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contributor authorT. Beikircher
contributor authorW. Spirkl
date accessioned2017-05-08T23:51:30Z
date available2017-05-08T23:51:30Z
date copyrightAugust, 1996
date issued1996
identifier issn0199-6231
identifier otherJSEEDO-28265#156_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/117607
description abstractWe investigated the gas heat conduction in two types of evacuated tubular solar collectors for a wide range of Knudsen numbers. For tube-in-tube collectors, we generalized a solution of the gas kinetic Boltzmann equation, which has been obtained by the four-momentum method, to polyatomic gases. The resulting equation coincides with Sherman’s interpolation formula. For a plate-in-tube collector, we measured the stationary heat loss for gas pressures varying between 10−2 and 104 Pa. The accuracy of an earlier experiment was improved. For analysis we applied the temperature jump method: a heat conduction equation with boundary conditions of the third kind involving the temperature gradient and the pressure was numerically solved. The results with the temperature jump method agree with the experimental values nearly within the error bands. We also applied Sherman’s interpolation formula and found, as expected, that the heat conduction as function of the pressure is too steep. For both types of collectors, the influence of geometric parameters was theoretically studied.
publisherThe American Society of Mechanical Engineers (ASME)
titleAnalysis of Gas Heat Conduction in Evacuated Tube Solar Collectors
typeJournal Paper
journal volume118
journal issue3
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.2870898
journal fristpage156
journal lastpage161
identifier eissn1528-8986
keywordsHeat conduction AND Solar collectors
treeJournal of Solar Energy Engineering:;1996:;volume( 118 ):;issue: 003
contenttypeFulltext


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