The ANSS event ID is us7000mab9 and the event page is at https://earthquake.usgs.gov/earthquakes/eventpage/us7000mab9/executive.
2024/04/05 21:59:13 40.685 -74.735 9.4 4.0 New Jersey
USGS/SLU Moment Tensor Solution ENS 2024/04/05 21:59:13:0 40.69 -74.74 9.4 4.0 New Jersey Stations used: CN.KGNO IU.HRV IU.SSPA LD.FOR LD.GEDE LD.NPNY LD.PAL LD.SDMD N4.J57A N4.J59A N4.K57A N4.K62A N4.L56A N4.L59A N4.L61B N4.L64A N4.M57A N4.M63A N4.N58A N4.N62A N4.P57A N4.P61A N4.R61A NE.HNH NE.TRY NE.VT1 NE.WSPT PE.PAGS PE.PAKS PE.PALB PE.PAOC PE.PSBK PE.PSSK PE.PSUB PE.PSWB US.CBN US.LONY WU.MEDO WU.PECO Filtering commands used: cut o DIST/3.3 -40 o DIST/3.3 +50 rtr taper w 0.1 hp c 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2 Best Fitting Double Couple Mo = 4.79e+21 dyne-cm Mw = 3.72 Z = 11 km Plane Strike Dip Rake NP1 100 90 40 NP2 10 50 180 Principal Axes: Axis Value Plunge Azimuth T 4.79e+21 27 333 N 0.00e+00 50 100 P -4.79e+21 27 227 Moment Tensor: (dyne-cm) Component Value Mxx 1.25e+21 Mxy -3.45e+21 Mxz 3.03e+21 Myy -1.25e+21 Myz 5.34e+20 Mzz -2.69e+14 ############-- #################----- ###### ############------- ####### T #############------- ######### ##############-------- ############################-------- #############################--------- ##############################---------- ##############################---------- -----##########################----------- ----------------###############----------- --------------------------#####----------- -------------------------------######----- -----------------------------########### -----------------------------########### ------ ------------------########### ----- P -----------------########### ---- ----------------########### --------------------########## -----------------########### ------------########## ------######## Global CMT Convention Moment Tensor: R T P -2.69e+14 3.03e+21 -5.34e+20 3.03e+21 1.25e+21 3.45e+21 -5.34e+20 3.45e+21 -1.25e+21 Details of the solution is found at http://www.eas.slu.edu/eqc/eqc_mt/MECH.NA/20240405215913/index.html |
STK = 100 DIP = 90 RAKE = 40 MW = 3.72 HS = 11.0
The NDK file is 20240405215913.ndk The waveform inversion is preferred.
Given the availability of digital waveforms for determination of the moment tensor, this section documents the added processing leading to mLg, if appropriate to the region, and ML by application of the respective IASPEI formulae. As a research study, the linear distance term of the IASPEI formula for ML is adjusted to remove a linear distance trend in residuals to give a regionally defined ML. The defined ML uses horizontal component recordings, but the same procedure is applied to the vertical components since there may be some interest in vertical component ground motions. Residual plots versus distance may indicate interesting features of ground motion scaling in some distance ranges. A residual plot of the regionalized magnitude is given as a function of distance and azimuth, since data sets may transcend different wave propagation provinces.
Left: mLg computed using the IASPEI formula. Center: mLg residuals versus epicentral distance ; the values used for the trimmed mean magnitude estimate are indicated.
Right: residuals as a function of distance and azimuth.
Left: ML computed using the IASPEI formula for Horizontal components. Center: 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.
Right: Residuals from new relation as a function of distance and azimuth.
Left: ML computed using the IASPEI formula for Vertical components (research). Center: 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.
Right: Residuals from new relation as a function of distance and azimuth.
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The focal mechanism was determined using broadband seismic waveforms. The location of the event (star) and the stations used for (red) 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's 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 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2The results of this grid search are as follow:
DEPTH STK DIP RAKE MW FIT WVFGRD96 1.0 280 70 -10 3.60 0.4611 WVFGRD96 2.0 100 85 55 3.71 0.4835 WVFGRD96 3.0 100 85 55 3.72 0.5012 WVFGRD96 4.0 275 85 -50 3.71 0.5167 WVFGRD96 5.0 100 90 50 3.71 0.5323 WVFGRD96 6.0 100 90 50 3.70 0.5443 WVFGRD96 7.0 100 90 45 3.70 0.5538 WVFGRD96 8.0 275 80 -40 3.70 0.5613 WVFGRD96 9.0 100 90 40 3.70 0.5623 WVFGRD96 10.0 100 90 40 3.72 0.5631 WVFGRD96 11.0 100 90 40 3.72 0.5640 WVFGRD96 12.0 100 90 40 3.72 0.5628 WVFGRD96 13.0 275 80 -35 3.73 0.5617 WVFGRD96 14.0 275 80 -35 3.73 0.5589 WVFGRD96 15.0 100 90 35 3.74 0.5530 WVFGRD96 16.0 100 90 35 3.74 0.5485 WVFGRD96 17.0 275 80 -35 3.74 0.5448 WVFGRD96 18.0 275 80 -35 3.75 0.5387 WVFGRD96 19.0 275 80 -35 3.75 0.5320 WVFGRD96 20.0 100 90 40 3.77 0.5225 WVFGRD96 21.0 275 80 -35 3.78 0.5158 WVFGRD96 22.0 100 90 40 3.78 0.5061 WVFGRD96 23.0 100 90 40 3.79 0.4969 WVFGRD96 24.0 100 90 40 3.80 0.4874 WVFGRD96 25.0 275 80 -40 3.80 0.4786 WVFGRD96 26.0 275 80 -40 3.81 0.4683 WVFGRD96 27.0 100 90 40 3.81 0.4561 WVFGRD96 28.0 275 80 -40 3.82 0.4465 WVFGRD96 29.0 100 80 40 3.82 0.4336
The best solution is
WVFGRD96 11.0 100 90 40 3.72 0.5640
The mechanism corresponding 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, the velocity model used in the predictions may not be perfect and the epicentral parameters may be be off. 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 0.03 n 3 lp c 0.08 n 3 br c 0.12 0.25 n 4 p 2
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Figure 3. Waveform comparison for selected depth. Red: observed; Blue - predicted. The time shift with respect to the model prediction is indicated. The percent of fit is also indicated. The time scale is relative to the first trace sample. |
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Focal mechanism sensitivity at the preferred depth. The red color indicates a very good fit to the waveforms. 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.
The CUS.model used for the waveform synthetic seismograms and for the surface wave eigenfunctions and dispersion is as follows (The format is in the model96 format of Computer Programs in Seismology).
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