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    Rapid Heating of Gas/Small Particle Mixture

    Source: Journal of Solar Energy Engineering:;1987:;volume( 109 ):;issue: 002::page 143
    Author:
    K. Y. Wang
    ,
    W. W. Yuen
    DOI: 10.1115/1.3268191
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: The 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.
    keyword(s): Particulate matter , Mixtures , Heating , Temperature , Radiation scattering , Electromagnetic scattering , Carbon , Solar energy , Radiation (Physics) , Albedo , High temperature AND Pressure ,
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      Rapid Heating of Gas/Small Particle Mixture

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    http://yetl.yabesh.ir/yetl1/handle/yetl/103009
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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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