Estimation of hydrocarbon reserves is governed by natural, technological and economic factors. Re-estimations and reviews continue almost till the end of exploitation in many instances. Estimation of oil reserves, when a field is in its initial stages of development is a relatively easy task. The estimation will not invite critical or close scrutiny, as the oil production at that stage is far lower than the reserves calculated. However as the field matures and the cumulative oil production approaches the estimated value of reserves, the accuracy in the estimation of reserves becomes crucial and more important. Also the estimation process itself is a challenging task, in the light of uncovering geological complexities and reservoir dynamics during the development and the exploitation methods employed to produce the oil.
Bahrain field, the first discovery in the Arabian Gulf region, has been on production since 1933. It is a multi-stacked field with 16 oil and 4 gas reservoirs. Most of them are carbonate reservoirs. The nature of the fluids varies from tarry oil in the Aruma formation occurring at shallow depths to dry gas in the deep Khuff zones.
The geology of the field is complex with a large number of faults on the structure. The major oil zone Mauddud - an oil wet system -has been on gas injection from 1938. The gas injection has lead to the transfer of oil and gas into layers above and below through the faults. Though many reservoirs of the field have reached mature stage, there are some zones containing oil resources still unexploited due to the heterogeneities, complex nature of the fluid distribution, unfavorable rock-fluid characteristics, compartmentalization, thin oil rim overlain by gas and underlain by water, etc.
This paper brings out the challenges posed by the above situations while attempting to estimate and classify oil reserves.
Introduction
Bahrain field, discovered in 1932, has 16 oil reservoirs and 4 gas reservoirs (Figure: 1).1,2 The fluid content of the reservoirs vary from the tarry oil in Aruma to dry gas in the Khuff and pre-Khuff zones (Figure: 2). Most of the above reservoirs are carbonates and some of them are clastics. The carbonates of the Cretaceous have shale limestone sequences, while the Jurassic and Precambrian Khuff have dolomitic limestone embedded in anhydrites. Based on the depth of occurrence, the oil reservoirs have been separated into three groups. The shallow zones are the zones from Aruma to Ab, which are poor producers in general. The middle zones comprise of the Wara sand Ac, the major oil producer -Mauddud limestone and the Nahr Umr sands. These are prolific reservoirs and are known as Bahrain zones. The remaining deeper reservoirs, Kharaib, Arab zones and Fadhili are termed as Deep zones, which have moderate productivity.
The geology of the field is extremely complex with a large number of faults, especially in the shallow and Bahrain zones. Also some reservoirs are fractured. In a single field, there are large variations in the rock properties and the fluid properties. This makes the work of estimating and classifying the oil reserves a challenging task.