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dc.contributor.authorF. C. Hooper
dc.contributor.authorA. P. Brunger
dc.contributor.authorC. S. Chan
dc.date.accessioned2017-05-08T23:25:41Z
dc.date.available2017-05-08T23:25:41Z
dc.date.copyrightFebruary, 1987
dc.date.issued1987
dc.identifier.issn0199-6231
dc.identifier.otherJSEEDO-28196#9_1.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl/handle/yetl/103017
dc.description.abstractA model, previously proposed, describing the sky radiance as a continuous function, has been calibrated from 11,000 individual measurements made in scans taken across springtime skies in Toronto using a narrow field of view radiometer. The model reproduces the measured sky radiance with a mean bias error under five percent and a root mean square error only slightly larger than the standard deviation of the measurements. The model is applied to the calculation of the ratio of the clear sky diffuse irradiance on a slope to that on a horizontal surface. Charts are presented for the direct determination of the expected values of these ratios for surfaces at three tilts and at any azimuth.
dc.publisherThe American Society of Mechanical Engineers (ASME)
dc.titleA Clear Sky Model of Diffuse Sky Radiance
dc.typeJournal Paper
dc.journal.volume109
dc.journal.issue1
dc.journal.titleJournal of Solar Energy Engineering
dc.identifier.doi10.1115/1.3268184
dc.journal.fristpage9
dc.journal.lastpage14
dc.identifier.eissn1528-8986
dc.keywordsRadiance
dc.keywordsErrors AND Measurement
dc.treeJournal of Solar Energy Engineering:;1987:;volume( 109 ):;issue: 001
dc.contenttypeFulltext


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