Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector
•Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Mai...
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description | •Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Main frequencies affecting the stability of the PTC structure are determined.
Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. A spectral analysis around the parabola and its receiver is also carried out in order to detect the most relevant frequencies related to the vortex shedding mechanism which affects the stability of the collector. |
doi_str_mv | 10.1016/j.apenergy.2014.05.037 |
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Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. A spectral analysis around the parabola and its receiver is also carried out in order to detect the most relevant frequencies related to the vortex shedding mechanism which affects the stability of the collector.</description><identifier>ISSN: 0306-2619</identifier><identifier>EISSN: 1872-9118</identifier><identifier>DOI: 10.1016/j.apenergy.2014.05.037</identifier><identifier>CODEN: APENDX</identifier><language>eng</language><publisher>Kidlington: Elsevier Ltd</publisher><subject>Applied sciences ; Calor ; Dinàmica de fluids ; Energia solar tèrmica ; Energia tèrmica solar ; Energies ; Energy ; Energy. Thermal use of fuels ; Exact sciences and technology ; Fluid dynamics ; Heat ; Heat transfer ; Heat transfer coefficient ; Large Eddy Simulations ; Natural energy ; Parabolic trough solar collector ; PTC stability ; Solar collectors ; Solar energy ; Solar thermal conversion ; Solar thermal energy ; Theoretical studies. Data and constants. Metering ; Transmission ; Transmissió ; Turbulence ; Turbulència ; Wind speed effect ; Àrees temàtiques de la UPC</subject><ispartof>Applied energy, 2014-10, Vol.130, p.200-211</ispartof><rights>2014 Elsevier Ltd</rights><rights>2015 INIST-CNRS</rights><rights>Attribution-NonCommercial-NoDerivs 3.0 Spain info:eu-repo/semantics/openAccess <a href="http://creativecommons.org/licenses/by-nc-nd/3.0/es/">http://creativecommons.org/licenses/by-nc-nd/3.0/es/</a></rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c432t-eecd95bd4802c90a013a3291b3c2d37de224fec16d05f2a119a091946ecfc1673</citedby><cites>FETCH-LOGICAL-c432t-eecd95bd4802c90a013a3291b3c2d37de224fec16d05f2a119a091946ecfc1673</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0306261914005327$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,776,780,881,3537,26951,27901,27902,65534</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=28610920$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Hachicha, A.A.</creatorcontrib><creatorcontrib>Rodríguez, I.</creatorcontrib><creatorcontrib>Oliva, A.</creatorcontrib><title>Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector</title><title>Applied energy</title><description>•Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Main frequencies affecting the stability of the PTC structure are determined.
Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. A spectral analysis around the parabola and its receiver is also carried out in order to detect the most relevant frequencies related to the vortex shedding mechanism which affects the stability of the collector.</description><subject>Applied sciences</subject><subject>Calor</subject><subject>Dinàmica de fluids</subject><subject>Energia solar tèrmica</subject><subject>Energia tèrmica solar</subject><subject>Energies</subject><subject>Energy</subject><subject>Energy. Thermal use of fuels</subject><subject>Exact sciences and technology</subject><subject>Fluid dynamics</subject><subject>Heat</subject><subject>Heat transfer</subject><subject>Heat transfer coefficient</subject><subject>Large Eddy Simulations</subject><subject>Natural energy</subject><subject>Parabolic trough solar collector</subject><subject>PTC stability</subject><subject>Solar collectors</subject><subject>Solar energy</subject><subject>Solar thermal conversion</subject><subject>Solar thermal energy</subject><subject>Theoretical studies. Data and constants. Metering</subject><subject>Transmission</subject><subject>Transmissió</subject><subject>Turbulence</subject><subject>Turbulència</subject><subject>Wind speed effect</subject><subject>Àrees temàtiques de la UPC</subject><issn>0306-2619</issn><issn>1872-9118</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>XX2</sourceid><recordid>eNqFkMFu3CAQhlHVSt2mfYWKS492Z8BrL7dGUZJWipRLqx7RLAxZVq6xwJsobx9Wm6THHBBi-L9h-IT4itAiYP9939LME-e7x1YBdi2sW9DDO7HCzaAag7h5L1agoW9Uj-aj-FTKHgAUKlgJ-zdOXpaZ2UsOgd0i0ySXHcswpgcZIo9eUo3smBa5ZJpK4Cwpp0Mtkpwp0zaN0dW7dLjbyZJGytKlcay9Uv4sPgQaC3953s_En6vL3xc_m5vb618X5zeN67RaGmbnzXrruw0oZ4AANWllcKud8nrwrFRXh8PewzooQjQEBk3Xswu1Ougzgae-rhyczew4O1psovj_cFwKBmWV1oPGyvTPTE6lZA52zvEf5UeLYI9q7d6-qLVHtRbWtqqt4LcTOFNxNIZqxcXySqtNj2AU1NyPU47rz-8jZ1tc5Mmxj3WoxfoU33rqCSCJk2w</recordid><startdate>20141001</startdate><enddate>20141001</enddate><creator>Hachicha, A.A.</creator><creator>Rodríguez, I.</creator><creator>Oliva, A.</creator><general>Elsevier Ltd</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>XX2</scope></search><sort><creationdate>20141001</creationdate><title>Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector</title><author>Hachicha, A.A. ; Rodríguez, I. ; Oliva, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c432t-eecd95bd4802c90a013a3291b3c2d37de224fec16d05f2a119a091946ecfc1673</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Applied sciences</topic><topic>Calor</topic><topic>Dinàmica de fluids</topic><topic>Energia solar tèrmica</topic><topic>Energia tèrmica solar</topic><topic>Energies</topic><topic>Energy</topic><topic>Energy. Thermal use of fuels</topic><topic>Exact sciences and technology</topic><topic>Fluid dynamics</topic><topic>Heat</topic><topic>Heat transfer</topic><topic>Heat transfer coefficient</topic><topic>Large Eddy Simulations</topic><topic>Natural energy</topic><topic>Parabolic trough solar collector</topic><topic>PTC stability</topic><topic>Solar collectors</topic><topic>Solar energy</topic><topic>Solar thermal conversion</topic><topic>Solar thermal energy</topic><topic>Theoretical studies. Data and constants. Metering</topic><topic>Transmission</topic><topic>Transmissió</topic><topic>Turbulence</topic><topic>Turbulència</topic><topic>Wind speed effect</topic><topic>Àrees temàtiques de la UPC</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hachicha, A.A.</creatorcontrib><creatorcontrib>Rodríguez, I.</creatorcontrib><creatorcontrib>Oliva, A.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Recercat</collection><jtitle>Applied energy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hachicha, A.A.</au><au>Rodríguez, I.</au><au>Oliva, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector</atitle><jtitle>Applied energy</jtitle><date>2014-10-01</date><risdate>2014</risdate><volume>130</volume><spage>200</spage><epage>211</epage><pages>200-211</pages><issn>0306-2619</issn><eissn>1872-9118</eissn><coden>APENDX</coden><abstract>•Large Eddy Simulations to study fluid flow and heat transfer on a PTC are performed.•Drag and lift forces were shown to be independent on the Reynolds number.•Nusselt number is highly dependent on the pitch angle.•Heat losses from the HCE are overestimated compared to literature’s correlations.•Main frequencies affecting the stability of the PTC structure are determined.
Parabolic trough solar collectors are currently one of the most mature and prominent solar technology for the production of electricity. These systems are usually located in an open terrain where strong winds may be found, and could affect their stability and optical performance, as well as the heat exchange between the solar receiver and the ambient air. In this context, a wind flow analysis around a parabolic trough solar collector under real working conditions is performed. A numerical aerodynamic and heat transfer study based on Large Eddy Simulations is carried out to characterise the wind loads and heat transfer coefficients. After the study carried out by the authors in an earlier work (Hachicha et al. 2013) at ReW1=3.9×105, computations are performed at a higher Reynolds number of ReW2=1×106, and for various pitch angles. The effects of wind speed and pitch angle on the averaged and instantaneous flow are assessed. The aerodynamic coefficients are calculated around the solar collector and validated with measurements performed in wind tunnel tests. The variation of the heat transfer coefficient around the heat collector element with the Reynolds number is presented and compared to the circular cylinder in cross-flow. The unsteady flow is studied for three pitch angles: θ=0°,θ=45° and θ=90° and different structures and recirculation regions are identified. A spectral analysis around the parabola and its receiver is also carried out in order to detect the most relevant frequencies related to the vortex shedding mechanism which affects the stability of the collector.</abstract><cop>Kidlington</cop><pub>Elsevier Ltd</pub><doi>10.1016/j.apenergy.2014.05.037</doi><tpages>12</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Applied sciences Calor Dinàmica de fluids Energia solar tèrmica Energia tèrmica solar Energies Energy Energy. Thermal use of fuels Exact sciences and technology Fluid dynamics Heat Heat transfer Heat transfer coefficient Large Eddy Simulations Natural energy Parabolic trough solar collector PTC stability Solar collectors Solar energy Solar thermal conversion Solar thermal energy Theoretical studies. Data and constants. Metering Transmission Transmissió Turbulence Turbulència Wind speed effect Àrees temàtiques de la UPC |
title | Wind speed effect on the flow field and heat transfer around a parabolic trough solar collector |
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