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- W2024215360 abstract "Abstract Sequence stratigraphy provides a predictive approach to potential porosity occurrence in subsurface carbonate rocks. This model predicts that most porosity within platform portions of depositional sequences results from meteoric dissolution accompanying subaerial exposure during sea-level lowstands. Porosity that may develop as a consequence of dolomitization during either sea-level highstands or lowstands, and preservation of primary depositional porosity, also are predicted by sequence stratigraphic concepts. To test the limitations of this model, the diagenesis of hydrocarbon reservoirs in Lower Permian periplatform carbonates in the Permian Basin is described in terms of porosity evolution within the framework of their burial depth histories. In some cases, porosity development in these carbonates was inherently related to sequence stratigraphy in that: (1) in limestones, it was inherited from meteoric dissolution on the platform prior to redeposition, or (2) it developed during dolomitization soon after sediment redeposition into periplatform settings. However, porosity formation via dissolution in both periplatform limestone and dolomite reservoirs also is a common mesogenetic (intermediate and deep-burial) phenomenon which operates long after redeposition. Dissolution in these cases is believed to record the expulsion of acidic fluids from hydrocarbon source rocks. Hence, porosity formation is neither temporally nor spatially related to sequence stratigraphy, and can not be predicted by this model." @default.
- W2024215360 created "2016-06-24" @default.
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- W2024215360 date "1994-09-01" @default.
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- W2024215360 title "Diagenesis in a sequence-stratigraphic setting: porosity evolution in periplatform carbonate reservoirs, Permian Basin, Texas and New Mexico" @default.
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- W2024215360 doi "https://doi.org/10.1016/0920-4105(94)90049-3" @default.
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