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Chapter 16



                   Modeling Reservoir Architecture



             Reservoir architecture is modeled by contouring and digitizing geologic
        maps. The mapping/contouring process is the point where the geological and
        geophysical interpretations have their greatest impact on the final representation
        of the reservoir. This process has been discussed by several authors, including
        Harpole [1985], Harris [1975], and Tearpock and Bischke [1991]. Methods for
        numerically representing reservoir architecture are discussed  in this chapter,


                                16.1  Mapping

             The different  parameters that must be digitized for use in a grid include
        elevations or structure tops, permeability in three orthogonal directions, porosity,
        gross thickness, net to gross thickness, and where appropriate, descriptions of
        faults,  fractures, and aquifers. The resulting maps are digitized by overlaying
        a grid on the maps and reading a value for each gridblock. The digitizing process
        is sketched in Figures  16-la through 16-Id.
             The resolution of the model depends on the resolution of the grid. A fine
        grid divides the reservoir into many small gridblocks. It gives the most accurate
        numerical representation, but has the greatest computational expense. A coarse
        grid has fewer gridblocks, but the coarse gridblocks must be larger than the fine
        gridblocks to cover the same model volume. As a result, the coarse grid is less
        expensive to run than a fine grid, but it is also less accurate numerically. The
        loss of accuracy is most evident when a coarse grid is used to model the interface
       between phases such a fluid contacts and displacement  fronts.  Thus, fine grid

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