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contributor authorYong Shuai
contributor authorXin-Lin Xia
contributor authorHe-Ping Tan
date accessioned2017-05-09T00:30:27Z
date available2017-05-09T00:30:27Z
date copyrightMay, 2008
date issued2008
identifier issn0199-6231
identifier otherJSEEDO-28411#021001_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/139297
description abstractThis paper aims at predicting radiation characteristics of the solar collector system by the Monte Carlo method with respect to the corresponding optical properties. Several probability models were introduced to analyze the effects of sunshape and surface roughness. Directional characteristics of radiative flux in the focal region and flux distribution of the cavity receiver were considered. An equivalent radiation flux method is presented for designing the shape of the cavity receiver. Based on the relative numerical simulation results, a new shape cavity receiver called “upside-down tear drop” is proposed to meet an almost uniform radiation flux field. Radiation effects due to multiple reflections and thermal emission in the cavity are parametrized by using the radiative exchange factor. The calculation results can be a valuable reference for the design and assemblage of the dish solar collector system.
publisherThe American Society of Mechanical Engineers (ASME)
titleNumerical Study of Radiation Characteristics in a Dish Solar Collector System
typeJournal Paper
journal volume130
journal issue2
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.2840570
journal fristpage21001
identifier eissn1528-8986
keywordsRadiation (Physics)
keywordsSolar collectors
keywordsCavities
keywordsShapes
keywordsErrors AND Monte Carlo methods
treeJournal of Solar Energy Engineering:;2008:;volume( 130 ):;issue: 002
contenttypeFulltext


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