The impact of model complexity on CO2 saturation and mass balance

Thursday, 17 December 2015
Poster Hall (Moscone South)
Edward Mehnert1, Naum I Gershenzon2, Amir H Kohanpur3, Roland T Okwen4, Chris Patterson1, Robert William Ritzi Jr5, Albert J Valocchi6 and GSCO2, (1)Illinois State Geological Survey, Champaign, IL, United States, (2)Wright State University Main Campus, Dayton, OH, United States, (3)University of Illinois at Urbana Champaign, Dept of Civil and Environmental Engineering, Urbana, IL, United States, (4)Univ of IL, Prairie Res Instit, Champaign, IL, United States, (5)Wright State Univ, Dayton, OH, United States, (6)Univ Illinois, Urbana, IL, United States
When modeling geologic carbon sequestration, predicting the saturation of carbon dioxide (CO2) over space and time and the distribution of CO2 mass (free, trapped or dissolved) over time are primary concerns. Modeling may be done to address short-term concerns such as determining the saturation of CO2 at the end of the injection period or long-term concerns such as estimating the mass of dissolved CO2 hundreds of years after the injection period. Model complexity describes the physics included in the flow model and encompasses how simply key input data can be described-- homogeneous or heterogeneous permeability, homogeneous or heterogeneous capillary pressure, simple or hysteretic relative permeability, and simple or hysteretic capillary pressure.

Starting with a simple 3D model and building to a complex model in a stepwise manner, the effects of additional complexity on the short-term and long-term CO2 saturation and mass balance (free supercritical fluid, trapped, and dissolved) are being evaluated. Initial results suggest that the CO2 plume footprint, plume extent and mass balance vary significantly with model complexity over the short- and long-term, and that representing full complexity (i.e., heterogeneity and hysteresis in the characteristic relationships for capillary pressure and relative permeability, as they vary within the reservoir’s geologic architecture) may be critical to properly representing CO2 dynamics in some candidate reservoirs. Ultimately, we seek to demonstrate the significance of various pore-scale processes to the continuum-scale distribution of CO2.