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contributor authorTodd P. Otanicar
contributor authorPatrick E. Phelan
contributor authorHimanshu Tyagi
contributor authorRobert A. Taylor
date accessioned2017-05-09T00:46:52Z
date available2017-05-09T00:46:52Z
date copyrightMay, 2011
date issued2011
identifier issn0199-6231
identifier otherJSEEDO-28440#024501_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/147587
description abstractDirect absorption solar thermal collectors have recently been shown to be a promising technology for photothermal energy conversion but many parameters affecting the overall performance of such systems have not been studied in depth, yet alone optimized. Earlier work has shown that the overall magnitude of the extinction coefficient can play a drastic role, with too high of an extinction coefficient actually reducing the efficiency. This study investigates how the extinction coefficient impacts the collector efficiency and how it can be tuned spatially to optimize the efficiency, and why this presents a unique design over conventional solar thermal collection systems. Three specific extinction profiles are investigated: uniform, linearly increasing, and exponentially increasing with the exponentially increasing profile demonstrating the largest efficiency improvement.
publisherThe American Society of Mechanical Engineers (ASME)
titleSpatially Varying Extinction Coefficient for Direct Absorption Solar Thermal Collector Optimization
typeJournal Paper
journal volume133
journal issue2
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.4003679
journal fristpage24501
identifier eissn1528-8986
keywordsFluids
keywordsAbsorption
keywordsSolar energy AND Optimization
treeJournal of Solar Energy Engineering:;2011:;volume( 133 ):;issue: 002
contenttypeFulltext


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