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MONITORING PASSIVE SEISMIC EMISSIONS WITH SURFACE AND SHALLOW BURIED ARRAYS  229

























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            FIGURE 10.18  Top left—Traces showing coherent noise generated between two of the arms of a star grid array. Horizontal grid lines
              represent 10 ms intervals. The noise is very broad band and is hitting the cable from the side and at a very high apparent velocity. This noise
            is very difficult to remove using standard filters. Top right—The same traces with the noise removed. Bottom left—Depth slice of a depth
            volume showing semblance computed from the unfiltered traces. Scale in feet. Bottom right—The same depth slice after trace filtering. Note
            that a microearthquake hypocenter is imaged clearly in the filtered data.

            times of these volumetric amplitude highs are the locations   remaining volumes into a final volume for use in computing
            and times of MEQs.                                   the fracture networks.

            Coherency and Semblance without Source Function      10.5.3  MEQ Methods
            Correction  The coherency can be computed across all of
            the traces without adjustment for wavelet changes between   10.5.3.1  MEQ Detection  To detect an MEQ, it must be
            the traces.  This method does not correct for the wavelet   located in X, Y, Z, and time. The accuracy of these measures
            changes with offset and azimuth and requires the presence of   depends on the grid design, aperture size, velocity model,
            signal that is long duration and that is P‐wave only.   and quality of calibration, as previously discussed. Various
            Documentation of this type of signal is shown by Sicking   approaches are employed for detecting the occurrence of
            et  al. (2014).  This method is used to compute the time   MEQs in surface microseismic data.
            steps  for cumulative activity imaging.  The workflow  for   One method employs STA/LTA. For this method, the
            this  method is to compute hundreds of thousands of   background amplitude in the trace data is computed by tak­
            semblance depth volumes, edit them both statistically and   ing the RMS amplitude of a very long‐time window, scanning
            graphically,  eliminate  the  volumes  that contain  larger   the trace for the RMS amplitude over a short‐time window
            amplitude slip dominated MEQs, and finally combine the   that slides along the trace, and taking the ratio of the short
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