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undertake a systematic study of fluid transport in diatomite; it appears that capillary driven flow
is relevant to reservoir flow processes. For diatomite, a clear understanding of the relationship
between pore structure, reservoir architecture, rock wettability, and oil recovery remains to be
developed. This is a monumental task and beyond the scope of this paper. Nevertheless, we
have begun by examining flow in clean, well-characterized rock samples. Our main focus is the
design of a novel CT monitorable imbibition cell and the study of multidimensional
spontaneous imbibition of water. We examine water-air and water-oil systems. Results are best
understood by considering jointly rock characteristics such as pore-size distribution, the
wetting-phase occupancy of pore space, and permeability.
Before describing our pore-level and core-level rock characterization procedures,
experimental imbibition apparatus, and results, we briefly discuss the mineralogy and
depositional environment of diatomite. Then theory regarding imbibition is reviewed to put
experimental results into context and simplify the discussion to follow.
Diatomite
Diatomite is a hydrous form of silica or opal composed of the depositional, consolidated
skeletal remains of colonies of unicellular aquatic plankton (Stosur and David 1971). Rock
color and texture bear resemblance to chalk, but diatomite contains virtually no carbonaceous
material. The mineral composition is primarily biogenic silica, detritus, and shale. Depending
on depth and composition, the silica may exist as Opal-A, Opal-CT, or Brown Shale (Schwartz
1988). Generally, amorphous silica is found at the shallowest depths. Diatomite is characterized
by permeabilities ranging from about 0.1 to 10 mD that result from a complex small diameter
pore network. Curiously, this low permeability occurs with a very high porosity that varies from
35 to 65%. The permeability versus porosity relationship indicates that this rock is different
from sandstone in pore-level characteristics. Mechanically, it is described as brittle and friable
(Wendel et al. 1988; Chase and Dietrich 1989). This aspect poses a problem when coring
samples for laboratory analysis.
In the San Joaquin Valley, California, diatomite is the uppermost productive member of
the Monterey formation. Initial oil saturations vary from 30 to 65% and total oil accumulations
in diatomite are estimated to be at least 10 to 12 billion barrels original oil in place (Ilderton et
al. 1996). Oil-bearing diatomite layers are interbedded among shale and mudstone layers
(Schwartz 1988). Individual layers vary in thickness from a few centimeters to several meters
and the gross thickness of these layers can exceed 330 m (1000 ft). The interbedding of
diatomaceous rock and shale resulted from cyclic/seasonal deposition of diatoms, mud, and silt
and the subsequent consolidation of diatom fragments and grains of mud/silt (Schwartz 1988).
Thus, the quality of diatomite varies from layer to layer and field to field. In some cases,
diatomite has a matrix that is almost entirely biogenic silica containing very little clay and is
probably water wet. In others, clay content can be relatively high and might contribute to
mixed-wettability of the rock. As described later, we choose to begin with and characterize
relatively clean diatomite.
In addition to natural fractures that may be cemented or uncemented, wells in diatomite
are hydraulically fractured to improve well productivity and injectivity. Induced fractures are
massive with heights on the order of 100 m and total lengths of roughly the same magnitude
(Ilderton et al. 1996). Such fractures are used for water (Patzek 1992) and steam injection
(Kovscek et al. 1996 a and b), as well as production.