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contributor authorA. M. Clausing
date accessioned2017-05-08T23:16:29Z
date available2017-05-08T23:16:29Z
date copyrightFebruary, 1983
date issued1983
identifier issn0199-6231
identifier otherJSEEDO-28156#29_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/97642
description abstractCavity solar receivers are generally believed to have higher thermal efficiencies than external receivers due to reduced losses. A simple analytical model was presented by the author which indicated that the ability to heat the air inside the cavity often controls the convective loss from cavity receivers. Thus, if the receiver contains a large amount of inactive hot wall area, it can experience a large convective loss. Excellent experimental data from a variety of cavity configurations and orientations have recently become available. These data provided a means of testing and refining the analytical model. In this manuscript, a brief description of the refined model is presented. Emphasis is placed on using available experimental evidence to substantiate the hypothesized mechanisms and assumptions. Detailed comparisons are given between analytical predictions and experimental results. Excellent agreement is obtained, and the important mechanisms are more clearly delineated.
publisherThe American Society of Mechanical Engineers (ASME)
titleConvective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental Results
typeJournal Paper
journal volume105
journal issue1
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.3266342
journal fristpage29
journal lastpage33
identifier eissn1528-8986
keywordsSolar energy
keywordsCavities
keywordsMechanisms
keywordsTesting AND Heat
treeJournal of Solar Energy Engineering:;1983:;volume( 105 ):;issue: 001
contenttypeFulltext


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