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contributor authorH. Ries
contributor authorH. R. Tschudi
contributor authorW. Spirkl
date accessioned2017-05-08T23:57:45Z
date available2017-05-08T23:57:45Z
date copyrightMay, 1998
date issued1998
identifier issn0199-6231
identifier otherJSEEDO-28278#96_1.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/121088
description abstractWe model the decomposition reaction of a solid powder into a solid plus gas in a mixed homogeneous open solar reactor and derive criteria for stability. Instability may occur via a feedback mechanism whereby gas produced in the decomposition reaction reduces the inflow, which leads to even higher reaction rate. For a variety of reactions proposed for solar application, we list the limits of stable operation as the maximum fraction of solid educt in the input carrier gas both for complete as well as for partial decomposition.
publisherThe American Society of Mechanical Engineers (ASME)
titleOn the Stability of Solar Chemical Particle Receivers
typeJournal Paper
journal volume120
journal issue2
journal titleJournal of Solar Energy Engineering
identifier doi10.1115/1.2888061
journal fristpage96
journal lastpage100
identifier eissn1528-8986
keywordsStability
keywordsParticulate matter
keywordsSolar energy
keywordsFeedback
keywordsInflow AND Mechanisms
treeJournal of Solar Energy Engineering:;1998:;volume( 120 ):;issue: 002
contenttypeFulltext


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