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Page 2 <br /> Tracy Tire Fire <br /> Celeste Temple,Project Officer <br /> BACKGROUND <br /> The Tracy Tire Fire site is located at 29425 S. MacArthur Rd. in Tracy (see Figure 1, Site <br /> Location Map). On August 7, 1998, a fire was started at the site, then named the Royster Tire <br /> facility. It was estimated that two to seven million tires were stored on the 30-acre site. In order <br /> to minimize environmental impacts, no measures were taken to mitigate or suppress the fire. <br /> Fires burn now only at a few scattered locations. The volume of tires and strength of the blaze <br /> have steadily diminished. <br /> The EPA is now preparing to implement the Quality Assurance Sampling Plan (QASP) that was <br /> completed in December 1998 to investigate the extent to which soil and water have been affected <br /> by the fire. This report of site geology/iiydrogeology will be used to determine potential <br /> contaminant migration paths and guide the investigation. The geology/hydrogeology and the <br /> groundwater analytical results are described below. <br /> REGIONAL GEOLOGY/HYDROGEOLOGY <br /> This section was developed from the reference listed in Attachment A. The geology found in the <br /> area consists of a series of coalescing alluvial fans and plains. Low topographic relief created by <br /> headward erosion of the fan surfaces by active stream channels reaches about 10 feet. The <br /> alluvial fans contain about 100 feet of Pleistocene to Holocene age unconsolidated clay, silt, sand <br /> and gravel derived from several seasonal east-flowing streams draining the Diablo Range to the <br /> west. The alluvial fans are underlain by approximately 800 feet of Pliocene to Pleistocene age <br /> unconsolidated alluvium of the Tulare Formation. The contact between the top of the Tulare <br /> Formation and the overlying alluvial sediments is not distinguishable, because the lithology is <br /> undifferentiated. The Tulare consists of upper and lower members of mainly coarse-grained <br /> lenticular alluvium. The Tulare Formation conformably overlies the San Pablo Group marine <br /> sediments of Miocene age. <br /> Near the top of the Tulare Formation, at a depth of approximately 300 feet (elevation -150 feet <br /> above Mean Sea Level [ft MSL]), an extensive clay bed called the Corcoran Clay separates <br /> alluvial sediments into upper and lower aquifers. Near the site, the Corcoran Clay is <br /> approximately 80 feet thick. The lower aquifer is confined by the Corcoran Clay. The upper <br /> aquifer is unconfined. <br /> Recharge to the unconfined, upper aquifer in the alluvium and upper Tulare is by infiltration of <br /> water from rainfall, streams, and excess irrigation. The infiltrated water cannot permeate the <br /> Corcoran Clay and is recovered by wells drawing from the upper aquifer. The water level in the <br /> upper aquifer is at a depth of approximately 75 feet (75 ft MSL). Movement of groundwater in <br /> the aquifer is in a general northeasterly direction. The water quality is generally poor. <br /> The recharge areas for the confined, lower aquifer is along the foot hills of the Diablo Range <br /> where the Tulare Formation outcrops, and the Corcoran Clay is absent. The lower aquifer, which <br /> bears fresh water, is located at a depth of approximately 400-500 feet (-250 to -350 ft MSL). <br /> I:100061 O\.SF3 89_0339TTRZXXUTTzur30.799.wpd <br /> 10/18/99 8:28 AM <br />