Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/102881
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dc.contributorDepartment of Building Environment and Energy Engineeringen_US
dc.creatorZou, Ben_US
dc.creatorJiang, Yen_US
dc.creatorYao, Yen_US
dc.creatorYang, Hen_US
dc.date.accessioned2023-11-17T02:58:23Z-
dc.date.available2023-11-17T02:58:23Z-
dc.identifier.issn0360-5442en_US
dc.identifier.urihttp://hdl.handle.net/10397/102881-
dc.language.isoenen_US
dc.publisherPergamon Pressen_US
dc.rights© 2019 Published by Elsevier Ltd.en_US
dc.rights© 2019. This manuscript version is made available under the CC-BY-NC-ND 4.0 license https://creativecommons.org/licenses/by-nc-nd/4.0/.en_US
dc.rightsThe following publication Zou, B., Jiang, Y., Yao, Y., & Yang, H. (2019). Impacts of non-ideal optical factors on the performance of parabolic trough solar collectors. Energy, 183, 1150-1165 is available at https://doi.org/10.1016/j.energy.2019.07.024.en_US
dc.subjectImpactsen_US
dc.subjectIncident angleen_US
dc.subjectOptical and thermal performanceen_US
dc.subjectOptical errorsen_US
dc.subjectParabolic trough solar collectoren_US
dc.subjectSunshapeen_US
dc.titleImpacts of non-ideal optical factors on the performance of parabolic trough solar collectorsen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage1150en_US
dc.identifier.epage1165en_US
dc.identifier.volume183en_US
dc.identifier.doi10.1016/j.energy.2019.07.024en_US
dcterms.abstractThis work investigated comprehensively the impacts of non-ideal optical factors, including incident angle, sunshape and optical errors on the performance of the parabolic trough collector (PTC). Each optical factor was defined based on their geometrical principles. It was revealed that the heat flux distribution distorted by optical factors was the main cause of changing performance of the PTC. The temperature distribution was completely dependent on the heat flux distribution. The incident angle caused cosine loss and end loss, which respectively reduced the effective incident solar radiation and produced a near-zero heat flux section at one end of the absorber. Based on the effective incident solar radiation, the collector efficiency was reduced by 41.11% with the incident angle increasing from 0° to 60°. Larger circumsolar ratios produced more uniform circumferential temperature distribution, while reduced greatly the collector efficiency. The specularity error and tracking error affected slightly the receiver's safety, while the slope error reduced obviously the threat to the receiver. When specularity error was small enough (<3 mrad), further improving reflector's specular quality reduced the optical efficiency. The offset direction along X-axis caused the greatest optical loss, and that along positive Y-axis caused local overheating, threatening the receiver's safety.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationEnergy, 15 Sept. 2019, v. 183, p. 1150-1165en_US
dcterms.isPartOfEnergyen_US
dcterms.issued2019-09-15-
dc.identifier.scopus2-s2.0-85068534667-
dc.identifier.eissn1873-6785en_US
dc.description.validate202310 bckwen_US
dc.description.oaAccepted Manuscripten_US
dc.identifier.FolderNumberBEEE-0339-
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Key R&D Program of Chinaen_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS14684729-
dc.description.oaCategoryGreen (AAM)en_US
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