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ARCHIVED REPORTS XR0011176
Environmental Health - Public
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3500 - Local Oversight Program
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PR0544922
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ARCHIVED REPORTS XR0011176
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Last modified
10/7/2019 3:38:56 PM
Creation date
10/7/2019 3:14:34 PM
Metadata
Fields
Template:
EHD - Public
ProgramCode
3500 - Local Oversight Program
File Section
ARCHIVED REPORTS
FileName_PostFix
XR0011176
RECORD_ID
PR0544922
PE
3528
FACILITY_ID
FA0003284
FACILITY_NAME
FOOD MART GASOLINE*
STREET_NUMBER
2185
Direction
E
STREET_NAME
FREMONT
STREET_TYPE
ST
City
STOCKTON
Zip
95205
APN
14113045
CURRENT_STATUS
02
SITE_LOCATION
2185 E FREMONT ST
P_LOCATION
01
P_DISTRICT
001
QC Status
Approved
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EHD - Public
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REMEDIATION TESTING <br /> AND DESIGN March 29 , 1993 <br /> backfilled U�'T Fit The test was conducted for appro..imately 6E <br /> minutes and semi-stable vacuum influence conditions was indicated <br /> The stabilized flow rate for VW-2a was 29 scam with a vacuu-n `f 10 <br /> inches of mercury ' During this test, significant vacuum influence wa3 <br /> noted in prDbes within the UST and only -light vacuum <br /> influence in one other probe (P-5 ) Vacuum influence was noted in <br /> only one monitor well (MW- 3 ) Figure 5 is a plot of the vacuum <br /> Inf luence in the "a" zone during "a" zone extz action from VW- 2a ThIs <br /> figure shows good vacuum influence in the "a" Lone over a large part <br /> of the site Figure 6 is a plot of the vacuum influence in the "b" <br /> zone during "a„ zone e}-traction from VW-2a. This plot shows goc,d <br /> influence In the "b" zone with a 2lightly smaller areal extent than <br /> that of the "a" zone The relatively low vacuum in well Via'-2U <br /> indicates that there is a good seal between the screens of VW-2a and <br /> VW-2r) <br /> Table 4 presents VEFT field data foi extraction from well VW-2b. The <br /> general result of this test showed that vacuum extraction works well <br /> in the "b" zone and induces vapor flow within the "a" zone , from the <br /> zone near the water table and within the backfilled UST pit <br /> E:_traction from VW-2b was conducted for approximately b5 minutes and <br /> stable vacuum influence conditions were not quite achieved Llacul um <br /> and flow rate in VW-2b stabilized at 10 inches of mercury and 35 scfm <br /> respectively. Vacuum influence was noted in probes P-7 and P-8 <br /> (within the UST backfill ) at levels significantly lower that the VW-2a <br /> test A much stronger vacuum influence was measured in monitor well <br /> MW-3 and slight influence was also noted in well MW-1 Figure 7 is a <br /> plot of the vacuum influence in the "b" :one during "b" zone <br /> extraction from VW-2b This plot shows a very strong influence ever <br /> most of the site . Figure 8 is a plot of the vacuum influence in the <br /> "a" zone during "b" zone extraction from VW-2b This plat shows <br /> strong vacuum influence in the "a" zone over most of the site The <br /> center of vacuum influence in the "a" zone as shown on Figure 8 is <br /> about 20 feet west northwest of the extraction well This off- <br /> centered feature is strong evidence that the seal between the well <br /> screens of VW-2a and VW- 2b is very good. Also , vacuum influence in <br /> the "a" Lone is stronger during "b" zone extraction than during "a." <br /> zone extraction ( compare Figure 5 and Figure 8 ) . <br /> Table 5 presents VEFT field data from the vacuum flow step testing <br /> conducted in all of the vacuum extraction wells and monitor well MW-3 <br /> The results of this test show that each well is a good extraction <br /> point for use during remedial activities The "a" zone wells flowed <br /> at a slightly higher rates under equal vacuum conditions than the "b" <br /> zone wells All of the vacuum extraction wells performed <br /> significantly better than monitoring well MW-3 Figure 9 is a graph <br /> of the average flow rates versus average vacuum levels for all of the <br /> vacuum extraction wells . This graph shows a nearly, linear <br /> rElationship between flow rates and required vacuum lsvels <br /> r <br /> 4 <br />
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