In early 2001, Terra Nova is expected to start production at an average rate of 115,000 barrels of oil per day. Terra Nova oil pool is the second largest oil pool discovered in the Grand Banks of the Canadian East Coast. As a part of the oil recovery process optimization effort, miscibility conditions were evaluated using different techniques, for Terra Nova oil with various gas streams available from the offshore production facilities.
The techniques used consisted of the conventional slim-tube test, the rising bubble apparatus and the recently developed Vanishing Interfacial Tension (VIT)technique. In addition, published correlations were also used in estimating minimum miscibility pressures. This paper presents the results of these experimental studies and compares them with predictions from correlations as well as with visual evidence of miscibility.
The VIT technique is based on the fundamental definition of miscibility as the point at which the interface between gas and oil vanishes or the interfacial tension diminishes to zero. A computerized drop shape analysis technique was used to determine gas-oil interfacial tensions.The miscibility pressures obtained from the new VIT technique were 3-5% higher than those from visual observations and agreed well with the slim-tube results as well as with the correlations, at enrichment levels greater than 30 mole% C 2+ in the injected gas stream. The rising bubble apparatus yielded significantly higher MMPs. This study demonstrates that the VIT technique is rapid, reproducible and quantitative in addition to providing visual evidence of gas-oil miscibility.