10’ n w 2 100 v) v) w a P v) v) w A 2 0 v) 2 lo-’ w z n Ap - 1.0 psi t = 1.0 hr PO 0.28 tO/CD - 1.35 CDe2s 10.0 PI : 42.55 psig 0 PRESSURE DATA -- PRESSURE-DERIVATIVE DATA - SIMULATIONS I I I I 10-2 I lo-’ 100 10‘ 102 103 104 DIMENSIONLESS TIME GROUP, t,/C, Figure 5-108. CarperlCenozoic Alluvium Pumping Test Drawdown Log-Log Plot with INTERPRET Simulation 4.0 I I 3.0 - - n .‘ 2.0 n ,012 - MATCH PARAMETERS .zP f 10 PSI 1.0 hr PD 0 28 ’D cD 135 C,e2* 100 P’ 42 55 psig 1 .o + DATA - SIMULATION 0.0 -1.0 I I 0.0 1 .o 2.0 DIMENSIONLESS SUPERPOSITION FUNCTION: FLOW PERIOD 1 Figure 5109. Carper/Cenozoic Alluvium Pumping Test Drawdown Dimensionless Homer Plot 130 with INTERPRET Simulation
6. DISCUSSION OF RUSTLER FLOW SYSTEM The single-well testing discussed in this report has provided significant information on the transmissivities and hydraulic-head relations <strong>of</strong> the five Rustler members. In particular, our knowledge <strong>of</strong> the distribution <strong>of</strong> transmissivity within the Culebra dolomite has increased considerably. Section 6.1 attempts to explain the distribution <strong>of</strong> Culebra transmissivity in the context <strong>of</strong> geologic models <strong>of</strong> halite deposition and dissolution within the Rustler Formation. Recent hydraulic-head measurements made at H-3d, H-14, H-16, and DOE-2 have helped to increase our understanding <strong>of</strong> the directions <strong>of</strong> potential vertical fluid movement within the Rustler. Section 6.2 discusses the hydraulic-head relations among the Rustler members, and their implications regarding recharge to the Rustler Formation. 6.1 Culebra Transmissivity Mercer (1 983) reported values for Culebra transmissivity at 20 locations. The testing described in this report has provided values for Culebra transmissivity at 15 new locations, and new estimates at 7 locations for which values had previously been reported. Combined with other recent work performed at DOE-2 (<strong>Beauheim</strong>, 1986), H-3 (<strong>Beauheim</strong>, <strong>1987</strong>a), H-11 (Saulnier, <strong>1987</strong>), and WIPP- 13 (<strong>Beauheim</strong>, <strong>1987</strong>b), the WlPP project has tested the Culebra at 38 locations. Figure 6-1 shows these 38 locations and the transmissivity values at each provided by this report or those referenced above. Figure 6-2 shows the areas around the WlPP site where halite is present in the non-dolomite Rustler members, as indicated by Snyder (1985 and personal communication) and Powers (personal communication). According to Snyder, halite was originally deposited in the unnamed lower, Tamarisk, and Forty-niner Members <strong>of</strong> the Rustler over the entire area covered by Figure 6-2. The present-day absence <strong>of</strong> halite from these members reflects the eastward progression <strong>of</strong> a dissolution front. This dissolution front apparently affects the uppermost Rustler halite, that in the Forty-niner, first, and works progressively downsection to the upper Salado Formation. Thus, the eastwarc extent o e Fortyniner dissolution front is greater than that <strong>of</strong> the Tamarisk dissolution front, which is in turn greater than the eastward extent <strong>of</strong> the dissolution front in the unnamed lower member (Figure 6-2). Dissolution <strong>of</strong> the upper Salado follows dissolution <strong>of</strong> halite from the unnamed lower member <strong>of</strong> the Rustler. Lagging behind the dissolution front in each member is a second front where anhydrite is being hydrated to gypsum. In Snyder’s view, as halite is removed beneath the Rustler dolomites, the dolomites subside and fracture. Similar subsidence and fracturing may affect the anhydrites, allowing more groundwater flow through them which may effect their hydration to gypsum. Note that the areas shown on Figure 6-2 indicate only that some halite is present in the appropriate members, not that the full thicknesses originally deposited are present. For example, Snyder (1985) states that only about half <strong>of</strong> the halite originally present in the unnamed lower member at WIPP-21 is there today. Alternatively, Holt and Powers (1988) believe that the different amounts <strong>of</strong> halite seen in the Rustler members at the WlPP site more likely represent original depositional differences and/or syndepositional dissolution than later progressive dissolution. They relate fracturing to stress relief caused by unloading <strong>of</strong> the Rustler, citing a preponderance <strong>of</strong> horizontal (as opposed to vertical) fractures within the Rustler as evidence. According to their hypothesis, fracturing would be expected to become less pronounced eastward as the depth <strong>of</strong> burial <strong>of</strong> the Rustler increases. Holt and Powers (1988) also do not believe that all <strong>of</strong> the gypsum present in the Rustler is related to the hydration <strong>of</strong> anhydrite, but that it is instead primary, pointing to the presenration <strong>of</strong> primary sedimentary structures as evidence. Holt and Powers do find evidence for latestage dissolution <strong>of</strong> halite from the upper Salado in Nash Draw, however, and relate disruption <strong>of</strong> the overlying Rustler to this dissolution. As can be seen on Figure 6-2, the highest values <strong>of</strong> Culebra transmissivity are found in areas in or close 131
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SANDIA REPORT SAND87 -0039 UC - 70
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SAND87-0039 Unlimited Release Print
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a transmissivity of about 7 x 10-2
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5 . TEST OBJECTIVES AND INTERPRETAT
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3-18 3-19 3-20 3-21 3-22 3-23 3-24
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5-35 H-l5/Culebra Drillstem and Slu
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5-78 5-79 5-80 5-81 5-82 5-83 5-84
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A-2 A-3 A4 A-5 A-6 Single-Porosity
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'H-6 o DOE-2 OHIPP-13 OAIPP 12 OH-1
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WlPP site. The aggregate thickness
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deep. The gamma-ray log used to gui
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3347.11 ft \ - -12.25-inch HOLE -8.
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~ 3409.6 n __ - - HOLOCENE DEPOSITS
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Ylf M (t -1wt 5 n nch REAMED BOREHO
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3418.96 n 7.875-inch REAMED BOREHOL
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2.375-inch TUBING 4.5-inch. 9.5 Ibl
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WELL CASING 2.375-inch TUBING TEST-
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1.5-Inch GALVANIZED PIPE WELL CASIN
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I I I I PRE-TEST STATIC PRESSURE i/
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(or areal extent) of the aquifer on
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:7001 J EQUILIBRATION / r.. .......
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Once straddle tests proved impossib
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1300 c - J PRE-TEST PRESSURE IN TES
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- < a m L: * m 3 L a I Start Date:
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uildups were caused by the natural
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TABLE 5-1 EFFECTIVE DST FLOW RATES
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TABLE 5-2 SUMMARY OF NON-CULEBRA SI
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simulation shown, however, uses a t
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1 .o 0.9 0.8 p' = 79.08 paig pi = 6
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~ ~~ TABLE 5-3 SUMMARY OF CULEBRA S
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Two factors raised questions about
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102 I I 1 1 1 W K 3 v) v) W K n v)
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5.2.2.21 below) and DOE-2 (Beauheim
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..A 225 - PRESSURE ABOVE TEST INTER
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10' n ui K 3 v) v) W a n v) v) 100
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10' MATCH PARAMETERS O n w a 3 v) v
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..CI__._._..__....__.I 5.2.2.6 H-15
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8.0 1 I I I MATCH PARAMETERS AP 1.0
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- 200 150 5 - EQUILIBRATION \Feu 'S
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- Page 138 and 139: 7. SUMMARY AND CONCLUSIONS Single-w
- Page 140 and 141: REFERENCES Bachman, G.O. 1984. Regi
- Page 142 and 143: INTERA Technologies, Inc. 1986. WlP
- Page 144 and 145: Stensrud, W.A.; Bame, M.A.; Lantr,
- Page 146 and 147: (A-4)
- Page 148 and 149: distinct value of Coe2s. Pressure-d
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- Page 152 and 153: where: n = number of normal sets of
- Page 154 and 155: (A-21) and for spherical blocks the
- Page 156 and 157: where: tp* = Vfq, V = total flow pr
- Page 158 and 159: Figure A-5. Semilog Slug-Test Type
- Page 160 and 161: A.4 INTERPRET WELL-TEST INTERPRETAT
- Page 162 and 163: DISTRIBUTION: U. S. Department of E
- Page 164 and 165: INTERA Technologies, Inc. (9) 6580
- Page 166 and 167: WlPP Public Reading Room Carlsbad M
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