Mass flow rate enhancement inside a solar chimney power plant

dc.contributor.authorDaimallah, Ahmed
dc.contributor.authorLebbi, Mohamed
dc.contributor.authorLounici, Mohand Said
dc.date.accessioned2024-02-14T12:49:22Z
dc.date.available2024-02-14T12:49:22Z
dc.date.issued2023
dc.description.abstractThe Solar chimney power plant is a system that converts solar energy to mechanical energy and then to electrical energy. The present work aims to conduct numerical investigation on the influence of the radius ratio Rt* = Rtout/Rtinlet and the height of the tower-chimney, on the flow behavior inside the SCPP of Manzanares. A 2D axi-symetric turbulent model is adopted. The momentum and energy equations are solved using the finite volume method and the simple algorithm. Results show that velocity and mass flow rate inside the SCPP are affected by the radius ratio Rt*, the height of tower-chimney Ht* and intensity radiation Q. We obtain an enhancement of mass flow rate by about 58.23% for the divergence of the tower-chimney.en_US
dc.identifier.issn25629034
dc.identifier.urihttps://journals.library.torontomu.ca/index.php/ictea/article/view/1858
dc.identifier.urihttps://dspace.univ-boumerdes.dz/handle/123456789/13444
dc.language.isoenen_US
dc.publisherToronto Metropolitan Universityen_US
dc.relation.ispartofseriesICTEA 2023: 14th International Conference on Thermal Engineering: Theory and Applications, ( May 25-27)2023, Yalova, Turkiye / Vol. 2023, N° 1(2023);pp. 1-4
dc.subjectSolar chimneyen_US
dc.subjectRadius ratioen_US
dc.subjectHeight of tower-chimneyen_US
dc.subjectSimulationen_US
dc.subjectThermo-hydrodynamic behavioren_US
dc.titleMass flow rate enhancement inside a solar chimney power planten_US
dc.typeArticleen_US

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