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CORRESPONDENCE_*2022
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CORRESPONDENCE_*2022
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Last modified
6/24/2022 8:57:36 AM
Creation date
5/23/2022 2:26:47 PM
Metadata
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EHD - Public
ProgramCode
4400 - Solid Waste Program
File Section
CORRESPONDENCE
FileName_PostFix
*2022
RECORD_ID
PR0504901
PE
1635
FACILITY_ID
FA0006395
FACILITY_NAME
MARISCOS COSTA ALEGRE #4Z77195
STREET_NUMBER
2440
Direction
S
STREET_NAME
AIRPORT
STREET_TYPE
WAY
City
STOCKTON
Zip
95206
APN
16913327
CURRENT_STATUS
02
SITE_LOCATION
2440 S AIRPORT WAY
P_LOCATION
01
P_DISTRICT
001
QC Status
Approved
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SJGOV\cfield
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EHD - Public
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underlying layer of dry soil as shown in Fig. 6b. Around 66–67 m, <br />there was a downward progression of different resistivity zones <br />(1000–2500 Xm, then 250–530 Xm, and 530–1100 Xm) which <br />TP6 on AL1 revealed as demolition waste close to the surface, fol- <br />lowed by a gentle progression of semi-wet to dry soil as shown <br />in Fig. 6c. However,Fig. 5b also revealed a structure between 28 <br />and 44 m along the line, with resistivity similar to that of exca- <br />vated demolition waste. In this case, it was clearly not demolition <br />waste but a part of the geological formation of the area, as evi- <br />denced by a similar structure underlying the dump in Fig. 5a. This <br />was further revealed by TP9 at 40–42 m on AL2 (Fig. 5b) as compact <br />and dry soil similar to the one in Fig. 6h. <br />Glass hotspots were expected to be in the dark orange to dark <br />red zones (>8000 Xm). There were a number of such zones on all <br />three lines in Fig. 5.OnAL1 (Fig. 5a), three TPs were excavated <br />between 11 and 15 m (TP1), 23–25 m (TP2) and 43–45 m (TP4) <br />and all revealed glass, although it was more abundant at 23– <br />25 m and 43–45 m (Fig. 6d). As such, these two regions were <br />identified as hotspots from which materials for physico- <br />chemical characterisation were sampled as samples S1 and S2 <br />respectively. Although the region between 11 and 15 m was also <br />a glass hotspot, it was not sampled but glass abundance was visu- <br />ally qualified based on amounts of other waste fractions seen <br />during excavations. On AL2 (Fig. 5b), a TP between 13 and 18 m <br />(TP7) also showed abundant glass waste as shown in Fig. 6e. <br />The region around 4–10 m in Fig. 5b clearly contained abundant <br />glass also as could be seen from the surface, but a verification TP <br />could not be excavated since the region was sloppy with unstable <br />ground, and thus unsafe for the excavator. Similarly, there was <br />abundant glass on the surface around 29–34 m in Fig. 5b, and <br />therefore the highly resistive region beneath was designated as <br />a hotspot. Materials for physico-chemical characterisation were <br />thus sampled from the regions between 13 and 18 m and 29– <br />31 m in Fig. 5b (sample S3). On AL3 (Fig. 5c), TP12 was excavated <br />at 14–16 m which was another glass hotspot and was thus sam- <br />pled as S4. <br />It was noted, however, that the bedrock around the dump <br />showed resistivity similar to some dumped materials. In Fig. 5b, <br />for instance, resistivity >8000 Xm is progressively registered in <br />the region around 0–34 m and between 10 and 15 m depths. A <br />TP excavated at 26–28 m (TP8) and 1–2 m depths revealed big <br />stones (Fig. 6f) with an underlying bigger rock which the excavator <br />could not remove. It was thus concluded that the bedrock was <br />responsible for resistivity zones >8000 Xm other than glass hot- <br />spots. Alsterfors site has granite bedrock with a moraine soil depth <br />of 3–10 m (SGU, 2019). Granite and soda-lime glass have similar <br />Fig. 4.Madesjö glass dump; (a) demolition waste heap at the start of ML1; (b) start of ML2 near the stream; (c) TP excavations across the dump. <br />R.N. Mutafela et al./Waste Management 106 (2020) 213–225 219
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