2013/06/14 11:53:01 60.892 -149.973 37.8 3.8 Alaska
USGS Felt map for this earthquake
USGS/SLU Moment Tensor Solution ENS 2013/06/14 11:53:01:0 60.89 -149.97 37.8 3.8 Alaska Stations used: AK.BAL AK.BRLK AK.CAST AK.CNP AK.GLI AK.KTH AK.RC01 AK.SCM AK.SSN AK.TRF AT.MENT AT.PMR AT.SVW2 AT.TTA IU.COLA Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 6.53e+21 dyne-cm Mw = 3.81 Z = 42 km Plane Strike Dip Rake NP1 220 55 -80 NP2 23 36 -104 Principal Axes: Axis Value Plunge Azimuth T 6.53e+21 9 303 N 0.00e+00 8 34 P -6.53e+21 77 164 Moment Tensor: (dyne-cm) Component Value Mxx 1.58e+21 Mxy -2.81e+21 Mxz 1.91e+21 Myy 4.46e+21 Myz -1.27e+21 Mzz -6.04e+21 ############## #####################- #######################--### ###################--------### ##############-------------#### # T ############---------------##### ## ##########------------------##### ##############--------------------###### ############----------------------###### ############-----------------------####### ###########------------------------####### ##########---------- ------------####### #########----------- P -----------######## #######------------ ----------######## #######-------------------------######## #####-------------------------######## ####-----------------------######### ###----------------------######### #--------------------######### #-----------------########## -----------########### ############## Global CMT Convention Moment Tensor: R T P -6.04e+21 1.91e+21 1.27e+21 1.91e+21 1.58e+21 2.81e+21 1.27e+21 2.81e+21 4.46e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20130614115301/index.html |
STK = 220 DIP = 55 RAKE = -80 MW = 3.81 HS = 42.0
The NDK file is 20130614115301.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2013/06/14 11:53:01:0 60.89 -149.97 37.8 3.8 Alaska Stations used: AK.BAL AK.BRLK AK.CAST AK.CNP AK.GLI AK.KTH AK.RC01 AK.SCM AK.SSN AK.TRF AT.MENT AT.PMR AT.SVW2 AT.TTA IU.COLA Filtering commands used: hp c 0.02 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 6.53e+21 dyne-cm Mw = 3.81 Z = 42 km Plane Strike Dip Rake NP1 220 55 -80 NP2 23 36 -104 Principal Axes: Axis Value Plunge Azimuth T 6.53e+21 9 303 N 0.00e+00 8 34 P -6.53e+21 77 164 Moment Tensor: (dyne-cm) Component Value Mxx 1.58e+21 Mxy -2.81e+21 Mxz 1.91e+21 Myy 4.46e+21 Myz -1.27e+21 Mzz -6.04e+21 ############## #####################- #######################--### ###################--------### ##############-------------#### # T ############---------------##### ## ##########------------------##### ##############--------------------###### ############----------------------###### ############-----------------------####### ###########------------------------####### ##########---------- ------------####### #########----------- P -----------######## #######------------ ----------######## #######-------------------------######## #####-------------------------######## ####-----------------------######### ###----------------------######### #--------------------######### #-----------------########## -----------########### ############## Global CMT Convention Moment Tensor: R T P -6.04e+21 1.91e+21 1.27e+21 1.91e+21 1.58e+21 2.81e+21 1.27e+21 2.81e+21 4.46e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20130614115301/index.html |
(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.
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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:
hp c 0.02 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 250 45 -90 3.06 0.2517 WVFGRD96 1.0 285 85 0 3.08 0.2093 WVFGRD96 2.0 255 45 -90 3.20 0.2874 WVFGRD96 3.0 290 75 10 3.25 0.2488 WVFGRD96 4.0 300 55 25 3.30 0.2467 WVFGRD96 5.0 145 30 -15 3.26 0.2770 WVFGRD96 6.0 140 30 -25 3.27 0.3127 WVFGRD96 7.0 135 30 -30 3.28 0.3337 WVFGRD96 8.0 125 25 -35 3.35 0.3430 WVFGRD96 9.0 125 25 -35 3.34 0.3474 WVFGRD96 10.0 135 30 -30 3.33 0.3489 WVFGRD96 11.0 135 30 -30 3.33 0.3498 WVFGRD96 12.0 135 30 -30 3.33 0.3511 WVFGRD96 13.0 135 30 -30 3.34 0.3519 WVFGRD96 14.0 240 80 -60 3.36 0.3533 WVFGRD96 15.0 240 80 -60 3.37 0.3572 WVFGRD96 16.0 245 85 -55 3.38 0.3614 WVFGRD96 17.0 245 85 -55 3.39 0.3650 WVFGRD96 18.0 245 85 -55 3.40 0.3678 WVFGRD96 19.0 240 65 -50 3.43 0.3717 WVFGRD96 20.0 240 65 -50 3.44 0.3781 WVFGRD96 21.0 240 65 -50 3.46 0.3839 WVFGRD96 22.0 240 65 -50 3.47 0.3901 WVFGRD96 23.0 235 60 -55 3.48 0.3973 WVFGRD96 24.0 230 55 -55 3.49 0.4043 WVFGRD96 25.0 230 55 -55 3.50 0.4127 WVFGRD96 26.0 230 55 -55 3.51 0.4224 WVFGRD96 27.0 225 55 -60 3.53 0.4335 WVFGRD96 28.0 225 55 -65 3.54 0.4460 WVFGRD96 29.0 225 55 -65 3.55 0.4608 WVFGRD96 30.0 225 55 -65 3.56 0.4770 WVFGRD96 31.0 225 55 -65 3.58 0.4942 WVFGRD96 32.0 230 55 -65 3.59 0.5130 WVFGRD96 33.0 225 55 -70 3.61 0.5298 WVFGRD96 34.0 225 55 -70 3.62 0.5439 WVFGRD96 35.0 225 55 -70 3.63 0.5538 WVFGRD96 36.0 225 55 -70 3.64 0.5602 WVFGRD96 37.0 220 50 -75 3.65 0.5652 WVFGRD96 38.0 220 50 -75 3.67 0.5698 WVFGRD96 39.0 215 50 -80 3.69 0.5732 WVFGRD96 40.0 220 55 -80 3.79 0.5746 WVFGRD96 41.0 220 55 -80 3.80 0.5796 WVFGRD96 42.0 220 55 -80 3.81 0.5805 WVFGRD96 43.0 215 50 -85 3.82 0.5780 WVFGRD96 44.0 215 50 -85 3.83 0.5773 WVFGRD96 45.0 215 50 -85 3.84 0.5730 WVFGRD96 46.0 25 40 -95 3.84 0.5686 WVFGRD96 47.0 25 40 -95 3.85 0.5625 WVFGRD96 48.0 215 50 -85 3.85 0.5542 WVFGRD96 49.0 30 40 -90 3.86 0.5461
The best solution is
WVFGRD96 42.0 220 55 -80 3.81 0.5805
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
hp c 0.02 n 3 lp c 0.10 n 3 br c 0.12 0.25 n 4 p 2
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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 WUS model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows:
MODEL.01 Model after 8 iterations 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 1.9000 3.4065 2.0089 2.2150 0.302E-02 0.679E-02 0.00 0.00 1.00 1.00 6.1000 5.5445 3.2953 2.6089 0.349E-02 0.784E-02 0.00 0.00 1.00 1.00 13.0000 6.2708 3.7396 2.7812 0.212E-02 0.476E-02 0.00 0.00 1.00 1.00 19.0000 6.4075 3.7680 2.8223 0.111E-02 0.249E-02 0.00 0.00 1.00 1.00 0.0000 7.9000 4.6200 3.2760 0.164E-10 0.370E-10 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: