Radiant fraction from sooting jet fires
The objective of this article is to investigate numerically the radiative structure of methane, ethylene and acetylene lab-scale jet flames ranging from the transitional to the momentum-driven regimes. The numerical model involves a hybrid flamelet/transported PDF method coupled to an acetylene-benz...
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Veröffentlicht in: | Combustion and flame 2019-10, Vol.208, p.51-62 |
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description | The objective of this article is to investigate numerically the radiative structure of methane, ethylene and acetylene lab-scale jet flames ranging from the transitional to the momentum-driven regimes. The numerical model involves a hybrid flamelet/transported PDF method coupled to an acetylene-benzene soot production model and a Wide-Band Correleted-K gas radiation model. Model predictions in terms of mean and rms soot volume fraction and temperature, integrated soot volume fraction and radiant fraction are in reasonable agreement with the available experimental data. In particular, the model reproduces quantitatively the decrease in radiant fraction observed as the flow becomes momentum driven. This behavior results mainly from two mechanisms: (i) an increase in flame self-absorption due to an enhancement in flame volume and (ii) for the ethylene and acetylene flames a reduction in the soot emission per unit flame volume owing to a strong decrease in soot production. In addition, for a given fuel, gas emission per unit flame volume remains approximatively constant as the exit strain rate increases whereas the soot emission per unit flame volume and the characteristic soot volume fraction scale with the Kolmogorov time scale. It was also found that competitive mechanisms govern the effects of Turbulence-Radiation Interaction (TRI) on radiant fraction. Enhancement mechanisms are due to gas emission TRI and temperature self-correlation effects on soot emission whereas inhibiting mechanisms results from the negative correlation between soot volume fraction and temperature. Enhancement mechanisms dominate in weakly sooting methane flames and taking TRI into account increases the radiant fraction. On the other hand, inhibiting mechanisms become significant in moderately and highly sooting fuels, with their importance increasing with both the fuel sooting propensity and the Reynolds number. For flames dominated by soot radiation, the inhibiting mechanisms prevail and taking TRI into account reduces the radiant fraction. |
doi_str_mv | 10.1016/j.combustflame.2019.06.030 |
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The numerical model involves a hybrid flamelet/transported PDF method coupled to an acetylene-benzene soot production model and a Wide-Band Correleted-K gas radiation model. Model predictions in terms of mean and rms soot volume fraction and temperature, integrated soot volume fraction and radiant fraction are in reasonable agreement with the available experimental data. In particular, the model reproduces quantitatively the decrease in radiant fraction observed as the flow becomes momentum driven. This behavior results mainly from two mechanisms: (i) an increase in flame self-absorption due to an enhancement in flame volume and (ii) for the ethylene and acetylene flames a reduction in the soot emission per unit flame volume owing to a strong decrease in soot production. In addition, for a given fuel, gas emission per unit flame volume remains approximatively constant as the exit strain rate increases whereas the soot emission per unit flame volume and the characteristic soot volume fraction scale with the Kolmogorov time scale. It was also found that competitive mechanisms govern the effects of Turbulence-Radiation Interaction (TRI) on radiant fraction. Enhancement mechanisms are due to gas emission TRI and temperature self-correlation effects on soot emission whereas inhibiting mechanisms results from the negative correlation between soot volume fraction and temperature. Enhancement mechanisms dominate in weakly sooting methane flames and taking TRI into account increases the radiant fraction. On the other hand, inhibiting mechanisms become significant in moderately and highly sooting fuels, with their importance increasing with both the fuel sooting propensity and the Reynolds number. For flames dominated by soot radiation, the inhibiting mechanisms prevail and taking TRI into account reduces the radiant fraction.</description><identifier>ISSN: 0010-2180</identifier><identifier>EISSN: 1556-2921</identifier><identifier>DOI: 10.1016/j.combustflame.2019.06.030</identifier><language>eng</language><publisher>New York: Elsevier Inc</publisher><subject>Acetylene ; Benzene ; Computational fluid dynamics ; Engineering Sciences ; Ethylene ; Fluid flow ; Fuels ; Jet flow ; Mathematical models ; Methane ; Momentum ; Numerical models ; Radiant fraction ; Reynolds number ; Soot ; Sooting jet fires ; Strain rate ; Transported PDF method ; Turbulence effects ; Turbulence–radiation interactions</subject><ispartof>Combustion and flame, 2019-10, Vol.208, p.51-62</ispartof><rights>2019 The Combustion Institute</rights><rights>Copyright Elsevier BV Oct 2019</rights><rights>Attribution - NonCommercial</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c475t-867886874a995da3ad4fece038ec5bdd7fa35a8da48899064412f12414d296833</citedby><cites>FETCH-LOGICAL-c475t-867886874a995da3ad4fece038ec5bdd7fa35a8da48899064412f12414d296833</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.combustflame.2019.06.030$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,780,784,885,3550,27924,27925,45995</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02971308$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Nmira, F.</creatorcontrib><creatorcontrib>Consalvi, J.L.</creatorcontrib><creatorcontrib>Delichatsios, M.A.</creatorcontrib><title>Radiant fraction from sooting jet fires</title><title>Combustion and flame</title><description>The objective of this article is to investigate numerically the radiative structure of methane, ethylene and acetylene lab-scale jet flames ranging from the transitional to the momentum-driven regimes. The numerical model involves a hybrid flamelet/transported PDF method coupled to an acetylene-benzene soot production model and a Wide-Band Correleted-K gas radiation model. Model predictions in terms of mean and rms soot volume fraction and temperature, integrated soot volume fraction and radiant fraction are in reasonable agreement with the available experimental data. In particular, the model reproduces quantitatively the decrease in radiant fraction observed as the flow becomes momentum driven. This behavior results mainly from two mechanisms: (i) an increase in flame self-absorption due to an enhancement in flame volume and (ii) for the ethylene and acetylene flames a reduction in the soot emission per unit flame volume owing to a strong decrease in soot production. In addition, for a given fuel, gas emission per unit flame volume remains approximatively constant as the exit strain rate increases whereas the soot emission per unit flame volume and the characteristic soot volume fraction scale with the Kolmogorov time scale. It was also found that competitive mechanisms govern the effects of Turbulence-Radiation Interaction (TRI) on radiant fraction. Enhancement mechanisms are due to gas emission TRI and temperature self-correlation effects on soot emission whereas inhibiting mechanisms results from the negative correlation between soot volume fraction and temperature. Enhancement mechanisms dominate in weakly sooting methane flames and taking TRI into account increases the radiant fraction. On the other hand, inhibiting mechanisms become significant in moderately and highly sooting fuels, with their importance increasing with both the fuel sooting propensity and the Reynolds number. For flames dominated by soot radiation, the inhibiting mechanisms prevail and taking TRI into account reduces the radiant fraction.</description><subject>Acetylene</subject><subject>Benzene</subject><subject>Computational fluid dynamics</subject><subject>Engineering Sciences</subject><subject>Ethylene</subject><subject>Fluid flow</subject><subject>Fuels</subject><subject>Jet flow</subject><subject>Mathematical models</subject><subject>Methane</subject><subject>Momentum</subject><subject>Numerical models</subject><subject>Radiant fraction</subject><subject>Reynolds number</subject><subject>Soot</subject><subject>Sooting jet fires</subject><subject>Strain rate</subject><subject>Transported PDF method</subject><subject>Turbulence effects</subject><subject>Turbulence–radiation interactions</subject><issn>0010-2180</issn><issn>1556-2921</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNqNkE9LxDAQxYMouK5-h0UP4qF1JknT1NvivxUWBNFzyCappmybNeku-O1tWRGPnmaYee8x8yPkHCFHQHHd5Ca0q23q67VuXU4BqxxEDgwOyASLQmS0onhIJgAIGUUJx-QkpQYASs7YhFy-aOt118_qqE3vQzc0oZ2lEHrfvc8aN2x8dOmUHNV6ndzZT52St4f719tFtnx-fLqdLzPDy6LPpCilFLLkuqoKq5m2vHbGAZPOFCtry1qzQkuruZRVBYJzpDVSjtzSSkjGpuRqn_uh12oTfavjlwraq8V8qcYZ0KpEBnKHg_Zir93E8Ll1qVdN2MZuOE9RBiVyRDaqbvYqE0NK0dW_sQhqhKga9ReiGiEqEGqAOJjv9mY3_LzzLqpkvOuMswMU0ysb_H9ivgGKZH70</recordid><startdate>20191001</startdate><enddate>20191001</enddate><creator>Nmira, F.</creator><creator>Consalvi, J.L.</creator><creator>Delichatsios, M.A.</creator><general>Elsevier Inc</general><general>Elsevier BV</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TB</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><scope>VOOES</scope></search><sort><creationdate>20191001</creationdate><title>Radiant fraction from sooting jet fires</title><author>Nmira, F. ; Consalvi, J.L. ; Delichatsios, M.A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c475t-867886874a995da3ad4fece038ec5bdd7fa35a8da48899064412f12414d296833</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Acetylene</topic><topic>Benzene</topic><topic>Computational fluid dynamics</topic><topic>Engineering Sciences</topic><topic>Ethylene</topic><topic>Fluid flow</topic><topic>Fuels</topic><topic>Jet flow</topic><topic>Mathematical models</topic><topic>Methane</topic><topic>Momentum</topic><topic>Numerical models</topic><topic>Radiant fraction</topic><topic>Reynolds number</topic><topic>Soot</topic><topic>Sooting jet fires</topic><topic>Strain rate</topic><topic>Transported PDF method</topic><topic>Turbulence effects</topic><topic>Turbulence–radiation interactions</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Nmira, F.</creatorcontrib><creatorcontrib>Consalvi, J.L.</creatorcontrib><creatorcontrib>Delichatsios, M.A.</creatorcontrib><collection>CrossRef</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Combustion and flame</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Nmira, F.</au><au>Consalvi, J.L.</au><au>Delichatsios, M.A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radiant fraction from sooting jet fires</atitle><jtitle>Combustion and flame</jtitle><date>2019-10-01</date><risdate>2019</risdate><volume>208</volume><spage>51</spage><epage>62</epage><pages>51-62</pages><issn>0010-2180</issn><eissn>1556-2921</eissn><abstract>The objective of this article is to investigate numerically the radiative structure of methane, ethylene and acetylene lab-scale jet flames ranging from the transitional to the momentum-driven regimes. The numerical model involves a hybrid flamelet/transported PDF method coupled to an acetylene-benzene soot production model and a Wide-Band Correleted-K gas radiation model. Model predictions in terms of mean and rms soot volume fraction and temperature, integrated soot volume fraction and radiant fraction are in reasonable agreement with the available experimental data. In particular, the model reproduces quantitatively the decrease in radiant fraction observed as the flow becomes momentum driven. This behavior results mainly from two mechanisms: (i) an increase in flame self-absorption due to an enhancement in flame volume and (ii) for the ethylene and acetylene flames a reduction in the soot emission per unit flame volume owing to a strong decrease in soot production. In addition, for a given fuel, gas emission per unit flame volume remains approximatively constant as the exit strain rate increases whereas the soot emission per unit flame volume and the characteristic soot volume fraction scale with the Kolmogorov time scale. It was also found that competitive mechanisms govern the effects of Turbulence-Radiation Interaction (TRI) on radiant fraction. Enhancement mechanisms are due to gas emission TRI and temperature self-correlation effects on soot emission whereas inhibiting mechanisms results from the negative correlation between soot volume fraction and temperature. Enhancement mechanisms dominate in weakly sooting methane flames and taking TRI into account increases the radiant fraction. On the other hand, inhibiting mechanisms become significant in moderately and highly sooting fuels, with their importance increasing with both the fuel sooting propensity and the Reynolds number. For flames dominated by soot radiation, the inhibiting mechanisms prevail and taking TRI into account reduces the radiant fraction.</abstract><cop>New York</cop><pub>Elsevier Inc</pub><doi>10.1016/j.combustflame.2019.06.030</doi><tpages>12</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Acetylene Benzene Computational fluid dynamics Engineering Sciences Ethylene Fluid flow Fuels Jet flow Mathematical models Methane Momentum Numerical models Radiant fraction Reynolds number Soot Sooting jet fires Strain rate Transported PDF method Turbulence effects Turbulence–radiation interactions |
title | Radiant fraction from sooting jet fires |
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