FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2307644128> ?p ?o ?g. }

• W2307644128 abstract "Abstract Matrix acidizing is a technique used for stimulating carbonate formations. Fluids used for this purpose are routinely characterized in the laboratory by means of core flood testing. Though several key insights can be obtained using the laboratory core flood technique, simulating exact downhole environments and extrapolation of the results obtained to field-scale has proven challenging. This paper addresses two specific topics related to acid wormholing—upscaling laboratory results to field scenarios and the interaction of reaction products in high pressure reservoirs. To study the upscaling of acid wormholing experiments in field scenarios, a radial core flood testing apparatus was set up to better mimic actual wellbore acidizing flow conditions. The effects of radial flow path and completion type (i.e. openhole versus cased hole) as well as the applicability of the upscaling wormhole propagation model were studied. Furthermore, CT scans of related core samples were performed to characterize wormhole patterns generated by acid dissolution. In addition, tests were performed at high pressures and flow rates to study the effects of the interaction of reaction products on the wormholing process at typical high bottomhole pressure values. Results from radial core flood techniques showed significant differences in terms of pore volume to breakthrough (PVBT) based on well completion type. Further, a current upscaling algorithm for wormhole propagation modeling was verified by comparison to corresponding experimental data, thus demonstrating the suitability of described linear core flow testing methods for fluid characterization and data modeling. The wormhole propagation model (based on the use of fitting coefficient) is well-justified by the probability of increased fluid loss from the wormhole in the case of deeper radial penetration, which overall reduces the efficiency of wormholing. CT scan results revealed nonuniform radial distribution of wormhole propagation, thus shedding light on challenges associated with achieving 360° stimulation around the wellbore. Experiments at higher pressures showed that, at higher flow rates investigated (or beyond optimum) wormhole propagation has a higher than one third dependence on interstitial velocity, signifying that high pressure reservoirs require greater volumes of acid for proper stimulation. Experimental observations are presented to correlate the results obtained thus far and help resolve controversies between various publications. Presented studies highlight the effects of higher pressure in acid wormholing and signify the need for proper volume accounting in terms of job design. A simple radial core flood technique has been developed in this work, and has an advantage in terms of diversion studies by providing a means of arranging high and low permeability core samples in the same order as formation layers and accounting for fluid entrance position." @default.
• W2307644128 created "2016-06-24" @default.
• W2307644128 creator A5027223270 @default.
• W2307644128 creator A5046768638 @default.
• W2307644128 creator A5046777376 @default.
• W2307644128 creator A5065192662 @default.
• W2307644128 creator A5069959226 @default.
• W2307644128 date "2016-03-22" @default.
• W2307644128 modified "2023-09-25" @default.
• W2307644128 title "HP/HT Carbonate Acidizing—Recent Discoveries and Contradictions in Wormhole Phenomenon" @default.
• W2307644128 cites W1975651902 @default.
• W2307644128 cites W1976232491 @default.
• W2307644128 cites W1976930454 @default.
• W2307644128 cites W1978567419 @default.
• W2307644128 cites W1981014492 @default.
• W2307644128 cites W1997724037 @default.
• W2307644128 cites W2010809101 @default.
• W2307644128 cites W2011521727 @default.
• W2307644128 cites W2013550668 @default.
• W2307644128 cites W2022905963 @default.
• W2307644128 cites W2035647668 @default.
• W2307644128 cites W2044826107 @default.
• W2307644128 cites W2065142096 @default.
• W2307644128 cites W2065384567 @default.
• W2307644128 cites W2071123978 @default.
• W2307644128 cites W2074983047 @default.
• W2307644128 cites W2077220356 @default.
• W2307644128 cites W2079447366 @default.
• W2307644128 cites W2097911916 @default.
• W2307644128 cites W2284720457 @default.
• W2307644128 cites W2332473552 @default.
• W2307644128 cites W4233726702 @default.
• W2307644128 doi "https://doi.org/10.4043/26714-ms" @default.
• W2307644128 hasPublicationYear "2016" @default.
• W2307644128 type Work @default.
• W2307644128 sameAs 2307644128 @default.
• W2307644128 citedByCount "5" @default.
• W2307644128 countsByYear W23076441282016 @default.
• W2307644128 countsByYear W23076441282018 @default.
• W2307644128 countsByYear W23076441282019 @default.
• W2307644128 countsByYear W23076441282023 @default.
• W2307644128 crossrefType "proceedings-article" @default.
• W2307644128 hasAuthorship W2307644128A5027223270 @default.
• W2307644128 hasAuthorship W2307644128A5046768638 @default.
• W2307644128 hasAuthorship W2307644128A5046777376 @default.
• W2307644128 hasAuthorship W2307644128A5065192662 @default.
• W2307644128 hasAuthorship W2307644128A5069959226 @default.
• W2307644128 hasConcept C121332964 @default.
• W2307644128 hasConcept C127313418 @default.
• W2307644128 hasConcept C127413603 @default.
• W2307644128 hasConcept C132459708 @default.
• W2307644128 hasConcept C134306372 @default.
• W2307644128 hasConcept C187320778 @default.
• W2307644128 hasConcept C191897082 @default.
• W2307644128 hasConcept C192562407 @default.
• W2307644128 hasConcept C2780659211 @default.
• W2307644128 hasConcept C29013271 @default.
• W2307644128 hasConcept C33923547 @default.
• W2307644128 hasConcept C38349280 @default.
• W2307644128 hasConcept C41008148 @default.
• W2307644128 hasConcept C42360764 @default.
• W2307644128 hasConcept C57879066 @default.
• W2307644128 hasConcept C62520636 @default.
• W2307644128 hasConcept C78762247 @default.
• W2307644128 hasConcept C88380143 @default.
• W2307644128 hasConceptScore W2307644128C121332964 @default.
• W2307644128 hasConceptScore W2307644128C127313418 @default.
• W2307644128 hasConceptScore W2307644128C127413603 @default.
• W2307644128 hasConceptScore W2307644128C132459708 @default.
• W2307644128 hasConceptScore W2307644128C134306372 @default.
• W2307644128 hasConceptScore W2307644128C187320778 @default.
• W2307644128 hasConceptScore W2307644128C191897082 @default.
• W2307644128 hasConceptScore W2307644128C192562407 @default.
• W2307644128 hasConceptScore W2307644128C2780659211 @default.
• W2307644128 hasConceptScore W2307644128C29013271 @default.
• W2307644128 hasConceptScore W2307644128C33923547 @default.
• W2307644128 hasConceptScore W2307644128C38349280 @default.
• W2307644128 hasConceptScore W2307644128C41008148 @default.
• W2307644128 hasConceptScore W2307644128C42360764 @default.
• W2307644128 hasConceptScore W2307644128C57879066 @default.
• W2307644128 hasConceptScore W2307644128C62520636 @default.
• W2307644128 hasConceptScore W2307644128C78762247 @default.
• W2307644128 hasConceptScore W2307644128C88380143 @default.
• W2307644128 hasLocation W23076441281 @default.
• W2307644128 hasOpenAccess W2307644128 @default.
• W2307644128 hasPrimaryLocation W23076441281 @default.
• W2307644128 hasRelatedWork W2055114552 @default.
• W2307644128 hasRelatedWork W2055487584 @default.
• W2307644128 hasRelatedWork W2351773383 @default.
• W2307644128 hasRelatedWork W2357409530 @default.
• W2307644128 hasRelatedWork W2359342574 @default.
• W2307644128 hasRelatedWork W2370586348 @default.
• W2307644128 hasRelatedWork W3101151780 @default.
• W2307644128 hasRelatedWork W3144486045 @default.
• W2307644128 hasRelatedWork W4320523533 @default.
• W2307644128 hasRelatedWork W4327699117 @default.
• W2307644128 isParatext "false" @default.
• W2307644128 isRetracted "false" @default.
• W2307644128 magId "2307644128" @default.
• W2307644128 workType "article" @default.