2013/03/25 07:21:00 41.77 19.95 10.0 4.3 Albania
USGS Felt map for this earthquake
USGS/SLU Moment Tensor Solution ENS 2013/03/25 07:21:00:0 41.77 19.95 10.0 4.3 Albania Stations used: HT.AGG HT.ALN HT.FNA HT.HORT HT.KNT HT.LIT HT.PAIG HT.SIGR HT.SOH HT.SRS HT.THE HT.XOR HU.BUD HU.MORH HU.PSZ MN.BLY MN.PDG MN.TIR MN.VTS RO.BZS RO.VOIR SJ.BBLS SJ.FRGS Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 9.23e+21 dyne-cm Mw = 3.91 Z = 23 km Plane Strike Dip Rake NP1 245 80 -70 NP2 0 22 -153 Principal Axes: Axis Value Plunge Azimuth T 9.23e+21 32 318 N 0.00e+00 20 61 P -9.23e+21 51 178 Moment Tensor: (dyne-cm) Component Value Mxx 5.51e+19 Mxy -3.13e+21 Mxz 7.61e+21 Myy 2.91e+21 Myz -2.95e+21 Mzz -2.97e+21 ###########--- ##################---- ########################---- ##########################---- ###### #####################---- ####### T ######################---- ######## #######################-### #############################------##### ########################------------#### #####################----------------##### #################--------------------##### ##############-----------------------##### ##########---------------------------##### ######------------------------------#### ####-------------------------------##### #----------------- -------------#### ----------------- P ------------#### ---------------- -----------#### --------------------------#### ------------------------#### ------------------#### -----------### Global CMT Convention Moment Tensor: R T P -2.97e+21 7.61e+21 2.95e+21 7.61e+21 5.51e+19 3.13e+21 2.95e+21 3.13e+21 2.91e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.EU/20130325072100/index.html |
STK = 245 DIP = 80 RAKE = -70 MW = 3.91 HS = 23.0
The waveform inversion is preferred.
The following compares this source inversion to others
USGS/SLU Moment Tensor Solution ENS 2013/03/25 07:21:00:0 41.77 19.95 10.0 4.3 Albania Stations used: HT.AGG HT.ALN HT.FNA HT.HORT HT.KNT HT.LIT HT.PAIG HT.SIGR HT.SOH HT.SRS HT.THE HT.XOR HU.BUD HU.MORH HU.PSZ MN.BLY MN.PDG MN.TIR MN.VTS RO.BZS RO.VOIR SJ.BBLS SJ.FRGS Filtering commands used: hp c 0.02 n 3 lp c 0.06 n 3 Best Fitting Double Couple Mo = 9.23e+21 dyne-cm Mw = 3.91 Z = 23 km Plane Strike Dip Rake NP1 245 80 -70 NP2 0 22 -153 Principal Axes: Axis Value Plunge Azimuth T 9.23e+21 32 318 N 0.00e+00 20 61 P -9.23e+21 51 178 Moment Tensor: (dyne-cm) Component Value Mxx 5.51e+19 Mxy -3.13e+21 Mxz 7.61e+21 Myy 2.91e+21 Myz -2.95e+21 Mzz -2.97e+21 ###########--- ##################---- ########################---- ##########################---- ###### #####################---- ####### T ######################---- ######## #######################-### #############################------##### ########################------------#### #####################----------------##### #################--------------------##### ##############-----------------------##### ##########---------------------------##### ######------------------------------#### ####-------------------------------##### #----------------- -------------#### ----------------- P ------------#### ---------------- -----------#### --------------------------#### ------------------------#### ------------------#### -----------### Global CMT Convention Moment Tensor: R T P -2.97e+21 7.61e+21 2.95e+21 7.61e+21 5.51e+19 3.13e+21 2.95e+21 3.13e+21 2.91e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.EU/20130325072100/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 3The results of this grid search from 0.5 to 19 km depth are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 0.5 240 50 90 3.51 0.3356 WVFGRD96 1.0 60 40 90 3.57 0.3505 WVFGRD96 2.0 65 40 95 3.66 0.4144 WVFGRD96 3.0 240 50 90 3.74 0.4084 WVFGRD96 4.0 235 55 85 3.76 0.3344 WVFGRD96 5.0 220 65 65 3.74 0.2805 WVFGRD96 6.0 240 90 -75 3.68 0.3002 WVFGRD96 7.0 60 90 75 3.68 0.3448 WVFGRD96 8.0 60 90 75 3.77 0.3750 WVFGRD96 9.0 60 90 75 3.77 0.4209 WVFGRD96 10.0 60 90 75 3.78 0.4604 WVFGRD96 11.0 240 85 -75 3.79 0.4987 WVFGRD96 12.0 240 85 -75 3.79 0.5300 WVFGRD96 13.0 240 85 -75 3.80 0.5573 WVFGRD96 14.0 235 80 -75 3.82 0.5816 WVFGRD96 15.0 240 80 -70 3.83 0.6027 WVFGRD96 16.0 240 80 -70 3.84 0.6211 WVFGRD96 17.0 240 80 -70 3.85 0.6363 WVFGRD96 18.0 240 80 -70 3.86 0.6491 WVFGRD96 19.0 240 80 -70 3.87 0.6591 WVFGRD96 20.0 240 80 -70 3.88 0.6666 WVFGRD96 21.0 240 80 -70 3.89 0.6716 WVFGRD96 22.0 240 80 -70 3.90 0.6747 WVFGRD96 23.0 245 80 -70 3.91 0.6760 WVFGRD96 24.0 245 80 -70 3.92 0.6756 WVFGRD96 25.0 245 80 -70 3.93 0.6731 WVFGRD96 26.0 245 80 -70 3.94 0.6687 WVFGRD96 27.0 245 80 -70 3.94 0.6626 WVFGRD96 28.0 245 80 -70 3.95 0.6548 WVFGRD96 29.0 250 80 -65 3.97 0.6455
The best solution is
WVFGRD96 23.0 245 80 -70 3.91 0.6760
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
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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=Mon Mar 25 08:20:52 CDT 2013