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contributor authorH. M. Güven
contributor authorR. B. Bannerot
date accessioned2017-05-08T23:23:17Z
date available2017-05-08T23:23:17Z
date copyrightNovember, 1986
date issued1986
identifier issn0199-6231
identifier otherJSEEDO-28193#275_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/101610
description abstractA study is presented where potential optical errors in parabolic troughs are divided into two groups: random and nonrandom. It is shown that the intercept factor is a function of both random and nonrandom errors as well as geometric parameters such as concentration ratio and rim angle. Three error parameters, universal to all collector geometries, that is, “universal” error parameters which combine random and nonrandom errors with collector geometric parameters, are derived analytically. The mathematical derivation of these universal error parameters is presented. A numerical technique, a detailed ray-trace computer routine which maps rays from elemental reflector surfaces to the absorber surface, is used to validate the existence of the universal error parameters. The universal error parameters are made up of one universal random error parameter, σ* ( =σC ), and two universal nonrandom error parameters, β* ( = βC ) and d * (=(d r )y /D ). The use of universal error parameters for comprehensive optical analysis of troughs is also presented.
publisherThe American Society of Mechanical Engineers (ASME)
titleDerivation of Universal Error Parameters for Comprehensive Optical Analysis of Parabolic Troughs
typeJournal Paper
journal volume108
journal issue4
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.3268106
journal fristpage275
journal lastpage281
identifier eissn1528-8986
keywordsErrors
keywordsParabolic troughs AND Computers
treeJournal of Solar Energy Engineering:;1986:;volume( 108 ):;issue: 004
contenttypeFulltext


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