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dc.contributor.authorBalakin, Boris
dc.contributor.authorStava, Mattias
dc.contributor.authorKosinska, Anna Dorota
dc.date.accessioned2022-06-29T06:34:23Z
dc.date.available2022-06-29T06:34:23Z
dc.date.created2022-05-20T09:43:20Z
dc.date.issued2022
dc.identifier.issn0038-092X
dc.identifier.urihttps://hdl.handle.net/11250/3001415
dc.description.abstractNanofluid-based direct absorption of solar heat results in thermal efficiencies superior to conventional solar thermal technology. In addition, convection of nanofluid can be sustained pump-free in the collector. In this article, we study an aqueous magnetic nanofluid capable to establish the photothermal convection in a lab-scale direct absorption solar collector equipped with a solenoid. The nanofluid consisted of 60-nm Fe2O3 particles dispersed in distilled water at concentration in the range 0.5% wt.-2.0% wt. An empirical model of the photothermal convection was developed based on the experiments. The model accounted for magnetic and thermophoretic forces acting within the nanofluid. The nanofluid with up to 2.0% wt. iron oxide nanoparticles obtained the velocity of ∼5 mm/s under the magnetic field of up to 28 mT. This resulted in the maximum thermal efficiency of the collector equal to 65%.en_US
dc.language.isoengen_US
dc.publisherElsevieren_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titlePhotothermal convection of a magnetic nanofluid in a direct absorption solar collectoren_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2022 The Author(s)en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1016/j.solener.2022.04.027
dc.identifier.cristin2025871
dc.source.journalSolar Energyen_US
dc.source.pagenumber33-39en_US
dc.relation.projectNorges forskningsråd: 300286en_US
dc.identifier.citationSolar Energy. 2022, 239, 33-39.en_US
dc.source.volume239en_US


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