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Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector

Solar energy application through parabolic dish collector is promising finite green energy such as electric generation. A study of solar parabolic dish collector had been carried out on the geometry and flux distribution at focal region. Rim angle is an important parameter to determine the imaging a...

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Main Authors: Billy, Anak Sup, Mohd Farid, Zainudin, Tanti Zanariah, Shamshir Ali, R. A., Bakar, Gan, Leong Ming
Format: Article
Language:English
Published: Elsevier Ltd 2015
Subjects:
TJ Mechanical engineering and machinery
Online Access:http://umpir.ump.edu.my/id/eprint/9271/1/Effect%20of%20Rim%20Angle%20to%20the%20Flux%20Distribution%20Diameter%20in%20Solar%20Parabolic%20Dish%20Collector.pdf
http://umpir.ump.edu.my/id/eprint/9271/
http://dx.doi.org/10.1016/j.egypro.2015.03.231
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spelling my.ump.umpir.92712018-04-27T07:48:32Z http://umpir.ump.edu.my/id/eprint/9271/ Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector Billy, Anak Sup Mohd Farid, Zainudin Tanti Zanariah, Shamshir Ali R. A., Bakar Gan, Leong Ming TJ Mechanical engineering and machinery Solar energy application through parabolic dish collector is promising finite green energy such as electric generation. A study of solar parabolic dish collector had been carried out on the geometry and flux distribution at focal region. Rim angle is an important parameter to determine the imaging and non-imaging diameter of the flux radiation. The imaging and non-imaging geometry were simulated using the ray tracing simulation and 2D computer aided drawing. The flux distribution was then tabulated on coordinated graph to obtain the diameter. The imaging diameters are in the ranges of 17 mm to 286 mm while the non-imaging diameter values are in the ranges of 23 mm to 345 mm. Reflex rim angle yields small imaging and non-imaging diameters which values are 37 mm and 53 mm respectively. An acute rim angle yields larger imaging and non-imaging diameter. It shows that the optimum parameter of the parabolic dish is important to achieve high intensity of focus point. Elsevier Ltd 2015 Article PeerReviewed application/pdf en http://umpir.ump.edu.my/id/eprint/9271/1/Effect%20of%20Rim%20Angle%20to%20the%20Flux%20Distribution%20Diameter%20in%20Solar%20Parabolic%20Dish%20Collector.pdf Billy, Anak Sup and Mohd Farid, Zainudin and Tanti Zanariah, Shamshir Ali and R. A., Bakar and Gan, Leong Ming (2015) Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector. Energy Procedia, 68. pp. 45-52. ISSN 1876-6102 http://dx.doi.org/10.1016/j.egypro.2015.03.231 doi: 10.1016/j.egypro.2015.03.231
institution Universiti Malaysia Pahang
building UMP Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Malaysia Pahang
content_source UMP Institutional Repository
url_provider http://umpir.ump.edu.my/
language English
topic TJ Mechanical engineering and machinery
spellingShingle TJ Mechanical engineering and machinery
Billy, Anak Sup
Mohd Farid, Zainudin
Tanti Zanariah, Shamshir Ali
R. A., Bakar
Gan, Leong Ming
Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
description Solar energy application through parabolic dish collector is promising finite green energy such as electric generation. A study of solar parabolic dish collector had been carried out on the geometry and flux distribution at focal region. Rim angle is an important parameter to determine the imaging and non-imaging diameter of the flux radiation. The imaging and non-imaging geometry were simulated using the ray tracing simulation and 2D computer aided drawing. The flux distribution was then tabulated on coordinated graph to obtain the diameter. The imaging diameters are in the ranges of 17 mm to 286 mm while the non-imaging diameter values are in the ranges of 23 mm to 345 mm. Reflex rim angle yields small imaging and non-imaging diameters which values are 37 mm and 53 mm respectively. An acute rim angle yields larger imaging and non-imaging diameter. It shows that the optimum parameter of the parabolic dish is important to achieve high intensity of focus point.
format Article
author Billy, Anak Sup
Mohd Farid, Zainudin
Tanti Zanariah, Shamshir Ali
R. A., Bakar
Gan, Leong Ming
author_facet Billy, Anak Sup
Mohd Farid, Zainudin
Tanti Zanariah, Shamshir Ali
R. A., Bakar
Gan, Leong Ming
author_sort Billy, Anak Sup
title Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
title_short Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
title_full Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
title_fullStr Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
title_full_unstemmed Effect of Rim Angle to the Flux Distribution Diameter in Solar Parabolic Dish Collector
title_sort effect of rim angle to the flux distribution diameter in solar parabolic dish collector
publisher Elsevier Ltd
publishDate 2015
url http://umpir.ump.edu.my/id/eprint/9271/1/Effect%20of%20Rim%20Angle%20to%20the%20Flux%20Distribution%20Diameter%20in%20Solar%20Parabolic%20Dish%20Collector.pdf
http://umpir.ump.edu.my/id/eprint/9271/
http://dx.doi.org/10.1016/j.egypro.2015.03.231
_version_ 1643666084844273664
score 13.211869

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