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medium velocity ( 2880 to 30.80 ft / sec ) materials extended from 2 <br /> to 7 feet down to depths of 15 to 25 feet , where medium velocity <br /> ( 3660 ft / sec ) materials were encountered . Again , the medium <br /> velocity' materials extended to depths in excess of 96 feet . <br /> An anomalously low velocity ( 2100 ft /sec ) zone was <br /> encountered at depths of a few feet to about 15 to 20 feet <br /> beneath the ground surface in the vicinity of the central 75 feet <br /> of line S-3 . This zone corresponds to measurably lower blow <br /> counts from boring B-3 , and may represent less cemented or weaker <br /> materials or perhaps a filled , buried channel . An anomalously <br /> high velocity ( 6250 ft / sec ) zone was encountered ju.st east of the <br /> middle of line S-4 at a depth of a few feet down to perhaps 10 or <br /> 15 feet beneath the ground surface . This zone may represent a <br /> more cemented or gravelly matrix in .that location . Many of the <br /> lines have data with scatter , indicative of variations in the <br /> degree of cementation or content of rock fragments ( gravels or <br /> cobbles ) . <br /> Rippability <br /> The low to medium velocity materials should be rippable with <br /> relative ease . The medium velocity materials may require heavy <br /> excavation equipment , but should be rippable without blasting to <br /> facilitate mass excavation . Figure 5 relates ripper performance <br /> to seismic wave velocities . Subsurface materials at this site are <br /> alluvial fan deposits and include clays , silts , sands , and <br /> gravels as well as various combinations of these constituents . <br /> Groundwater <br /> Because seismic velo-cities remained well below 5000 ft /sec , <br /> it is unlikely that saturated aquifers will be encountered to <br /> depths of at least about 96 feet beneath the project site . Thin , <br /> perched groundwater zones may be present , having . escaped <br /> detection with the methods employed in this survey . <br /> Method and Equipment <br /> The seismic refraction survey procedure used for all lines <br /> consisted of placing 12 geophones in as straight a line as <br /> practical ( in plan ) spaced at 25— foot intervals along as constant <br /> a slope as practical ( in profile ) . A large sledge hammer was <br /> impacted 12 . 5 feet off both ends and at the center of each <br /> seismic line . The hammer impact generated seismic compression <br /> waves which were refracted thifough subsurface materials and <br /> received by the deployed geophones . Signals from the energy <br /> source initiation Ctime break ) and from the geophones were <br /> monitored ( amplified and filtered ) simultaneously by a <br /> seismograph and displayed graphically in analog form by an <br /> oscillograph . Permanent records produced by the oscillograph were <br /> field checked , catalogued , and returned to the office for data <br /> reduction and interpretation . <br /> Seismic refraction lines were surveyed for location and <br />