The Sequence Stratigraphy of the Maastrichtian (Upper Cretaceous)
Reservoir
at Wafra field, Partitioned Neutral Zone,
Saudi Arabia and Kuwait: Key to
Reservoir
Modeling and Assessment
Dennis W. Dull, Raymond A. Garber, and W. Scott Meddaugh
Chevron Energy Technology Company, Houston, TX
The Maastrichtian (Upper Cretaceous)
reservoir
is one of five prolific oil reservoirs in the giant Wafra oil field. Although discovered and first produced in 1959, the
reservoir
is currently in early development because of its low but variable oil gravity, high sulfur content, relatively high water-cut, and apparent compartmentalization made it a much less attractive resource than other productive intervals at Wafra field. Less than 1 percent of the OOIP in the Maastrichtian has been produced. This study was undertaken to (1) determine
reservoir
volumetrics, (2) understand the areal and stratigraphic distribution of intervals likely to yield higher volumes of better
quality
oil, and (3) provide a
reservoir
property model for use in fluid flow simulation.
The key to modeling the
reservoir
was the construction of an appropriately detailed sequence stratigraphic framework for use in building a geostatistical
reservoir
model with high
quality
descriptions from five cored wells in the
reservoir
. The Maastrichtian
reservoir
was deposited during an initial transgressive phase (TST) that evolved into a high stand (HST). Within this sequence stratigraphic framework, ten high frequency sequences (HFS) could be correlated, albeit with some difficulty, across the entire field.
The geostatistical model of the Maastrichtian
reservoir
demonstrates the layered and compartmentalized nature of the
reservoir
and clearly shows that the location of the
reservoir
facies within the Maastrichtian is controlled by the original depositional fabric and subsequent dolomitization, both of which have been influenced by the paleotopography. Such understanding is critical to efficiently develop the 1.5 billion barrel oil Maastricthian resource at Wafra field.