2013/04/22 22:00:42 43.24 18.83 10.0 3.7 NW Balkan Region
USGS Felt map for this earthquake
USGS/SLU Moment Tensor Solution ENS 2013/04/22 22:00:42:0 43.24 18.83 10.0 3.7 NW Balkan Region Stations used: HT.HORT HT.KNT HT.LIT HT.SOH HT.SRS HT.THE HU.BUD MN.PDG MN.TRI MN.VTS RO.BZS SJ.BBLS SJ.FRGS SL.JAVS SL.KNDS SL.SKDS SL.VOJS Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 1.95e+21 dyne-cm Mw = 3.46 Z = 14 km Plane Strike Dip Rake NP1 22 74 -143 NP2 280 55 -20 Principal Axes: Axis Value Plunge Azimuth T 1.95e+21 12 147 N 0.00e+00 50 42 P -1.95e+21 37 246 Moment Tensor: (dyne-cm) Component Value Mxx 1.12e+21 Mxy -1.30e+21 Mxz 4.21e+19 Myy -4.94e+20 Myz 1.07e+21 Mzz -6.27e+20 ############## ###################--- ######################------ #######################------- #########################--------- #########################----------- #######---------------####------------ ####----------------------###----------- #-------------------------#######------- --------------------------##########------ --------------------------############---- -------------------------###############-- ------- --------------#################- ------ P --------------################# ------ -------------################## --------------------################## ------------------################## ----------------################## ------------########### #### ----------############ T ### -----############## ############## Global CMT Convention Moment Tensor: R T P -6.27e+20 4.21e+19 -1.07e+21 4.21e+19 1.12e+21 1.30e+21 -1.07e+21 1.30e+21 -4.94e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.EU/20130422220042/index.html |
STK = 280 DIP = 55 RAKE = -20 MW = 3.46 HS = 14.0
The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2013/04/22 22:00:42:0 43.24 18.83 10.0 3.7 NW Balkan Region Stations used: HT.HORT HT.KNT HT.LIT HT.SOH HT.SRS HT.THE HU.BUD MN.PDG MN.TRI MN.VTS RO.BZS SJ.BBLS SJ.FRGS SL.JAVS SL.KNDS SL.SKDS SL.VOJS Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 1.95e+21 dyne-cm Mw = 3.46 Z = 14 km Plane Strike Dip Rake NP1 22 74 -143 NP2 280 55 -20 Principal Axes: Axis Value Plunge Azimuth T 1.95e+21 12 147 N 0.00e+00 50 42 P -1.95e+21 37 246 Moment Tensor: (dyne-cm) Component Value Mxx 1.12e+21 Mxy -1.30e+21 Mxz 4.21e+19 Myy -4.94e+20 Myz 1.07e+21 Mzz -6.27e+20 ############## ###################--- ######################------ #######################------- #########################--------- #########################----------- #######---------------####------------ ####----------------------###----------- #-------------------------#######------- --------------------------##########------ --------------------------############---- -------------------------###############-- ------- --------------#################- ------ P --------------################# ------ -------------################## --------------------################## ------------------################## ----------------################## ------------########### #### ----------############ T ### -----############## ############## Global CMT Convention Moment Tensor: R T P -6.27e+20 4.21e+19 -1.07e+21 4.21e+19 1.12e+21 1.30e+21 -1.07e+21 1.30e+21 -4.94e+20 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.EU/20130422220042/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:
hp c 0.02 n 3 lp c 0.06 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 0.5 255 45 -70 3.23 0.3053 WVFGRD96 1.0 285 90 0 3.15 0.3262 WVFGRD96 2.0 105 85 0 3.24 0.4098 WVFGRD96 3.0 105 90 -10 3.27 0.4224 WVFGRD96 4.0 105 90 -40 3.35 0.4378 WVFGRD96 5.0 275 65 -40 3.38 0.4612 WVFGRD96 6.0 275 50 -30 3.40 0.4727 WVFGRD96 7.0 275 50 -30 3.41 0.4849 WVFGRD96 8.0 275 50 -30 3.44 0.4880 WVFGRD96 9.0 275 50 -30 3.45 0.4982 WVFGRD96 10.0 275 50 -30 3.45 0.5042 WVFGRD96 11.0 280 55 -20 3.44 0.5073 WVFGRD96 12.0 280 55 -20 3.45 0.5114 WVFGRD96 13.0 280 55 -20 3.46 0.5136 WVFGRD96 14.0 280 55 -20 3.46 0.5144 WVFGRD96 15.0 280 55 -20 3.47 0.5139 WVFGRD96 16.0 280 55 -20 3.47 0.5124 WVFGRD96 17.0 280 55 -20 3.48 0.5099 WVFGRD96 18.0 280 55 -15 3.49 0.5069 WVFGRD96 19.0 110 70 25 3.47 0.5048 WVFGRD96 20.0 110 70 25 3.47 0.5004 WVFGRD96 21.0 110 70 20 3.48 0.4961 WVFGRD96 22.0 110 70 20 3.49 0.4919 WVFGRD96 23.0 110 70 20 3.49 0.4873 WVFGRD96 24.0 285 60 -5 3.52 0.4850 WVFGRD96 25.0 290 70 25 3.52 0.4808 WVFGRD96 26.0 290 70 25 3.52 0.4771 WVFGRD96 27.0 290 70 25 3.53 0.4735 WVFGRD96 28.0 290 70 25 3.53 0.4696 WVFGRD96 29.0 290 70 25 3.54 0.4653
The best solution is
WVFGRD96 14.0 280 55 -20 3.46 0.5144
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 0.06 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.
Should the national backbone of the USGS Advanced National Seismic System (ANSS) be implemented with an interstation separation of 300 km, it is very likely that an earthquake such as this would have been recorded at distances on the order of 100-200 km. This means that the closest station would have information on source depth and mechanism that was lacking here.
Dr. Harley Benz, USGS, provided the USGS USNSN digital data. The digital data used in this study were provided by Natural Resources Canada through their AUTODRM site http://www.seismo.nrcan.gc.ca/nwfa/autodrm/autodrm_req_e.php, and IRIS using their BUD interface.
Thanks also to the many seismic network operators whose dedication make this effort possible: University of Alaska, University of Washington, Oregon State University, University of Utah, Montana Bureas of Mines, UC Berkely, Caltech, UC San Diego, Saint L ouis University, Universityof Memphis, Lamont Doehrty Earth Observatory, Boston College, the Iris stations and the Transportable Array of EarthScope.
The WUS 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:
DATE=Tue Apr 23 08:44:26 CDT 2013