling at the Green's functions.
The source inversion is a multipass operation since a lower frequency filter band is used for larger earthquakes and since a search is made over depth. Up to three passed of the outer loop are made, after which the moment magnitude is determined and filter settings readjusted. The inner loop over depth samples all depths from 0 to 800 km with 5 km increments in depth to 50 km, followed by 10 km depth sampling for the remaining range.
The following filter ranges are used according to the moment magnitude Mw:
FILTER_BAND 1/FH(s) 1/FL(s)
1 60 12 Mw < 6.4
2 100 20 6.4 < Mw <= 6.9
3 120 40 Mw > 6.9
The map displays the distribution of stations used for this source inversion.
Location of the earthquake (yellow star) and great circle path from the epicenter to each station (red) [created using GMT (Wessel, P., and W. H. F. Smith, New version of Generic Mapping Tools released, EOS Trans. AGU, 76 329, 1995.)] |
For this data set the favored solution is
WVFGRD96 5.0 350 90 40 6.53 0.4546
The following figures show the sensitivity of the goodness of fit parameter so source depth, the waveform comparison as a function of epicentral distance in degrees and the source to station azimuth
|
| Goodness of fit as a function of source depth. The measure is 1 - SUM (o -p)2 / SUM o2. A value of 1.0 is the best fit. The best double couple mechanism for the solution depth is plotted above goodness of fit value to indicate how the mefhanism may change with depth. |
| P-wave Z component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
| SH-wave T component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
| SV-wave R component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
All observed and Greens function waveforms are corrected to instrument response to ground velocity in meters/sec for the passband of 0.004 - 5 Hz. The traces were then lowpass filtered at 0.25 Hz and interpolated to a sample rate of 1 second.
For the grid search, the observed traces and Green's functions are read in an cut using the following commands
#####
# Driver script for the teleseismic waveform inversion
#
# The depth HS must be of the form 0010 for a depth of 1.0 km
# of 6700 for a depth of 670.0 km
#
# The Filter_Band is an integer with the following meansing
#
# FILTER_BAND 1/FH 1/FL
# 1 60 12 for Mw < 6.4
# 2 100 20 6.4 =< Mw < 6.8
# 3 120 40 6.8 =< Mw < 7.2
# 4 143 80 7.2 =< Mw < 9.3
#####
# Source duration - halfwidth of triangular function
# this filters only the Green functions
#
# halfwidth = 1.05 * 10-8 * M0^1/3 (M0 is dyne-cm)
#
# MW half-width (sec)
# 5.0 0.75
# 6.0 2.45
# 7.0 7.7
# 8.0 24.5
# 9.0 74.3
# 0.5*(MW - 9)
# or half-width=74.3*10
# or echo 6.50 | awk '{print 74.3*exp(0.5*log(10.0)*(0300 - 9.0)) }'
#####
# Processing window for P (use SAC variable A for P arrival
# Start A - 30
# End A + 2*HALFWIDTH + 0.03*HS + 30 + 1/FH
# Processing window for SH (use SAC variable T0 for SH arrival
# Start T0 - 60
# End T0 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
# Processing window for SV (use SAC variable T1 for SV arrival
# Start T1 - 60
# End T1 + 2*HALFWIDTH + 0.06*HS + 30 + 1/FH
#
# The term involving HS serves to include the depth phases and
# to exclude the PP or SS at most distanace
#####
The cut windows attempt to include the P, pP, sP, pS, S and sS arrivals. However, oen must be very careful about the fact that PP may be included in some distance ranges.
The waveforms are then bandpass filtered by the application of the following high- and low-pass stages (an optional microseism filter):
hp c 0.0100 2 lp c 0.0500 2 int br c 0.12 0.25 n 4 p 2The traces were next integrated to ground displacment in meters. Finally the observed data are interpolated to ahve the same sampling at the Green's functions.
The source inversion is a multipass operation since a lower frequency filter band is used for larger earthquakes and since a search is made over depth. Up to three passed of the outer loop are made, after which the moment magnitude is determined and filter settings readjusted. The inner loop over depth samples all depths from 0 to 800 km with 5 km increments in depth to 50 km, followed by 10 km depth sampling for the remaining range.
The following filter ranges are used according to the moment magnitude Mw:
FILTER_BAND 1/FH(s) 1/FL(s)
1 60 12 Mw < 6.4
2 100 20 6.4 < Mw <= 6.9
3 120 40 Mw > 6.9
The map displays the distribution of stations used for this source inversion.
Location of the earthquake (yellow star) and great circle path from the epicenter to each station (red) [created using GMT (Wessel, P., and W. H. F. Smith, New version of Generic Mapping Tools released, EOS Trans. AGU, 76 329, 1995.)] |
For this data set the favored solution is
WVFGRD96 30.0 0 70 -50 6.47 0.5060
The following figures show the sensitivity of the goodness of fit parameter so source depth, the waveform comparison as a function of epicentral distance in degrees and the source to station azimuth
|
| Goodness of fit as a function of source depth. The measure is 1 - SUM (o -p)2 / SUM o2. A value of 1.0 is the best fit. The best double couple mechanism for the solution depth is plotted above goodness of fit value to indicate how the mefhanism may change with depth. |
| P-wave Z component |
|
| Comparison of the observed traces (red) and solution predicted traces (blue) ordered in terms of increasing epicentral distance. Each pair of traces is annotated with the station name, epicentral distance in degrees, source to station azimuth in degrees. Each pair of traces is plotted with the same scale and the peak amplitudes are indicated at the lect of each trace. Finally the time shift between the P-wave first arrival picked and the the theoretical P-wave first arrival in the predicted trace is indicated, with a positive sign indicating that the predicted trace has been shifted to the right by the given number of seconds. as a function of source to station azimuth in degrees (D). The purpose of this display is to highlight the azimuthal dependence on the first motion. The traces are annotated with the station name at the top. |
Starting Processing : Sat Apr 14 03:27:17 UTC 2007 Starting query to get files : Sat Apr 14 03:27:17 UTC 2007 Starting stareq for response: Sat Apr 14 03:36:36 UTC 2007 Starting deconvolution : Sat Apr 14 03:39:06 UTC 2007 Starting trace rotation : Sat Apr 14 03:40:37 UTC 2007 Starting distance selection : Sat Apr 14 03:40:58 UTC 2007 Starting trace QC : Sat Apr 14 03:41:06 UTC 2007 Starting MTD : Sat Apr 14 03:47:12 UTC 2007 Starting Grid Search : Sat Apr 14 04:17:59 UTC 2007