--> Predicting the Distribution of Porosity, Pore System Characteristics and Permeability from Openhole Log Datasets: Applications to Rock Typing in the Thamama Reservoir Zones, Haliba Field, UAE
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AAPG Middle East Region Geoscience Technology Workshop:
3rd Edition Carbonate Reservoirs of the Middle East

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Previous HitPredictingNext Hit the Distribution of Previous HitPorosityNext Hit, Pore System Characteristics and Permeability from Openhole Log Datasets: Applications to Rock Typing in the Thamama Previous HitReservoirNext Hit Zones, Haliba Field, UAE

Abstract

Rock types are the building blocks of Previous HitreservoirNext Hit models, and, as such, they must capture the key geological and Previous HitreservoirNext Hit quality variability, and be populated throughout a Previous HitreservoirNext Hit using standard subsurface datasets. Rock-typing studies often utilise openhole log or core data to define rock types, however, the key pre-requisites for a successful rock-typing scheme are rarely achieved unless both datasets are fully integrated. In this research and development study, geological and Previous HitreservoirNext Hit quality understanding, gained from detailed core and thin-section observations and laboratory-based petrophysical data, are integrated with openhole log data to define Previous HitreservoirNext Hit rock types (RRTs) in the Thamama Previous HitreservoirNext Hit zones in the Haliba Field. The RRTs honour the geological variability and provide an understanding of the distribution of Previous HitporosityNext Hit and permeability from standard subsurface data alone, therefore fulfilling the key requirements of a rock-typing scheme. Standard petrophysical parameters are calculated from the openhole logs and calibrated with core data, namely the Previous HitporosityNext Hit and permeability values, in seven wells. Log Previous HitporosityNext Hit, which is calculated from the neutron-density equation, strongly correlates with core Previous HitporosityNext Hit, indicating that the openhole logs are comparable in each well across the field, and that Previous HitporosityNext Hit can be confidently predicted in uncored wells from the logs. Young's Modulus also strongly correlates with core Previous HitporosityNext Hit, and is therefore useful for the same purpose. At high porosities, low Sxo values correspond to high core permeabilities (>10mD), whereas higher Sxo values tend to relate to lower core permeabilities. Log permeability, calculated using Sxo in the Coates equation, is also positively correlated with core permeability, particularly in hydrocarbon-bearing intervals.Lastly, high Young's Modulus values at a given Previous HitporosityNext Hit typically correspond to macropore-dominated pore systems with high core permeabilities, whereas low Young's Modulus values at the same Previous HitporosityNext Hit are associated with micropore-dominated pore systems. These relationships, relating openhole log data to core Previous HitporosityNext Hit and permeability, are used to define core Previous HitporosityNext Hit and permeability clusters from the openhole logs, which are called petrophysical rock types (PRTs). 34 PRTs are defined and categorised into 10 PRT clusters, according to their core Previous HitporosityNext Hit and permeability values, each cluster is characterised by a unique Previous HitporosityNext Hit and/or permeability range. Core-based geological rock types, which are defined according to pore systems characteristics from core, thin-section and laboratory-based petrophysical data, are then integrated to refine the clusters into 11 RRTs. Each RRT has a distinctive Previous HitporosityNext Hit and/or permeability range and is characterised by a particular pore system. The RRTs are populated in all wells using standard openhole log data, and thereby provide a prediction of the distribution of Previous HitreservoirNext Hit quality throughout the Thamama Previous HitreservoirTop intervals.study. The obtained results are valuable information to further rock physics modelling and well placement.