FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2005444709> ?p ?o ?g. }

• W2005444709 abstract "SPE Members Abstract This paper discusses a new approach for interpreting the effect of pore pressure on the conductivity and permeability of artificially fractured rocks. The mathematical model formulated includes the non-linear effect of pressure dependence of fracture conductivity and formation permeability through a modified concept of fracture conductivity. New type curves for pressure-sensitive fracture formation systems were generated and a method of pressure analysis to interpret this effect is provided. The pressure behavior of wells intercepting pressure-sensitive finite conductivity fractures was investigated by solving numerically the non-linear mathematical model. A conductivity modulus in the fracture (fD) and a permeability modulus in the formation (D) determine the intensity of the pore pressure effect. Results of our investigation demonstrate that when the fracture conductivity is pressure dependent, the use of conventional techniques to evaluate fractured wells may lead to incorrect estimates of the fracture-formation properties. The slope of the pseudo-bilinear flow period () becomes function of CfD and fD, ranging from 0.25 to 0.35. The interpretation of pressure data is carried out through a graph of p vs t . However the pore pressure effect has no influence on the one-half slope of the linear flow. A novel correlation to detect the approximate time and pressure when the fracture closure occurs is presented. Equations relating the pseudo-bilinear slope with CfD and fD were obtained by using multivariate non-linear regression analysis. The expressions facilitate the analysis of well-test data and detect the pore pressure effect on conductivity. Introduction Conductivity and permeability of porous media are known to depend on pore pressure and/or stress field. The pore pressure dependency of conductivity is even stronger in fractured porous media, particularly on artificially fractured formations. As pore pressure declines, deformations on the proppant material-fracturing fluids-porous media make the conductivity of the fractured system to become quite sensitive to pore-pressure. Mathematically this phenomenon constitutes a non-linear problem. An approach used to solve this non-linear problem is the use of transformations to linearize the modeling equations. A modified form of Kirchoff transformation has been extensively used to formulate the non-linear problem. However, this approach presents the disadvantage of the requirement of extensive experimental data of permeability-pore pressure. An important result of the experimental work on pressure and stress dependence of porosity and permeability published in the literature, is that the rock permeability or conductivity behaves in an exponential manner with the pore pressure variation. The same variation has been found for the porosity, but the magnitude of the pressure dependence of porosity is considerably lower than it is for permeability. Experimental results on permeable rocks have shown that permeability is a function of both the confining pressure and pore pressure. P. 445" @default.
• W2005444709 created "2016-06-24" @default.
• W2005444709 creator A5007337733 @default.
• W2005444709 creator A5048674878 @default.
• W2005444709 date "1996-05-22" @default.
• W2005444709 modified "2023-10-18" @default.
• W2005444709 title "Effect of Pore Pressure on Conductivity and Permeability of Fractured Rocks" @default.
• W2005444709 doi "https://doi.org/10.2118/35694-ms" @default.
• W2005444709 hasPublicationYear "1996" @default.
• W2005444709 type Work @default.
• W2005444709 sameAs 2005444709 @default.
• W2005444709 citedByCount "11" @default.
• W2005444709 countsByYear W20054447092014 @default.
• W2005444709 countsByYear W20054447092015 @default.
• W2005444709 countsByYear W20054447092017 @default.
• W2005444709 countsByYear W20054447092018 @default.
• W2005444709 crossrefType "proceedings-article" @default.
• W2005444709 hasAuthorship W2005444709A5007337733 @default.
• W2005444709 hasAuthorship W2005444709A5048674878 @default.
• W2005444709 hasConcept C102579867 @default.
• W2005444709 hasConcept C120882062 @default.
• W2005444709 hasConcept C121332964 @default.
• W2005444709 hasConcept C127313418 @default.
• W2005444709 hasConcept C131540310 @default.
• W2005444709 hasConcept C147789679 @default.
• W2005444709 hasConcept C159390177 @default.
• W2005444709 hasConcept C159750122 @default.
• W2005444709 hasConcept C185592680 @default.
• W2005444709 hasConcept C187320778 @default.
• W2005444709 hasConcept C192562407 @default.
• W2005444709 hasConcept C41625074 @default.
• W2005444709 hasConcept C43369102 @default.
• W2005444709 hasConcept C55493867 @default.
• W2005444709 hasConcept C57879066 @default.
• W2005444709 hasConcept C63184880 @default.
• W2005444709 hasConceptScore W2005444709C102579867 @default.
• W2005444709 hasConceptScore W2005444709C120882062 @default.
• W2005444709 hasConceptScore W2005444709C121332964 @default.
• W2005444709 hasConceptScore W2005444709C127313418 @default.
• W2005444709 hasConceptScore W2005444709C131540310 @default.
• W2005444709 hasConceptScore W2005444709C147789679 @default.
• W2005444709 hasConceptScore W2005444709C159390177 @default.
• W2005444709 hasConceptScore W2005444709C159750122 @default.
• W2005444709 hasConceptScore W2005444709C185592680 @default.
• W2005444709 hasConceptScore W2005444709C187320778 @default.
• W2005444709 hasConceptScore W2005444709C192562407 @default.
• W2005444709 hasConceptScore W2005444709C41625074 @default.
• W2005444709 hasConceptScore W2005444709C43369102 @default.
• W2005444709 hasConceptScore W2005444709C55493867 @default.
• W2005444709 hasConceptScore W2005444709C57879066 @default.
• W2005444709 hasConceptScore W2005444709C63184880 @default.
• W2005444709 hasLocation W20054447091 @default.
• W2005444709 hasOpenAccess W2005444709 @default.
• W2005444709 hasPrimaryLocation W20054447091 @default.
• W2005444709 hasRelatedWork W2017552158 @default.
• W2005444709 hasRelatedWork W2043638266 @default.
• W2005444709 hasRelatedWork W2051310431 @default.
• W2005444709 hasRelatedWork W2242450858 @default.
• W2005444709 hasRelatedWork W2263373129 @default.
• W2005444709 hasRelatedWork W2625835519 @default.
• W2005444709 hasRelatedWork W3041140742 @default.
• W2005444709 hasRelatedWork W3202676940 @default.
• W2005444709 hasRelatedWork W47837499 @default.
• W2005444709 hasRelatedWork W796889711 @default.
• W2005444709 isParatext "false" @default.
• W2005444709 isRetracted "false" @default.
• W2005444709 magId "2005444709" @default.
• W2005444709 workType "article" @default.