USGS/SLU Moment Tensor Solution ENS 2020/10/24 16:18:47:0 62.25 -124.43 6.5 4.7 Canada, NWT Stations used: 1E.MONT2 1E.MONT7 1E.MONT9 AK.BESE AK.JIS AK.LOGN AK.PIN AK.PNL AK.R32K AK.S31K AK.S32K AK.U33K AK.V35K AT.SIT CN.BRWY CN.DAWY CN.DLBC CN.FNSB CN.FSJB CN.HYT CN.INK CN.KUKN CN.NAB1 CN.NAB2 CN.NAHA CN.NBC1 CN.NBC5 CN.NBC7 CN.NBC8 CN.PLBC CN.WHY CN.YUK2 CN.YUK3 CN.YUK4 CN.YUK5 CN.YUK6 CN.YUK7 CN.YUK8 EO.FSJ2 NY.MMPY NY.WGLY NY.WTLY RV.DEDWA TA.EPYK TA.F30M TA.F31M TA.G29M TA.G30M TA.H29M TA.H31M TA.I28M TA.I30M TA.J29N TA.J30M TA.K29M TA.L27K TA.L29M TA.M29M TA.M30M TA.M31M TA.N30M TA.N31M TA.O28M TA.O29M TA.O30N TA.P29M TA.P30M TA.P32M TA.P33M TA.Q32M TA.R31K TA.R33M TA.S34M TA.T33K TA.T35M US.WRAK Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 6.61e+22 dyne-cm Mw = 4.48 Z = 4 km Plane Strike Dip Rake NP1 325 65 80 NP2 168 27 110 Principal Axes: Axis Value Plunge Azimuth T 6.61e+22 68 215 N 0.00e+00 9 329 P -6.61e+22 19 62 Moment Tensor: (dyne-cm) Component Value Mxx -6.63e+21 Mxy -1.99e+22 Mxz -2.80e+22 Myy -4.32e+22 Myz -3.15e+22 Mzz 4.98e+22 #------------- ###------------------- ----##---------------------- ---#######-------------------- ----###########------------------- ----##############------------- -- ----################------------ P --- -----##################---------- ---- -----####################--------------- -----######################--------------- -----#######################-------------- ------#######################------------- ------########## ###########------------ -----########## T ############---------- ------######### ############---------- ------########################-------- ------########################------ ------#######################----- ------#####################--- -------###################-- ------################ ------######## Global CMT Convention Moment Tensor: R T P 4.98e+22 -2.80e+22 3.15e+22 -2.80e+22 -6.63e+21 1.99e+22 3.15e+22 1.99e+22 -4.32e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20201024161847/index.html |
STK = 325 DIP = 65 RAKE = 80 MW = 4.48 HS = 4.0
The NDK file is 20201024161847.ndk
Although not very scientific, I like this one because it agrees with expected direction of maximum compressive stress axis of previous events.I had problems with the other two events this month, on 10/14 and 1/18I will review those again. Although not very scientific, I like this one because it agrees with expected direction of maximum compressive stress axis of previous events.I had problems with the other two events this month, on 10/14 and 1/18I will review those again
As I did before, I looked at the CMPINC and CMPAZ of the four NY network stations. The two that were HHZ had CMPINC and CMPAZ for E and their HHE had CMPINC CMPAZ for Z. The reason that I changed them is that the rotation with the given angles did not separate the Rayleigh and Love at low frequencies.
Since this event was larger I used the 0.025 - 0.06 Hz frequency band to avoid problems of velocity model. I used the CUS (craton) model since the long period waveforms were simple pulses in general and since many paths were on the continental side of the Rockies.
This mechanism is very dip-slippish. Perhaps this explains the lack of depth control on the earlier events this month.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2020/10/24 16:18:47:0 62.25 -124.43 6.5 4.7 Canada, NWT Stations used: 1E.MONT2 1E.MONT7 1E.MONT9 AK.BESE AK.JIS AK.LOGN AK.PIN AK.PNL AK.R32K AK.S31K AK.S32K AK.U33K AK.V35K AT.SIT CN.BRWY CN.DAWY CN.DLBC CN.FNSB CN.FSJB CN.HYT CN.INK CN.KUKN CN.NAB1 CN.NAB2 CN.NAHA CN.NBC1 CN.NBC5 CN.NBC7 CN.NBC8 CN.PLBC CN.WHY CN.YUK2 CN.YUK3 CN.YUK4 CN.YUK5 CN.YUK6 CN.YUK7 CN.YUK8 EO.FSJ2 NY.MMPY NY.WGLY NY.WTLY RV.DEDWA TA.EPYK TA.F30M TA.F31M TA.G29M TA.G30M TA.H29M TA.H31M TA.I28M TA.I30M TA.J29N TA.J30M TA.K29M TA.L27K TA.L29M TA.M29M TA.M30M TA.M31M TA.N30M TA.N31M TA.O28M TA.O29M TA.O30N TA.P29M TA.P30M TA.P32M TA.P33M TA.Q32M TA.R31K TA.R33M TA.S34M TA.T33K TA.T35M US.WRAK Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 6.61e+22 dyne-cm Mw = 4.48 Z = 4 km Plane Strike Dip Rake NP1 325 65 80 NP2 168 27 110 Principal Axes: Axis Value Plunge Azimuth T 6.61e+22 68 215 N 0.00e+00 9 329 P -6.61e+22 19 62 Moment Tensor: (dyne-cm) Component Value Mxx -6.63e+21 Mxy -1.99e+22 Mxz -2.80e+22 Myy -4.32e+22 Myz -3.15e+22 Mzz 4.98e+22 #------------- ###------------------- ----##---------------------- ---#######-------------------- ----###########------------------- ----##############------------- -- ----################------------ P --- -----##################---------- ---- -----####################--------------- -----######################--------------- -----#######################-------------- ------#######################------------- ------########## ###########------------ -----########## T ############---------- ------######### ############---------- ------########################-------- ------########################------ ------#######################----- ------#####################--- -------###################-- ------################ ------######## Global CMT Convention Moment Tensor: R T P 4.98e+22 -2.80e+22 3.15e+22 -2.80e+22 -6.63e+21 1.99e+22 3.15e+22 1.99e+22 -4.32e+22 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20201024161847/index.html |
|
(a) mLg computed using the IASPEI formula; (b) mLg residuals ; the values used for the trimmed mean are indicated.
(a) ML computed using the IASPEI formula for Horizontal components; (b) ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
(a) ML computed using the IASPEI formula for Vertical components (research); (b) ML residuals computed using a modified IASPEI formula that accounts for path specific attenuation; the values used for the trimmed mean are indicated. The ML relation used for each figure is given at the bottom of each plot.
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 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 1.0 305 80 75 4.55 0.6777 WVFGRD96 2.0 310 75 75 4.50 0.6808 WVFGRD96 3.0 315 70 75 4.47 0.6868 WVFGRD96 4.0 325 65 80 4.48 0.6891 WVFGRD96 5.0 155 25 95 4.48 0.6835 WVFGRD96 6.0 155 30 95 4.48 0.6678 WVFGRD96 7.0 330 60 90 4.47 0.6475 WVFGRD96 8.0 330 60 90 4.45 0.6244 WVFGRD96 9.0 265 50 -55 4.44 0.6282 WVFGRD96 10.0 265 50 -55 4.46 0.6277 WVFGRD96 11.0 265 50 -55 4.46 0.6355 WVFGRD96 12.0 265 50 -55 4.46 0.6363 WVFGRD96 13.0 265 50 -55 4.45 0.6316 WVFGRD96 14.0 270 50 -50 4.45 0.6233 WVFGRD96 15.0 270 50 -50 4.45 0.6136 WVFGRD96 16.0 270 50 -50 4.45 0.6024 WVFGRD96 17.0 270 50 -50 4.45 0.5906 WVFGRD96 18.0 270 50 -50 4.45 0.5788 WVFGRD96 19.0 270 50 -50 4.45 0.5671 WVFGRD96 20.0 270 50 -50 4.47 0.5508 WVFGRD96 21.0 270 50 -50 4.47 0.5360 WVFGRD96 22.0 335 55 -80 4.46 0.5252 WVFGRD96 23.0 335 55 -80 4.46 0.5166 WVFGRD96 24.0 335 55 -80 4.46 0.5072 WVFGRD96 25.0 335 55 -80 4.47 0.4976 WVFGRD96 26.0 340 55 -75 4.47 0.4880 WVFGRD96 27.0 340 55 -75 4.47 0.4780 WVFGRD96 28.0 340 55 -75 4.47 0.4679 WVFGRD96 29.0 340 55 -75 4.48 0.4577
The best solution is
WVFGRD96 4.0 325 65 80 4.48 0.6891
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 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.025 n 3 lp c 0.06 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.
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 Bureau of Mines, UC Berkely, Caltech, UC San Diego, Saint Louis University, University of Memphis, Lamont Doherty Earth Observatory, the Oklahoma Geological Survey, TexNet, the Iris stations, the Transportable Array of EarthScope and other networks.
The CUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
MODEL.01 CUS Model with Q from simple gamma values 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 1.0000 5.0000 2.8900 2.5000 0.172E-02 0.387E-02 0.00 0.00 1.00 1.00 9.0000 6.1000 3.5200 2.7300 0.160E-02 0.363E-02 0.00 0.00 1.00 1.00 10.0000 6.4000 3.7000 2.8200 0.149E-02 0.336E-02 0.00 0.00 1.00 1.00 20.0000 6.7000 3.8700 2.9020 0.000E-04 0.000E-04 0.00 0.00 1.00 1.00 0.0000 8.1500 4.7000 3.3640 0.194E-02 0.431E-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: