
Requirements for subsurface modeling have changed substantially over the past years: the perception that limits of hydrocarbon availability are in sight has moved attention in exploration and development to more complex reservoirs; more data has become available for predicting and monitoring performance that now need to be integrated in subsurface models. Targets for (re)development have become more sophisticated and depend more critically on accurate models of geometry and actual properties. This paper attempts to analyze the requirements of ‘static’ modeling at reservoir to basin scales and simulation of dynamic subsurface behavior, covering fluid flow as well as geomechanical response to man-made changes in the subsurface.
A quick look back into methods for describing subsurface reservoirs tells us that over the past 15 years using 2-D maps as carrier of geometry and property information have been gradually replaced by 3-D reservoir models, usually built for single reservoir intervals. Maps are still an important means of documentation for securing funding and getting well plans certified, but in general are a derivative of 3-D reservoir models. The latter are now the main mechanism by which a thorough understanding of subsurface processes and their impact on hydrocarbon availability is created. As understanding of processes grew, it has become apparent that 'static reservoir properties' are not static but time-variant, being influenced by phenomena at scales greatly different from that of reservoirs. Production is affected by mechanical processes at foot scale as well as by full-field compaction responding to underburden and overburden up to surface. Large-scale models are also required when using 4D seismic data as a constraint in reservoir modeling and simulation. Effectively the phenomena to be considered for a balanced solution occur at 5 orders of magnitude. Complex or just very mature assets cannot be optimized based on single reservoir models. What is required are multi-scale, 3-D consistent representations of the subsurface - in other words we still need Shared Earth Models even though the term has become less fashionable.
Another learning has been that production data are often not accurate enough for optimizing mature fields, shifting the focus from detailed history matching to real-time measurements of the current performance and using this information for continuous optimization of asset performance. To do so one needs an evergreen model. Therefore our subsurface models should not only be comprehensive but also easily updatable.
Current reality is different though and practice in maturation teams is frequently pitched at lower levels of sophistication and integration. Sometimes for a good reason - there are indeed cases where re-development can be done well on the basis of decline curve analysis and where models or tools are of secondary importance to experience and skill. However, simple assets can become complex when aging and the number of experienced engineers capable of running a field by decline curves is getting smaller. While integration is required, practice often shows workflows where optimization occurs in single expertise areas. So what is causing this underperformance of all past integration attempts? In our opinion a significant blocker to integration has so far been overlooked; it is actually the 'heart' of all modeling packages, the so-called '3-D gridder' that determines how comprehensive models can be and how easily they can be updated.
Grid Types in Geological Modeling
Different approaches have been developed to subdivide the subsurface into cells. The simplest of all grids is the 'voxel grid' or 'sugar cube grid'; well known from storage of seismic data - a matrix of uniformly sized cells with horizontal tops and vertical sides. For capturing geological shape into such grids one would need to use fairly small cells to suppress raster artifacts that are harmful in flow simulation. All more sophisticated grid types use n general the corner points of cells to describe the subsurface geometry; properties can be stored at the cell center.
In summary, the discussed grid types all have specific strengths and weaknesses. When judged solely on capabilities with geometry handling, Pillar Grids show most fundamental limitations while s-Grids tend to be heavy, at least when it is attempted to limit inaccuracies at faults by using small cells. Faulted s-Grids are most flexible in capturing geometry: there is no need to align the grid with faults or dip, cell size can be changed - faults will always split cells exactly where they occur, even if it means splitting cells multiple times when using coarser grids. The only fundamental limitation of Faulted s-Grids lies in the representation of very steep to overturning strata.
Capabilities with Property Modeling
In more complex structures, the large variation in cell size in Pillar Grids is problematic - it may become necessary to use finer grids to assure decent property sampling in zones where pillars fan out. Faulted and unfaulted s-Grids are less suitable for storing property distributions in strata dipping more than 45 degrees while pillars can eventually be tilted to compensate the dip effect. Only SKUA grids support properties in very steep and overturning strata well.
Upscaling into Simulation Grids and Downscaling
Most grid types mentioned above are also suitable to serve as simulation grids - as far as information on SKUA Grids is available it seems that they are re-sampled into s-Grids. It must be reiterated here that simulators do not directly use these simulation grids but execute finite difference flow simulations on a so-called 'simulation matrix', in which geometrical knowledge is reduced to cell center depth, node volume and, to some degree transmissibility's as calculated from permeability and cell contact area. Upscaling and derivation of transmissibility's works best if modeling grid and simulation matrix are similar and communicate with each other in terms of integers (e.g. 3 cells in the geological grid to 1 cell in simulation grid and matrix), which is the case for all grid types except for SKUA Grids. The same holds for downscaling simulation results back into reservoir models, in order to "close the loop" between geological modeling and reservoir simulation.
Performance of Grid Types in Simulation
Through the integration of (3rd party) reservoir simulators such as provided by CMG, Faulted s-Grids (Jewel Grids) can communicate complex structure and grid properties directly to the to the reservoir simulation deck generator. This process allows for properly handling the polyhedral cells at the fault locations by computing the cell pore volumes and generating the non-neighbor connections across the fault surfaces. An important advantage of this method is consistent X and Y permeability values, resulting in more precise transmissibility calculations and reservoir simulation results.
A great number of tests have been executed that compare simulation results in identical structure and property distributions that are stored in different grid types. The Faulted s-Grids perform in simulation with equivalent speed and gave identical results to s-Grids when benchmarked in CMG's IMEX simulation engine on the (unfaulted) SPE1 and SPE10 models. A more interesting benchmark was conducted on a structurally more challenging model where the effects of grid sampling on transmissibility across faults could be evaluated more extensively. The two most common dynamic simulation grids (s-Grid, Pillar Grid) along with the Faulted s-Grids were evaluated for flow across a model using one water injector in dead oil and keeping the BHP constant with two producing wells on the other side of the faults. The model comprises of 10 intervals with alternating permeability's.
The results show that water breakthrough times are different by 50% in Pillar Grids versus the Stair Step and Faulted s-Grids. More importantly, visualization and evaluation of the results would most probably yield significantly different development and in-fill drilling planning.
In general it can be stated that simulation tests show results from s-Grids and Faulted s-Grids to be similar. Given that s-Grids are most similar in geometry to simulation matrices results from s-Grids can be assumed to be correct if they are fine enough to represent geology properly. Additional testing is currently ongoing to better understand the differences in simulation behavior.
Grid Types and Integrated Workflows
In integrated workflows, the overall performance of the Grid in iterative loops between geological modeling and reservoir simulation is by far more critical rather than its performance in individual discipline areas. The ability to utilize, analyze and interpret all of the subsurface data available in hydrocarbon assets can be greatly facilitated by newer gridding technologies and approaches that can properly deal with the range of scales associated with all data contributing to reservoir performance. Older gridding techniques were devised and implemented in computing environments that were limited in processing and visualization power. Newer application engineering techniques in conjunction with powerful and yet familiar Microsoft Windows 32 and 64 bit desktop operating systems enable new gridding capabilities that can more effectively manage the scaling challenges associated Integrated reservoir Modeling (IRM). Finally, industry leading packages such as SMT's Kingdom Suite and CMG's IMEX can easily be integrated into a IRM workflow due to the unique Jewel Grid (Faulted s-Grid) in conjunction with Microsoft .NET application engineering environment without compromising critical detail. Through the realization of the benefits of IRM, hydrocarbon assets can now be more efficiently and effectively managed in a proactive manner saving both time and cost. For additional information about JewelSuite please contact us through www.jewelsuite.com .