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contributor authorK. Y. Wang
contributor authorW. W. Yuen
date accessioned2017-05-08T23:25:40Z
date available2017-05-08T23:25:40Z
date copyrightMay, 1987
date issued1987
identifier issn0199-6231
identifier otherJSEEDO-28197#143_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/103009
description abstractThe concept of using a mixture of particles and air as a medium to absorb radiative energy has been proposed for various applications. In this paper, carbon particles mixed with gas form a medium that absorbs radiation from sources such as concentrated solar energy. A single-particle, two-temperature model is used to study the transient temperature of the particle/gas mixture as it undergoes a constant pressure expansion process. The results indicate that for particles smaller than 1 μm in diameter, the surrounding air can be heated as quickly as the particles, while for particles larger than 1 mm in diameter, the air temperature stays relatively unchanged and the particles are heated to a very high temperature. The scattering albedos from the particles are also calculated, revealing that their contribution from scattering to the heating process is insignificant for particles with diameter less than 1 μm.
publisherThe American Society of Mechanical Engineers (ASME)
titleRapid Heating of Gas/Small Particle Mixture
typeJournal Paper
journal volume109
journal issue2
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.3268191
journal fristpage143
journal lastpage149
identifier eissn1528-8986
keywordsParticulate matter
keywordsMixtures
keywordsHeating
keywordsTemperature
keywordsRadiation scattering
keywordsElectromagnetic scattering
keywordsCarbon
keywordsSolar energy
keywordsRadiation (Physics)
keywordsAlbedo
keywordsHigh temperature AND Pressure
treeJournal of Solar Energy Engineering:;1987:;volume( 109 ):;issue: 002
contenttypeFulltext


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