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contributor authorHanna H. Klein
contributor authorRachamim Rubin
contributor authorJacob Karni
date accessioned2017-05-09T00:21:33Z
date available2017-05-09T00:21:33Z
date copyrightAugust, 2006
date issued2006
identifier issn0199-6231
identifier otherJSEEDO-28397#406_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/134609
description abstractIn high-temperature solar-thermal systems the conversion of solar to thermal energy requires a radiation absorbing surface to transfer the radiative solar energy to the working fluid. The present study focuses on the generation of a moving radiation absorber using particles suspended in the working fluid. Three methods of particle entrainment in a gas were investigated. Elutriating fine particles from a spouted bed was found to be the preferred method. The diameter range of the entrained carbon black particles was 0.030–25μm, with 99.7% of the particles having an equivalent diameter less than 1μm, and 48% of the projected surface area was due to agglomerated particles with average equivalent diameter >5μm. The moving radiation absorber was tested in a solar receiver using nitrogen as a working fluid. The inner wall temperatures in the receiver cavity were below the gas exit temperature, which shows that the bulk heat transfer from the incoming solar radiation to the gas takes place via the moving radiation absorbing particles.
publisherThe American Society of Mechanical Engineers (ASME)
titleGeneration of a Radiation Absorbing Medium for a Solar Receiver by Elutriation of Fine Particles From a Spouted Bed
typeJournal Paper
journal volume128
journal issue3
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.2212441
journal fristpage406
journal lastpage408
identifier eissn1528-8986
keywordsRadiation (Physics)
keywordsParticulate matter
keywordsSolar energy AND Carbon black pigments
treeJournal of Solar Energy Engineering:;2006:;volume( 128 ):;issue: 003
contenttypeFulltext


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