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    Computational Fluid Dynamics Simulation of a Tubular Aerosol Reactor for Solar Thermal ZnO Decomposition

    Source: Journal of Solar Energy Engineering:;2007:;volume( 129 ):;issue: 004::page 391
    Author:
    Christopher Perkins
    ,
    Alan Weimer
    DOI: 10.1115/1.2769700
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: Computational fluid dynamics simulations were performed to model solar ZnO dissociation in a tubular aerosol reactor at ultrahigh temperatures (1900–2300K). Reactor aspect ratios ranged between 0.15 and 0.45, with the smallest ratio base case corresponding to a reactor diameter of 0.02286m. Gas flow rates were set such that the Ar:ZnO ratio was greater than 3:1 and the system residence time was below 2s. The system was found to exhibit highly laminar flow in all cases (Re∼10), but gas velocity profiles did not seriously affect temperature profiles. Particle heating was nearly instantaneous, a result of the high radiation heat flux from the wall. There was essentially no difference between gas and particle temperatures due to the high surface area for conductive heat exchange between the phases. Calculation of ZnO conversion showed that significant conversions (>90%) could be attained for residence times typical of rapid aerosol processing. Particle sizes of >1μm negatively affected conversion, but sizes of 10μm still gave acceptable conversion levels. Simulation of reaction of product oxygen with the reactor wall showed that a reactor constructed of an oxidation-sensitive material would not be a viable choice for a high temperature solar reactor.
    keyword(s): Temperature , Particulate matter , Solar energy , Aerosols , Radiation (Physics) , Wall temperature , Computational fluid dynamics , Flow (Dynamics) , Oxygen , Gas flow , Diffusion (Physics) AND Equations ,
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      Computational Fluid Dynamics Simulation of a Tubular Aerosol Reactor for Solar Thermal ZnO Decomposition

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    https://yetl.yabesh.ir/yetl1/handle/yetl/136766
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    contributor authorChristopher Perkins
    contributor authorAlan Weimer
    date accessioned2017-05-09T00:25:38Z
    date available2017-05-09T00:25:38Z
    date copyrightNovember, 2007
    date issued2007
    identifier issn0199-6231
    identifier otherJSEEDO-28408#391_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/136766
    description abstractComputational fluid dynamics simulations were performed to model solar ZnO dissociation in a tubular aerosol reactor at ultrahigh temperatures (1900–2300K). Reactor aspect ratios ranged between 0.15 and 0.45, with the smallest ratio base case corresponding to a reactor diameter of 0.02286m. Gas flow rates were set such that the Ar:ZnO ratio was greater than 3:1 and the system residence time was below 2s. The system was found to exhibit highly laminar flow in all cases (Re∼10), but gas velocity profiles did not seriously affect temperature profiles. Particle heating was nearly instantaneous, a result of the high radiation heat flux from the wall. There was essentially no difference between gas and particle temperatures due to the high surface area for conductive heat exchange between the phases. Calculation of ZnO conversion showed that significant conversions (>90%) could be attained for residence times typical of rapid aerosol processing. Particle sizes of >1μm negatively affected conversion, but sizes of 10μm still gave acceptable conversion levels. Simulation of reaction of product oxygen with the reactor wall showed that a reactor constructed of an oxidation-sensitive material would not be a viable choice for a high temperature solar reactor.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleComputational Fluid Dynamics Simulation of a Tubular Aerosol Reactor for Solar Thermal ZnO Decomposition
    typeJournal Paper
    journal volume129
    journal issue4
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.2769700
    journal fristpage391
    journal lastpage404
    identifier eissn1528-8986
    keywordsTemperature
    keywordsParticulate matter
    keywordsSolar energy
    keywordsAerosols
    keywordsRadiation (Physics)
    keywordsWall temperature
    keywordsComputational fluid dynamics
    keywordsFlow (Dynamics)
    keywordsOxygen
    keywordsGas flow
    keywordsDiffusion (Physics) AND Equations
    treeJournal of Solar Energy Engineering:;2007:;volume( 129 ):;issue: 004
    contenttypeFulltext
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