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dc.contributor.authorCHEN, CHen_US
dc.contributor.authorCHENG, MCen_US
dc.date.accessioned2014-12-08T15:04:10Z-
dc.date.available2014-12-08T15:04:10Z-
dc.date.issued1994en_US
dc.identifier.issn0010-2202en_US
dc.identifier.urihttp://hdl.handle.net/11536/2662-
dc.description.abstractA theoretical analysis is developed to study the effect of radiative heat transfer on downward flame spread over a thin fuel in low gravity. The combustion model, which is an extension of that in Duh and Chen (1991), approximates gas-phase radiation using a two-flux method applied in the cross-stream direction. Numerical results show that there is a quenching limit in the low-gravity region which is inaccessible if radiation is neglected. The main controlling factor in low gravity (g < 0.05) is the conduction to radiation parameter (N(infinity)) where the flame spread rate increases with an increase in N(infinity). Also, the Damkohler number alone is found to be insufficient to characterize the flame spread behavior. On the other hand, in higher gravity the Damkohler number becomes dominant. Parametric studies are carried out by changing the gravity level and the ambient oxygen concentration subject to gas-phase radiation. Finally, a flammability map is constructed that combines the two effects.en_US
dc.language.isoen_USen_US
dc.titleGAS-PHASE RADIATIVE EFFECTS ON DOWNWARD FLAME SPREAD IN LOW GRAVITYen_US
dc.typeArticleen_US
dc.identifier.journalCOMBUSTION SCIENCE AND TECHNOLOGYen_US
dc.citation.volume97en_US
dc.citation.issue1-3en_US
dc.citation.spage63en_US
dc.citation.epage83en_US
dc.contributor.department交大名義發表zh_TW
dc.contributor.department機械工程學系zh_TW
dc.contributor.departmentNational Chiao Tung Universityen_US
dc.contributor.departmentDepartment of Mechanical Engineeringen_US
dc.identifier.wosnumberWOS:A1994PJ44000004-
dc.citation.woscount16-
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