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DOE 2000. - Waste Isolation Pilot Plant - U.S. Department of Energy

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WIPP RH PSAR <strong>DOE</strong>/WIPP-03-3174 CHAPTER 2<br />

Up to August 1981, NMT calculated magnitudes differently than other organizations. As a result,<br />

systematic differences in calculated magnitudes were observed. In Table 2.5-3, all magnitudes calculated<br />

by organizations other than NMT were modified by applying corrections. In all cases, these<br />

modifications reduced the reported magnitude by amounts ranging from 0.3 to 0.5.<br />

After August 1981, NMT started using a magnitude scale based on the duration (t D ) <strong>of</strong> the recorded<br />

signal from onset <strong>of</strong> the P phase to when the trace amplitude approaches background noise. The equation<br />

used,<br />

M D = 2.79 log t D - 3.63<br />

was derived by LANL researchers 21 and determined to be equivalent to the Richter local magnitude scale<br />

for earthquakes in northern New Mexico. Ake and Sanford 18 established that the LANL formula can be<br />

applied to earthquakes in central New Mexico which fall in the local magnitude range <strong>of</strong> 1.1 to 4.2. A<br />

careful study <strong>of</strong> the applicability <strong>of</strong> the formula to earthquakes in southeastern New Mexico and west<br />

Texas has not been made.<br />

However, random comparisons between magnitudes calculated from the amplitude <strong>of</strong> S g (Shear Wave)<br />

and duration <strong>of</strong> ground motion in the time period 1962 to 1974 indicate general consensus good<br />

agreement (within 0.3 magnitude units) between the two methods.<br />

Most recurrence formulas in Section 2.5.4.2 are based on the earthquake data set included in Table 2.5-3,<br />

but at lower magnitudes. Therefore, the latest listing <strong>of</strong> events within the WIPP facility region does not<br />

require an upward revision in earthquake risk or the DBE.<br />

2.5.1.2.2 Completeness <strong>of</strong> the Earthquake Data Set<br />

From January 1, 1962 to April 5, 1974, events in the WIPP facility region were located by readings from<br />

stations generally several hundred miles from the epicenter. On April 5, 1974, a single station (CLN)<br />

was established near the center location <strong>of</strong> the WIPP facility which continued operation to September<br />

1980. These stations are plotted in Figure 2.5-3. From November 1975 to late 1979, a seismograph<br />

array was in operation near Kermit, Texas. These are shown in Figure 2.5-4.<br />

A small network <strong>of</strong> stations centered in the Davis Mountains <strong>of</strong> West Texas was operated by the UTA<br />

from July 1977 to July 1978. No stations were running near the location <strong>of</strong> the WIPP facility from<br />

shutdown <strong>of</strong> station CLN in September 1980 to startup <strong>of</strong> a three station network in August 1982. The<br />

WIPP seismograph network was not fully operational until March 1983.<br />

The histograms in Figure 2.5-5 illustrate how the shifts in instrumentation affected the completeness <strong>of</strong><br />

the earthquake data set presented in Table 2.5-3. The period from January 1, 1962 through September<br />

30, 1986 was divided into eight time intervals <strong>of</strong> 1130 days, and the number <strong>of</strong> events greater than 3.0,<br />

2.5, 2.0, and 1.5 were determined for each interval. The first four intervals (from January 1, 1962<br />

through May 17, 1974) cover the period prior to installation <strong>of</strong> any stations at, or near the location <strong>of</strong> the<br />

WIPP facility. The fifth and sixth intervals (from May 18, 1974 through July 24, 1980) cover the period<br />

when station CLN, the Kermit array, and the UTA networks were in operation. Most <strong>of</strong> the seventh<br />

interval (from July 25, 1980 to August 28, 1983) covers the period between shutdown <strong>of</strong> station CLN<br />

and startup <strong>of</strong> the WIPP seismographic network. During the last interval (from August 29, 1983 through<br />

September 30, 1986) the WIPP array was fully operational.<br />

2.5-3 January 24, 2003

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