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    Effect of Carbon Particle Feeding as Radiant Absorbent for Enhanced Heat Transfer

    Source: Journal of Solar Energy Engineering:;2021:;volume( 144 ):;issue: 002::page 21006-1
    Author:
    Abedini, Hamed
    ,
    Ozalp, Nesrin
    DOI: 10.1115/1.4052938
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: Carbon particles can be used as catalyst in solar reactors where they serve as radiant absorbent and nucleation sites for the heterogeneous decomposition reaction. Unlike commonly used metal catalysts, carbon catalyst does not have durability problem and high cost. However, in order to achieve sustainable catalytic decomposition of feedstock over carbon catalysts at elevated temperatures, the surface area of the carbon particles must be maintained. A subsequent treatment of deactivated carbon samples with CO2 at about 1000 °C would increase the surface and would recover the original activity as catalyst. In a windowed solar reactor, carbon particles are directly exposed to the high flux irradiation providing efficient radiation heat transfer directly to the reaction site. Therefore, one of the key parameters to achieve higher conversion efficiencies in a solar reactor is the presence and transport of carbon particles. In this paper, a transient one-dimensional model is presented to describe the effect of carbon particle feeding on energy transport and temperature profile of a cavity-type solar receiver. The model was developed by dividing the receiver into several control volumes and formulating energy balance equations for gas phase, particles, and cavity walls within each control volume. Monte Carlo ray tracing method was used to determine the solar heat absorbed by particles and cavity walls, as well as the radiative exchange between particles and cavity walls. Model accuracy was verified by experimental work using a solar receiver where carbon particles were injected uniformly. Comparison of simulation results with the experimentally measured temperatures at three different locations on cavity receiver wall showed an average deviation of 3.81%. The model was then used to study the effect of carbon particle size and feeding rate on the heat transfer, temperature profile, and energy absorption of the solar receiver. Based on the simulation results, it was found that injection of carbon particles with a size bigger than 500 µm has no significant influence on heat transfer of the system. However, by reducing the particle size lower than 500 µm, temperature uniformity and energy absorption can be enhanced.
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      Effect of Carbon Particle Feeding as Radiant Absorbent for Enhanced Heat Transfer

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4284229
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    • Journal of Solar Energy Engineering

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    contributor authorAbedini, Hamed
    contributor authorOzalp, Nesrin
    date accessioned2022-05-08T08:42:00Z
    date available2022-05-08T08:42:00Z
    date copyright11/25/2021 12:00:00 AM
    date issued2021
    identifier issn0199-6231
    identifier othersol_144_2_021006.pdf
    identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4284229
    description abstractCarbon particles can be used as catalyst in solar reactors where they serve as radiant absorbent and nucleation sites for the heterogeneous decomposition reaction. Unlike commonly used metal catalysts, carbon catalyst does not have durability problem and high cost. However, in order to achieve sustainable catalytic decomposition of feedstock over carbon catalysts at elevated temperatures, the surface area of the carbon particles must be maintained. A subsequent treatment of deactivated carbon samples with CO2 at about 1000 °C would increase the surface and would recover the original activity as catalyst. In a windowed solar reactor, carbon particles are directly exposed to the high flux irradiation providing efficient radiation heat transfer directly to the reaction site. Therefore, one of the key parameters to achieve higher conversion efficiencies in a solar reactor is the presence and transport of carbon particles. In this paper, a transient one-dimensional model is presented to describe the effect of carbon particle feeding on energy transport and temperature profile of a cavity-type solar receiver. The model was developed by dividing the receiver into several control volumes and formulating energy balance equations for gas phase, particles, and cavity walls within each control volume. Monte Carlo ray tracing method was used to determine the solar heat absorbed by particles and cavity walls, as well as the radiative exchange between particles and cavity walls. Model accuracy was verified by experimental work using a solar receiver where carbon particles were injected uniformly. Comparison of simulation results with the experimentally measured temperatures at three different locations on cavity receiver wall showed an average deviation of 3.81%. The model was then used to study the effect of carbon particle size and feeding rate on the heat transfer, temperature profile, and energy absorption of the solar receiver. Based on the simulation results, it was found that injection of carbon particles with a size bigger than 500 µm has no significant influence on heat transfer of the system. However, by reducing the particle size lower than 500 µm, temperature uniformity and energy absorption can be enhanced.
    publisherThe American Society of Mechanical Engineers (ASME)
    titleEffect of Carbon Particle Feeding as Radiant Absorbent for Enhanced Heat Transfer
    typeJournal Paper
    journal volume144
    journal issue2
    journal titleJournal of Solar Energy Engineering
    identifier doi10.1115/1.4052938
    journal fristpage21006-1
    journal lastpage21006-7
    page7
    treeJournal of Solar Energy Engineering:;2021:;volume( 144 ):;issue: 002
    contenttypeFulltext
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