Convective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental ResultsSource: Journal of Solar Energy Engineering:;1983:;volume( 105 ):;issue: 001::page 29Author:A. M. Clausing
DOI: 10.1115/1.3266342Publisher: The American Society of Mechanical Engineers (ASME)
Abstract: Cavity 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.
keyword(s): Solar energy , Cavities , Mechanisms , Testing AND Heat ,
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| contributor author | A. M. Clausing | |
| date accessioned | 2017-05-08T23:16:29Z | |
| date available | 2017-05-08T23:16:29Z | |
| date copyright | February, 1983 | |
| date issued | 1983 | |
| identifier issn | 0199-6231 | |
| identifier other | JSEEDO-28156#29_1.pdf | |
| identifier uri | http://yetl.yabesh.ir/yetl/handle/yetl/97642 | |
| description abstract | Cavity 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. | |
| publisher | The American Society of Mechanical Engineers (ASME) | |
| title | Convective Losses From Cavity Solar Receivers—Comparisons Between Analytical Predictions and Experimental Results | |
| type | Journal Paper | |
| journal volume | 105 | |
| journal issue | 1 | |
| journal title | Journal of Solar Energy Engineering | |
| identifier doi | 10.1115/1.3266342 | |
| journal fristpage | 29 | |
| journal lastpage | 33 | |
| identifier eissn | 1528-8986 | |
| keywords | Solar energy | |
| keywords | Cavities | |
| keywords | Mechanisms | |
| keywords | Testing AND Heat | |
| tree | Journal of Solar Energy Engineering:;1983:;volume( 105 ):;issue: 001 | |
| contenttype | Fulltext |