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ARCHIVED REPORTS_2011_25
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ARCHIVED REPORTS_2011_25
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Last modified
7/18/2020 12:45:50 AM
Creation date
7/3/2020 10:56:22 AM
Metadata
Fields
Template:
EHD - Public
ProgramCode
4400 - Solid Waste Program
File Section
ARCHIVED REPORTS
FileName_PostFix
2011_25
RECORD_ID
PR0440005
PE
4433
FACILITY_ID
FA0004516
FACILITY_NAME
FORWARD DISPOSAL SITE
STREET_NUMBER
9999
STREET_NAME
AUSTIN
STREET_TYPE
RD
City
MANTECA
Zip
95336
APN
20106001-3, 5
CURRENT_STATUS
01
SITE_LOCATION
9999 AUSTIN RD
P_LOCATION
99
P_DISTRICT
004
QC Status
Approved
Scanner
SJGOV\rtan
Supplemental fields
FilePath
\MIGRATIONS\SW\SW_4433_PR0440005_9999 AUSTIN_2011_25.tif
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EHD - Public
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Mr. Robert McClellon <br />March 7, 2011 <br />Page 5 <br />success of this design is the GCCS. This design has been demonstrated elsewhere including <br />the unlined or clay -only lined areas of the original portions of the Forward landfill (i.e. WMUs <br />B, C, and D-87 through D-88) which contain a LFG collection system. It is our understanding <br />that probes within 50 feet of the unlined or clay -only lined areas containing a LFG collection <br />system have not shown evidence of LFG migration. These observations prove that a properly <br />installed and operating LFG collection system can control LFG migration regardless of the set- <br />back from LFG monitoring probes even in an unlined cell. <br />Historical Setback Evaluation Based on Relocation/Offset of LFG Probes <br />As discussed with Scott Walker of CalRecycle during a January 26, 2011 meeting at the <br />Landfill with you, Lewis Engineering, and Republic personnel, there are no existing <br />mathematical models that can accurately predict an appropriate LFG probe setback. It was <br />agreed at this meeting by all parties that a LFG probe setback could best be estimated by a <br />review of the past performance of LFG probes at the site relative to the proximity to the edge <br />of waste. <br />Many of the past LFG issues at the Landfill have stemmed from exceedences in Probes GP - <br />11 and GP -12 (see Figure 2). Cornerstone believes that these issues are primarily due to <br />LFG migrating under the lining system from the former unlined Austin Road Landfall. <br />Because of the nature of this LFG migration, it is difficult to evaluate the appropriate setback <br />distance based on the performance of Probes GP -11 and GP -12, and therefore no correlation <br />in this regard has been made herein. However, Probes GP -8, GP -9, and GP -10 are also <br />located near lined waste management units. To address prior EHD comments, they have been <br />relocated further from the lined cell's edge of waste to avoid detecting LFG that may be <br />expected given the proximity to the edge of waste, and therefore within the GCCS radius of <br />influence. The purpose of this is to avoid making risk management decisions based on LFG <br />data that is not indicative of what could be actually migrating from the lined landfill cell. <br />Forward originally installed Probes GP -8, GP -9, and GP -10 sometime between 2000 and <br />2002. As shown on Figure 2, Probe GP -8 is located southwest of Waste Management Unit <br />(WMU) D-01, GP -9 is located directly west of WMU D-01, and GP -10 is located northwest <br />of WMU D-02 and south of WMU FU -06. All of these probes were relocated in 2006 <br />approximately 30 feet west of their original location due to their proximity of the edge of <br />waste. The probes were relocated to avoid detecting LFG that may be expected given their <br />proximity to the edge of waste and therefore within the radius of influence of the GCCS. A <br />summary of these probes' original and current distance from the edge of waste is shown <br />below in Table 1. <br />
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