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2010-03-03_REPORT - C1980007
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2010-03-03_REPORT - C1980007
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Last modified
8/24/2016 4:00:31 PM
Creation date
7/12/2010 11:31:58 AM
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DRMS Permit Index
Permit No
C1980007
IBM Index Class Name
REPORT
Doc Date
3/3/2010
Doc Name
2nd Quarter 2009 Seismic Monitoring Report (Email)
From
Kathy Welt
To
DRMS
Permit Index Doc Type
Stability Report
Email Name
TAK
Media Type
D
Archive
No
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North Fork ValleV Seismic Network - Fourth Quarter 2009 <br />located 2,118 events (not all of which were seismic events). Many more triggered waveform <br />files were recorded, many of which have insufficient station data for locating the events. <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; Figure 1). 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 />1.7 or greater in size at the different mining locations and used that as a guide for selecting other <br />events of approximate ML 1.7 and larger. <br />During the fourth quarter, the station OXM had timing problems (P. Swanson, NIOSH, personal <br />communications, 2010), which resulted in some erroneous Earthworm locations and <br />overestimated coda magnitudes. We do not use these magnitudes in Table 3 and they are <br />denoted by an asterisk. <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 8 arrival 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 earthquakes. HYP071 <br />requires a plane-layered velocity model, indicating depths to the top of each constant velocity <br />layer, as well as station locations and arrival times, in order to relocate the earthquakes. The <br />velocity model (Table 2) was determined from a detailed seismic study at the West Elk Mine <br />(Swanson and Koontz, 2006). In that study, the recording stations were directly above the <br />mining panel and so all the seismic rays were considered to be direct rays. Station elevation <br />corrections (Table 1) were incorporated into the location program based on the elevation <br />differences between the station and the velocity model datum (2420 m [7938 ft]) and using a <br />weighted average velocity over the layers between the datum and the station elevation. - <br />Table 2. Velocity Model Used in Locating Earthquakes <br />Depth to Top of layer (km) <br />[mi] Velocity (km/sec) [ft/sec] <br />0.00 [0.00] 2.21 [7,251] <br />0.07 [0.04] 2.73 [8,957] <br />0.27 [0.17] 3.01 [9,876] <br />0.37 [0.23] 3.18 [10,434] <br />1.00 [0.62] 3.9 [12,796] <br />1.50 [0.93] 4.60 [15,093] <br />um W:\X_WCFS\PROJECTS\WEST ELK-MTN COAL\2009 Q4\Q4_2009_MCC.DOC\2-MAR-10\\OAK 3
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