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(Powers; October 28, 1997)<br />

disturbed by construction or material brought in for construction, 2) Holocene('?) dune<br />

sand, 3) Pleistocene Berino soil, 4) Pleistocene Mescalero caliche, 5) Mioceno ­<br />

Pleistocene Gatufia Formation, 6) Triassic Santa Rosa Formation, and 7) Permian<br />

Dewey Lake Formation. All formations were encountered during the drilling gonerally<br />

as expected,<br />

.~II, construction material<br />

:........... HolOCene (?) dune sand<br />

f=::.:::::::=:j: Pleistocene Berino soil<br />

'--.-=~...,--<br />

=""1,, Pleistocene Mescalero caliche<br />

Miocene-Pleistocene<br />

Gatufia Formation<br />

Triassic Santa Rosa<br />

Formation<br />

. Permian Dewey Lake<br />

Formation<br />

Figure 1<br />

Units Commonly Encountered During<br />

Shallow Drilling at WIPP<br />

exshft2. wpd<br />

4<br />

(Geology ofPiezcmeter Holes)<br />

The geology of these<br />

drillholes could be forEicast on<br />

the basis of the mapping of the<br />

exhaust and air intake shafts<br />

(Holt and Powers, 1986, 1990)<br />

as well as nearby drillholes<br />

such as B-25 (Bechtel National,<br />

Inc" 1979) and WIPP:21<br />

(Sandia [National] Laboratories<br />

and US Geological SUI'Vey,<br />

1980). Drilling to inve!;tigate<br />

potash resources revealed the<br />

broader stratigraphic<br />

relationships and presl~nce of<br />

the Santa Rosa over the site<br />

(Jones, 1978). Numemus<br />

shallow holes (B series) were<br />

drilled in 1979 for desi!~n of<br />

surface facilities, and tl1ese<br />

drillholes demonstrated the<br />

lack of very shallow<br />

groundwater as well as; the<br />

distribution of near surface rock units (Sergent, Hauskins & Beckwith, 1979).

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