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2008-11-24_PERMIT FILE - C1996083 (5)
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2008-11-24_PERMIT FILE - C1996083 (5)
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Last modified
8/24/2016 3:38:13 PM
Creation date
2/23/2009 4:57:27 PM
Metadata
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Template:
DRMS Permit Index
Permit No
C1996083
IBM Index Class Name
Permit File
Doc Date
11/24/2008
Doc Name
3rd Quarter 2007 North Fork Valley Seimic Network Monitoring Report
Section_Exhibit Name
Volume IIIA Exhibit 18 Seismic Monitoring at BR Longwall Coal Mine
Media Type
D
Archive
No
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<br />North Fork Valley Seismic Network -Third Quarter 2001T <br />We reviewed the daily summary or heliocorder records (these are continuous recordings of 12- <br />hour periods conveniently plotted on one page) for filtered traces at three stations (WTM, LLM <br />and WFW). We also reviewed the list of events automatically detected and located by <br />Earthworm. Events were chosen based on amplitudes on the heliocorder records at the three <br />stations. We measured the amplitudes on these heliocorder records for events known to be ML <br />1.5 or greater in size at the different mining locations and used that as a guide for selecting other <br />events of approximate ML 1.5 and larger. <br />Location Methodology <br />We used the utility SUDSPICK in the program PC-SUDS (Banfill, 1996) to pick P- and S-wave <br />arrival times within the DMX files (triggered waveform data files) for our selected list of events. <br />Another utility within PC-SUDS, XTYHY71, was used to extract the arrival time picks from the <br />waveform data files and convert them to the correct format to be used in the location program <br />HYP071 (USGS, 1975). Only events with at least eight amval time picks were located. The <br />location accuracy usually improves as the number of stations increases. <br />A DOS version of the location program HYP071 was used to locate the seismic events. <br />HYP071 requires aplane-layered velocity model, indicating depths to the top of each constant <br />velocity layer, as well as station locations and arrival times, in order to relocate the seismic <br />events. The velocity model (Table 2) was determined from a detailed seismic study at the West <br />• Elk Mine (Swanson and Koontz, 2006). In that study, the recording stations were directly above <br />the mining panel and so all the seismic rays were considered to be direct rays. This velocity <br />model will be refined as further information is made available, particularly for recorded collapse <br />events with known locations. Station elevation corrections (Table 1) were incorporated into the <br />location program based on the elevation differences between the station and the velocity model <br />datum (6,500 ft [ 1.98 km]) and the velocity of the uppermost layer (7470 ft/sec [2.21 km/sec]). <br />Table 2. Velocity Model Used in Locating Seismic Events <br />Top of layer (km) [mi] Velocity (km/sec) [ft/sec] <br />0.00 [0.00] 2.21 [7,470] <br />0.07 [0.04] 2.73 [9,227] <br />0.27 [0.17] 3.01 [ 10,174] <br />0.37 [0.23] 3.18 [10,748] <br />1.50 [0.94] 3.96 [13,385] <br />2.50 [1.56] 4.40 [14,872] <br />6.00 [3.75] 6.00 [20,280] <br />Magnitude Estimation <br />Magnitudes in terms of ML were estimated for all mining-related events of ML 1.5 and greater <br />based on peak amplitudes as recorded on the Mesa State Seismic Network (MSSN) operated by <br />David Wolny. The standard Richter magnitude formula was used to calculate the ML values. <br />U~ W:UC_WCFS\PROJECTS\NORTH FORK-BOWIE\QUARTERLY REPORTS\2007 03\03_2007_BRL_FINAL.DOC112-FEB-OS\10AK 3 <br />
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