A model for the directional distribution of the diffuse sky radiance with an application to a CPC collector
The development of a new, semi-empirical model for the directional distribution of the diffuse radiance is reported. The proposed regression-type model, with the form of its base functions obtained from physical principles, is based on a combination of the purely physical reasoning approach and the...
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Veröffentlicht in: | Solar energy 1990, Vol.44 (5), p.291-296 |
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description | The development of a new, semi-empirical model for the directional distribution of the diffuse radiance is reported. The proposed regression-type model, with the form of its base functions obtained from physical principles, is based on a combination of the purely physical reasoning approach and the purely empirical approach. Direct multiple-scattering calculations are circumvented through the use of the method of successive orders of scattering. The model is calibrated for the mean diffuse radiance estimated under all sky conditions reported in a large and comprehensive diffuse radiance data set. It is found that only a small increase in accuracy is gained by including higher orders of scattering, and this increase does not justify the complexity of the resulting model. Therefore, the single scattering approximation is recommended. The use of the model is illustrated in a typical application, in which the fraction of diffuse radiation intercepted by the receiver of a compound parabolic concentrator is computed. |
doi_str_mv | 10.1016/0038-092X(90)90056-I |
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The use of the model is illustrated in a typical application, in which the fraction of diffuse radiation intercepted by the receiver of a compound parabolic concentrator is computed.</description><identifier>ISSN: 0038-092X</identifier><identifier>EISSN: 1471-1257</identifier><identifier>DOI: 10.1016/0038-092X(90)90056-I</identifier><identifier>CODEN: SRENA4</identifier><language>eng</language><publisher>Oxford: Elsevier Ltd</publisher><subject>140100 - Solar Energy- Resources & Availability ; ANGULAR DISTRIBUTION ; Applied sciences ; COMPOUND PARABOLIC CONCENTRATOR ; COMPOUND PARABOLIC CONCENTRATORS ; DIFFUSE SOLAR RADIATION ; DISTRIBUTION ; ENERGIA SOLAR ; ENERGIE SOLAIRE ; Energy ; EQUIPEMENT ; EQUIPO ; Exact sciences and technology ; INSOLATION ; LIGHT SCATTERING ; MATHEMATICAL MODELS ; MATHEMATICS ; MODELE ; MODELOS ; Natural energy ; ORDERS OF SCATTERING ; PARABOLIC MIRRORS ; PERFORMANCE TESTING ; RADIATIONS ; REGRESSION ANALYSIS ; SCATTERING ; SKY CONDITIONS ; SOLAR CONCENTRATORS ; SOLAR ENERGY ; SOLAR EQUIPMENT ; SOLAR FLUX ; SOLAR RADIATION ; STATISTICS ; STELLAR RADIATION ; TESTING</subject><ispartof>Solar energy, 1990, Vol.44 (5), p.291-296</ispartof><rights>1990</rights><rights>1990 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c410t-cf32c6420fe70213e7534b55626b1fa9fe804f63d583b77a1b908774fc2fa2a43</citedby><cites>FETCH-LOGICAL-c410t-cf32c6420fe70213e7534b55626b1fa9fe804f63d583b77a1b908774fc2fa2a43</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/0038-092X(90)90056-I$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,777,781,882,3537,4010,27904,27905,27906,45976</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=6846609$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/6565785$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Siala, F.M.F.</creatorcontrib><creatorcontrib>Hooper, F.C.</creatorcontrib><title>A model for the directional distribution of the diffuse sky radiance with an application to a CPC collector</title><title>Solar energy</title><description>The development of a new, semi-empirical model for the directional distribution of the diffuse radiance is reported. The proposed regression-type model, with the form of its base functions obtained from physical principles, is based on a combination of the purely physical reasoning approach and the purely empirical approach. Direct multiple-scattering calculations are circumvented through the use of the method of successive orders of scattering. The model is calibrated for the mean diffuse radiance estimated under all sky conditions reported in a large and comprehensive diffuse radiance data set. It is found that only a small increase in accuracy is gained by including higher orders of scattering, and this increase does not justify the complexity of the resulting model. Therefore, the single scattering approximation is recommended. The use of the model is illustrated in a typical application, in which the fraction of diffuse radiation intercepted by the receiver of a compound parabolic concentrator is computed.</description><subject>140100 - Solar Energy- Resources & Availability</subject><subject>ANGULAR DISTRIBUTION</subject><subject>Applied sciences</subject><subject>COMPOUND PARABOLIC CONCENTRATOR</subject><subject>COMPOUND PARABOLIC CONCENTRATORS</subject><subject>DIFFUSE SOLAR RADIATION</subject><subject>DISTRIBUTION</subject><subject>ENERGIA SOLAR</subject><subject>ENERGIE SOLAIRE</subject><subject>Energy</subject><subject>EQUIPEMENT</subject><subject>EQUIPO</subject><subject>Exact sciences and technology</subject><subject>INSOLATION</subject><subject>LIGHT SCATTERING</subject><subject>MATHEMATICAL MODELS</subject><subject>MATHEMATICS</subject><subject>MODELE</subject><subject>MODELOS</subject><subject>Natural energy</subject><subject>ORDERS OF SCATTERING</subject><subject>PARABOLIC MIRRORS</subject><subject>PERFORMANCE TESTING</subject><subject>RADIATIONS</subject><subject>REGRESSION ANALYSIS</subject><subject>SCATTERING</subject><subject>SKY CONDITIONS</subject><subject>SOLAR CONCENTRATORS</subject><subject>SOLAR ENERGY</subject><subject>SOLAR EQUIPMENT</subject><subject>SOLAR FLUX</subject><subject>SOLAR RADIATION</subject><subject>STATISTICS</subject><subject>STELLAR RADIATION</subject><subject>TESTING</subject><issn>0038-092X</issn><issn>1471-1257</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1990</creationdate><recordtype>article</recordtype><recordid>eNp9kV1rFDEUhoMouLb-AfEiiEi9mHqSycfMjVCWqgsFC1rwLmQyiRubnWyTrNJ_b6az9LJXSXifczjnCUJvCZwTIOITQNs10NNfZz187AG4aDbP0IowSRpCuXyOVo_IS_Qq5z8ARJJOrtDtBd7F0QbsYsJla_HokzXFx0mHes8l-eEwP3F0x9y5Q7Y4397jpEevJ2PxP1-2WE9Y7_fBG_3Al4g1Xl-vsYkh1JYxnaIXTodsXx_PE3Tz5fLn-ltz9f3rZn1x1RhGoDTGtdQIRsFZCZS0VvKWDZwLKgbidO9sB8yJduRdO0ipydBDJyVzhjpNNWtP0Lulb8zFq2x8sWZr4jTVKZTggsuOV-jDAu1TvDvYXNTOZ2ND0JONh6yqNspoJyvIFtCkmHOyTu2T3-l0rwioWb-a3arZrepBPehXm1r2_thfZ6ODS1WUz4-1omNCQF-xNwvmdFT6d6rIzY8eWsIlqeHnJbTV1l9v07yMrcKXT1Jj9E8P8R-LhKDt</recordid><startdate>1990</startdate><enddate>1990</enddate><creator>Siala, F.M.F.</creator><creator>Hooper, F.C.</creator><general>Elsevier Ltd</general><general>Elsevier</general><scope>FBQ</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SC</scope><scope>8FD</scope><scope>JQ2</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><scope>OTOTI</scope></search><sort><creationdate>1990</creationdate><title>A model for the directional distribution of the diffuse sky radiance with an application to a CPC collector</title><author>Siala, F.M.F. ; Hooper, F.C.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c410t-cf32c6420fe70213e7534b55626b1fa9fe804f63d583b77a1b908774fc2fa2a43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1990</creationdate><topic>140100 - Solar Energy- Resources & Availability</topic><topic>ANGULAR DISTRIBUTION</topic><topic>Applied sciences</topic><topic>COMPOUND PARABOLIC CONCENTRATOR</topic><topic>COMPOUND PARABOLIC CONCENTRATORS</topic><topic>DIFFUSE SOLAR RADIATION</topic><topic>DISTRIBUTION</topic><topic>ENERGIA SOLAR</topic><topic>ENERGIE SOLAIRE</topic><topic>Energy</topic><topic>EQUIPEMENT</topic><topic>EQUIPO</topic><topic>Exact sciences and technology</topic><topic>INSOLATION</topic><topic>LIGHT SCATTERING</topic><topic>MATHEMATICAL MODELS</topic><topic>MATHEMATICS</topic><topic>MODELE</topic><topic>MODELOS</topic><topic>Natural energy</topic><topic>ORDERS OF SCATTERING</topic><topic>PARABOLIC MIRRORS</topic><topic>PERFORMANCE TESTING</topic><topic>RADIATIONS</topic><topic>REGRESSION ANALYSIS</topic><topic>SCATTERING</topic><topic>SKY CONDITIONS</topic><topic>SOLAR CONCENTRATORS</topic><topic>SOLAR ENERGY</topic><topic>SOLAR EQUIPMENT</topic><topic>SOLAR FLUX</topic><topic>SOLAR RADIATION</topic><topic>STATISTICS</topic><topic>STELLAR RADIATION</topic><topic>TESTING</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Siala, F.M.F.</creatorcontrib><creatorcontrib>Hooper, F.C.</creatorcontrib><collection>AGRIS</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Computer and Information Systems Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Computer and Information Systems Abstracts Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>OSTI.GOV</collection><jtitle>Solar energy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Siala, F.M.F.</au><au>Hooper, F.C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A model for the directional distribution of the diffuse sky radiance with an application to a CPC collector</atitle><jtitle>Solar energy</jtitle><date>1990</date><risdate>1990</risdate><volume>44</volume><issue>5</issue><spage>291</spage><epage>296</epage><pages>291-296</pages><issn>0038-092X</issn><eissn>1471-1257</eissn><coden>SRENA4</coden><abstract>The development of a new, semi-empirical model for the directional distribution of the diffuse radiance is reported. The proposed regression-type model, with the form of its base functions obtained from physical principles, is based on a combination of the purely physical reasoning approach and the purely empirical approach. Direct multiple-scattering calculations are circumvented through the use of the method of successive orders of scattering. The model is calibrated for the mean diffuse radiance estimated under all sky conditions reported in a large and comprehensive diffuse radiance data set. It is found that only a small increase in accuracy is gained by including higher orders of scattering, and this increase does not justify the complexity of the resulting model. Therefore, the single scattering approximation is recommended. The use of the model is illustrated in a typical application, in which the fraction of diffuse radiation intercepted by the receiver of a compound parabolic concentrator is computed.</abstract><cop>Oxford</cop><pub>Elsevier Ltd</pub><doi>10.1016/0038-092X(90)90056-I</doi><tpages>6</tpages></addata></record> |
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subjects | 140100 - Solar Energy- Resources & Availability ANGULAR DISTRIBUTION Applied sciences COMPOUND PARABOLIC CONCENTRATOR COMPOUND PARABOLIC CONCENTRATORS DIFFUSE SOLAR RADIATION DISTRIBUTION ENERGIA SOLAR ENERGIE SOLAIRE Energy EQUIPEMENT EQUIPO Exact sciences and technology INSOLATION LIGHT SCATTERING MATHEMATICAL MODELS MATHEMATICS MODELE MODELOS Natural energy ORDERS OF SCATTERING PARABOLIC MIRRORS PERFORMANCE TESTING RADIATIONS REGRESSION ANALYSIS SCATTERING SKY CONDITIONS SOLAR CONCENTRATORS SOLAR ENERGY SOLAR EQUIPMENT SOLAR FLUX SOLAR RADIATION STATISTICS STELLAR RADIATION TESTING |
title | A model for the directional distribution of the diffuse sky radiance with an application to a CPC collector |
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