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dc.contributor.authorOstilla Monico, Rodolfo 
dc.contributor.authorArslan, Ali
dc.contributor.otherIngeniería Mecánica y Diseño Industriales_ES
dc.date.accessioned2025-12-03T13:02:03Z
dc.date.available2025-12-03T13:02:03Z
dc.date.issued2025
dc.identifier.issn1469-7645
dc.identifier.issn0022-1120
dc.identifier.urihttp://hdl.handle.net/10498/38137
dc.description.abstractWe study convection in a volumetrically heated fluid which is cooled from both plates and is under rotation through the use of direct numerical simulations. The onset of convection matches similar systems and predictions from asymptotic analysis. At low rotation rates, the fluid becomes more organised, enhancing heat transport and increasing boundary layer asymmetry, whereas high rotation rates suppress convection. Velocity and temperature statistics reveal that the top unstably stratified boundary layer exhibits behaviour consistent with other rotating convective systems, while the bottom boundary shows a unique interaction between unstable stratification and Ekman boundary layers. Additional flow statistics such as energy dissipation are analysed to rationalise the flow behaviour.es_ES
dc.formatapplication/pdfes_ES
dc.language.isoenges_ES
dc.publisherCambridge University Presses_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourceJournal of Fluid Mechanics - 2025, Vol. 1018, , A31.es_ES
dc.subjectconvectiones_ES
dc.subjectturbulent convectiones_ES
dc.titleRotationally affected internally heated convectiones_ES
dc.typejournal articlees_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1017/JFM.2025.10520
dc.type.hasVersionVoRes_ES


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Atribución 4.0 Internacional
This work is under a Creative Commons License Atribución 4.0 Internacional