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contributor authorR. Buck
contributor authorE. Teufel
date accessioned2017-05-09T00:35:22Z
date available2017-05-09T00:35:22Z
date copyrightFebruary, 2009
date issued2009
identifier issn0199-6231
identifier otherJSEEDO-28416#011001_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/141949
description abstractHeliostat canting (alignment of mirror facets) is known to have a major influence on the optical efficiency of heliostat fields and therefore on the power output of solar tower plants. In recent years several canting concepts were used, mainly on- and off-axis canting. Several new canting concepts, such as stretched-parabolic or target-aligned canting, were proposed in order to improve the performance of heliostats. As solar power plants become economically more attractive, knowledge about the influence of canting becomes more important. In this context, the influence of several factors on the canting method is discussed and optimal canting strategies are described. The considered factors comprise plant power level, heliostat position in the field, heliostat area, receiver dimension, and site latitude. It is concluded that the target-aligned tracking method is superior to all other variants in the majority of cases. As for the standard azimuth-elevation tracking methods, not one of these exhibits a clear advantage. It is only the on-axis method that performs worst in all cases.
publisherThe American Society of Mechanical Engineers (ASME)
titleComparison and Optimization of Heliostat Canting Methods
typeJournal Paper
journal volume131
journal issue1
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.3027500
journal fristpage11001
identifier eissn1528-8986
keywordsOptimization
keywordsSolar energy
keywordsErrors
keywordsIndustrial plants
keywordsMirrors
keywordsDimensions
keywordsSensitivity analysis
keywordsSolar power stations AND Evaluation methods
treeJournal of Solar Energy Engineering:;2009:;volume( 131 ):;issue: 001
contenttypeFulltext


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