FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2309061770> ?p ?o ?g. }

• W2309061770 abstract "Abstract Shale gas resources have received great attention in the last decade due to the decline of the conventional gas resources. Unlike conventional gas reservoirs, the gas flow in shale formations involves complex processes with many mechanisms such as Knudsen diffusion, slip flow (Klinkenberg effect), gas adsorption and desorption, strong rock-fluid interaction, etc. Shale formations are characterized by the tiny porosity and extremely low-permeability such that the Darcy equation may no longer be valid. Therefore, the Darcy equation needs to be revised through the permeability factor by introducing the apparent permeability. With respect to the rock formations, several studies have shown the existence of anisotropy in shale reservoirs, which is an essential feature that has been established as a consequence of the different geological processes over long period of time. Anisotropy of hydraulic properties of subsurface rock formations plays a significant role in dictating the direction of fluid flow. The direction of fluid flow is not only dependent on the direction of pressure gradient, but it also depends on the principal directions of anisotropy. Therefore, it is very important to take into consideration anisotropy when modeling gas flow in shale reservoirs. In this work, the gas flow mechanisms as mentioned earlier together with anisotropy are incorporated into the dual-porosity dual-permeability model through the full-tensor apparent permeability. We employ the multipoint flux approximation (MPFA) method to handle the full-tensor apparent permeability. We combine MPFA method with the experimenting pressure field approach, i.e., a newly developed technique that enables us to solve the global problem by breaking it into a multitude of local problems. This approach generates a set of predefined pressure fields in the solution domain in such a way that the undetermined coefficients are calculated from these pressure fields. In other words, the matrix of coefficients is constructed automatically within the solver. We ran a numerical model with different scenarios of anisotropy orientations and compared the results with the isotropic model in order to show the differences between them. We investigated the effect of anisotropy in both the matrix and fracture systems. The numerical results show anisotropy plays a crucial role in dictating the pressure fields as well as the gas flow streamlines. Furthermore, the numerical results clearly show the effects of anisotropy on the production rate and cumulative production. Incorporating anisotropy together with gas flow mechanisms in shale formations into the reservoir model is essential particularly for predicting maximum gas production from shale reservoirs." @default.
• W2309061770 created "2016-06-24" @default.
• W2309061770 creator A5014709706 @default.
• W2309061770 creator A5026966481 @default.
• W2309061770 creator A5047861147 @default.
• W2309061770 creator A5057212913 @default.
• W2309061770 creator A5081205740 @default.
• W2309061770 date "2015-11-09" @default.
• W2309061770 modified "2023-10-06" @default.
• W2309061770 title "Numerical Simulation of Natural Gas Flow in Anisotropic Shale Reservoirs" @default.
• W2309061770 cites W1530030810 @default.
• W2309061770 cites W1545095299 @default.
• W2309061770 cites W17416848 @default.
• W2309061770 cites W1778213744 @default.
• W2309061770 cites W1966799339 @default.
• W2309061770 cites W1967389627 @default.
• W2309061770 cites W1975054892 @default.
• W2309061770 cites W1975284527 @default.
• W2309061770 cites W1979431749 @default.
• W2309061770 cites W1981636025 @default.
• W2309061770 cites W1987563234 @default.
• W2309061770 cites W1995717402 @default.
• W2309061770 cites W1997095154 @default.
• W2309061770 cites W1998750388 @default.
• W2309061770 cites W2003471214 @default.
• W2309061770 cites W2009951639 @default.
• W2309061770 cites W2011707720 @default.
• W2309061770 cites W2017048267 @default.
• W2309061770 cites W2019006773 @default.
• W2309061770 cites W2028320146 @default.
• W2309061770 cites W2028824011 @default.
• W2309061770 cites W2031409368 @default.
• W2309061770 cites W2042151700 @default.
• W2309061770 cites W2051995369 @default.
• W2309061770 cites W2057807154 @default.
• W2309061770 cites W2062684873 @default.
• W2309061770 cites W2064019732 @default.
• W2309061770 cites W2074683285 @default.
• W2309061770 cites W2074811076 @default.
• W2309061770 cites W2080624765 @default.
• W2309061770 cites W2081367955 @default.
• W2309061770 cites W2091443061 @default.
• W2309061770 cites W2092952629 @default.
• W2309061770 cites W2093445429 @default.
• W2309061770 cites W2094348483 @default.
• W2309061770 cites W2118131776 @default.
• W2309061770 cites W2127468063 @default.
• W2309061770 cites W2127477904 @default.
• W2309061770 cites W2151655408 @default.
• W2309061770 cites W2170599187 @default.
• W2309061770 cites W2173813363 @default.
• W2309061770 cites W2300981316 @default.
• W2309061770 cites W28434911 @default.
• W2309061770 doi "https://doi.org/10.2118/177481-ms" @default.
• W2309061770 hasPublicationYear "2015" @default.
• W2309061770 type Work @default.
• W2309061770 sameAs 2309061770 @default.
• W2309061770 citedByCount "3" @default.
• W2309061770 countsByYear W23090617702016 @default.
• W2309061770 countsByYear W23090617702017 @default.
• W2309061770 crossrefType "proceedings-article" @default.
• W2309061770 hasAuthorship W2309061770A5014709706 @default.
• W2309061770 hasAuthorship W2309061770A5026966481 @default.
• W2309061770 hasAuthorship W2309061770A5047861147 @default.
• W2309061770 hasAuthorship W2309061770A5057212913 @default.
• W2309061770 hasAuthorship W2309061770A5081205740 @default.
• W2309061770 hasBestOaLocation W23090617702 @default.
• W2309061770 hasConcept C121332964 @default.
• W2309061770 hasConcept C127313418 @default.
• W2309061770 hasConcept C127413603 @default.
• W2309061770 hasConcept C151730666 @default.
• W2309061770 hasConcept C153127940 @default.
• W2309061770 hasConcept C2776608160 @default.
• W2309061770 hasConcept C38349280 @default.
• W2309061770 hasConcept C548081761 @default.
• W2309061770 hasConcept C57879066 @default.
• W2309061770 hasConcept C59427239 @default.
• W2309061770 hasConcept C62520636 @default.
• W2309061770 hasConcept C78762247 @default.
• W2309061770 hasConcept C85725439 @default.
• W2309061770 hasConceptScore W2309061770C121332964 @default.
• W2309061770 hasConceptScore W2309061770C127313418 @default.
• W2309061770 hasConceptScore W2309061770C127413603 @default.
• W2309061770 hasConceptScore W2309061770C151730666 @default.
• W2309061770 hasConceptScore W2309061770C153127940 @default.
• W2309061770 hasConceptScore W2309061770C2776608160 @default.
• W2309061770 hasConceptScore W2309061770C38349280 @default.
• W2309061770 hasConceptScore W2309061770C548081761 @default.
• W2309061770 hasConceptScore W2309061770C57879066 @default.
• W2309061770 hasConceptScore W2309061770C59427239 @default.
• W2309061770 hasConceptScore W2309061770C62520636 @default.
• W2309061770 hasConceptScore W2309061770C78762247 @default.
• W2309061770 hasConceptScore W2309061770C85725439 @default.
• W2309061770 hasLocation W23090617701 @default.
• W2309061770 hasLocation W23090617702 @default.
• W2309061770 hasOpenAccess W2309061770 @default.
• W2309061770 hasPrimaryLocation W23090617701 @default.
• W2309061770 hasRelatedWork W1971996461 @default.
• W2309061770 hasRelatedWork W1985098579 @default.
• W2309061770 hasRelatedWork W1991745847 @default.

• next