The [[karst]]-collapse model describes a [[touching vug]] pore system that is formed by massive dissolution of carbonate resulting from [[meteoric groundwater]] flow and subsequent collapse and filling of caverns ([[:file:carbonate-reservoir-models-facies-diagenesis-and-flow-characterization_fig4.png|Figure 4]]). This process is independent of the sediment's original environment of deposition. Most karsted carbonates are thought to be related to major dissolution concentrated in the [[vadose]] and upper [[phreatic]] zones producing a horizontality to the caverns. Cavern geometry is also controlled by fracture orientation, often resulting in caverns with linear trends. | The [[karst]]-collapse model describes a [[touching vug]] pore system that is formed by massive dissolution of carbonate resulting from [[meteoric groundwater]] flow and subsequent collapse and filling of caverns ([[:file:carbonate-reservoir-models-facies-diagenesis-and-flow-characterization_fig4.png|Figure 4]]). This process is independent of the sediment's original environment of deposition. Most karsted carbonates are thought to be related to major dissolution concentrated in the [[vadose]] and upper [[phreatic]] zones producing a horizontality to the caverns. Cavern geometry is also controlled by fracture orientation, often resulting in caverns with linear trends. |