USGS/SLU Moment Tensor Solution ENS 2021/04/19 22:57:11:1 47.77 16.13 5.0 4.3 Austria Stations used: BW.BGDS BW.BHG BW.MANZ BW.MGBB BW.ROTZ BW.SCE CH.BERNI CH.DAVOX CR.ZAG GR.BRG GR.CLL GR.GEC2 GR.GEC7 GR.GRA1 GR.GRA2 GR.GRA4 GR.GRB1 GR.GRB2 GR.GRB3 GR.GRB4 GR.GRB5 GR.GRC1 GR.GRC3 GR.GRC4 GR.MOX HU.BEHE HU.CSKK HU.EGYH HU.KOVH HU.MORH HU.MPLH HU.SOP HU.TIH MN.BLY MN.DPC MN.TRI OE.ABTA OE.ARSA OE.BIOA OE.CONA OE.CSNA OE.DAVA OE.FETA OE.KBA OE.MOA OE.MYKA OE.OBKA OE.SOKA OE.SQTA OE.VIE OE.WATA OX.BAD OX.BOO OX.CAE OX.CIMO OX.CLUD OX.DRE OX.FUSE OX.MLN OX.MPRI OX.PLRO OX.SABO OX.VARN SL.BOJS SL.CADS SL.CEY SL.CRES SL.CRNS SL.DOBS SL.GBAS SL.GBRS SL.GCIS SL.GOLS SL.GORS SL.GROS SL.JAVS SL.KNDS SL.KOGS SL.LJU SL.MOZS SL.PERS SL.ROBS SL.SKDS SL.VISS SL.VNDS SL.VOJS SL.ZAVS Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.14e+22 dyne-cm Mw = 3.97 Z = 15 km Plane Strike Dip Rake NP1 112 74 -110 NP2 345 25 -40 Principal Axes: Axis Value Plunge Azimuth T 1.14e+22 27 218 N 0.00e+00 19 118 P -1.14e+22 56 357 Moment Tensor: (dyne-cm) Component Value Mxx 2.21e+21 Mxy 4.58e+21 Mxz -8.83e+21 Myy 3.38e+21 Myz -2.49e+21 Mzz -5.59e+21 -------####### ----------------###### ----------------------###### -------------------------##### ----------------------------###### ---------------- ------------##### ----------------- P -------------##### ##---------------- -------------###### ####-------------------------------##### #######------------------------------##### ##########---------------------------##### #############------------------------##### #################--------------------##### #####################---------------#### ###########################--------##### ##################################---- ####### ######################---- ###### T #####################---- #### ####################--- #########################--- ####################-- #############- Global CMT Convention Moment Tensor: R T P -5.59e+21 -8.83e+21 2.49e+21 -8.83e+21 2.21e+21 -4.58e+21 2.49e+21 -4.58e+21 3.38e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210419225711/index.html |
STK = 345 DIP = 25 RAKE = -40 MW = 3.97 HS = 15.0
The NDK file is 20210419225711.ndk The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2021/04/19 22:57:11:1 47.77 16.13 5.0 4.3 Austria Stations used: BW.BGDS BW.BHG BW.MANZ BW.MGBB BW.ROTZ BW.SCE CH.BERNI CH.DAVOX CR.ZAG GR.BRG GR.CLL GR.GEC2 GR.GEC7 GR.GRA1 GR.GRA2 GR.GRA4 GR.GRB1 GR.GRB2 GR.GRB3 GR.GRB4 GR.GRB5 GR.GRC1 GR.GRC3 GR.GRC4 GR.MOX HU.BEHE HU.CSKK HU.EGYH HU.KOVH HU.MORH HU.MPLH HU.SOP HU.TIH MN.BLY MN.DPC MN.TRI OE.ABTA OE.ARSA OE.BIOA OE.CONA OE.CSNA OE.DAVA OE.FETA OE.KBA OE.MOA OE.MYKA OE.OBKA OE.SOKA OE.SQTA OE.VIE OE.WATA OX.BAD OX.BOO OX.CAE OX.CIMO OX.CLUD OX.DRE OX.FUSE OX.MLN OX.MPRI OX.PLRO OX.SABO OX.VARN SL.BOJS SL.CADS SL.CEY SL.CRES SL.CRNS SL.DOBS SL.GBAS SL.GBRS SL.GCIS SL.GOLS SL.GORS SL.GROS SL.JAVS SL.KNDS SL.KOGS SL.LJU SL.MOZS SL.PERS SL.ROBS SL.SKDS SL.VISS SL.VNDS SL.VOJS SL.ZAVS Filtering commands used: cut o DIST/3.3 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 1.14e+22 dyne-cm Mw = 3.97 Z = 15 km Plane Strike Dip Rake NP1 112 74 -110 NP2 345 25 -40 Principal Axes: Axis Value Plunge Azimuth T 1.14e+22 27 218 N 0.00e+00 19 118 P -1.14e+22 56 357 Moment Tensor: (dyne-cm) Component Value Mxx 2.21e+21 Mxy 4.58e+21 Mxz -8.83e+21 Myy 3.38e+21 Myz -2.49e+21 Mzz -5.59e+21 -------####### ----------------###### ----------------------###### -------------------------##### ----------------------------###### ---------------- ------------##### ----------------- P -------------##### ##---------------- -------------###### ####-------------------------------##### #######------------------------------##### ##########---------------------------##### #############------------------------##### #################--------------------##### #####################---------------#### ###########################--------##### ##################################---- ####### ######################---- ###### T #####################---- #### ####################--- #########################--- ####################-- #############- Global CMT Convention Moment Tensor: R T P -5.59e+21 -8.83e+21 2.49e+21 -8.83e+21 2.21e+21 -4.58e+21 2.49e+21 -4.58e+21 3.38e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20210419225711/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.
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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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 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 1.0 125 50 95 3.70 0.3803 WVFGRD96 2.0 305 40 90 3.78 0.4233 WVFGRD96 3.0 130 40 -85 3.83 0.3917 WVFGRD96 4.0 320 55 -75 3.85 0.3396 WVFGRD96 5.0 10 15 -10 3.86 0.4018 WVFGRD96 6.0 10 15 -10 3.86 0.4558 WVFGRD96 7.0 5 20 -15 3.85 0.4958 WVFGRD96 8.0 0 15 -20 3.93 0.5241 WVFGRD96 9.0 -5 15 -25 3.94 0.5579 WVFGRD96 10.0 355 20 -25 3.94 0.5852 WVFGRD96 11.0 345 20 -40 3.95 0.6060 WVFGRD96 12.0 345 20 -40 3.95 0.6201 WVFGRD96 13.0 345 25 -40 3.96 0.6306 WVFGRD96 14.0 345 25 -40 3.97 0.6360 WVFGRD96 15.0 345 25 -40 3.97 0.6370 WVFGRD96 16.0 345 25 -40 3.97 0.6346 WVFGRD96 17.0 345 25 -40 3.98 0.6294 WVFGRD96 18.0 350 25 -30 3.98 0.6227 WVFGRD96 19.0 350 25 -30 3.98 0.6144 WVFGRD96 20.0 350 25 -30 3.99 0.6050 WVFGRD96 21.0 355 25 -25 4.00 0.5956 WVFGRD96 22.0 355 25 -25 4.00 0.5844 WVFGRD96 23.0 -5 25 -25 4.01 0.5727 WVFGRD96 24.0 -5 25 -25 4.01 0.5601 WVFGRD96 25.0 -5 25 -25 4.01 0.5471 WVFGRD96 26.0 -5 25 -25 4.02 0.5336 WVFGRD96 27.0 0 25 -20 4.02 0.5197 WVFGRD96 28.0 0 25 -20 4.02 0.5056 WVFGRD96 29.0 0 25 -20 4.03 0.4912
The best solution is
WVFGRD96 15.0 345 25 -40 3.97 0.6370
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 -30 o DIST/3.3 +70 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.06 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.
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: