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dc.contributor.authorMolina, Luisa Tan
dc.contributor.authorAlmanza, Victor
dc.contributor.authorSosa, G.
dc.date.accessioned2013-03-06T15:58:56Z
dc.date.available2013-03-06T15:58:56Z
dc.date.issued2012-11
dc.date.submitted2012-09
dc.identifier.issn1680-7324
dc.identifier.issn1680-7316
dc.identifier.urihttp://hdl.handle.net/1721.1/77574
dc.description.abstractThis work presents a simulation of the plume trajectory emitted by flaring activities of the Miguel Hidalgo Refinery in Mexico. The flame of a representative sour gas flare is modeled with a CFD combustion code in order to estimate emission rates of combustion by-products of interest for air quality: acetylene, ethylene, nitrogen oxides, carbon monoxide, soot and sulfur dioxide. The emission rates of NO[subscript 2] and SO[subscript 2] were compared with measurements obtained at Tula as part of MILAGRO field campaign. The rates of soot, VOCs and CO emissions were compared with estimates obtained by Instituto Mexicano del Petróleo (IMP). The emission rates of these species were further included in WRF-Chem model to simulate the chemical transport of the plume from 22 to 27 March of 2006. The model presents reliable performance of the resolved meteorology, with respect to the Mean Absolute Error (MAE), Root Mean Square Error (RMSE), mean bias (BIAS), vector RMSE and Index of Agreement (IOA). WRF-Chem outputs of SO[subscript 2] and soot were compared with surface measurements obtained at the three supersites of MILAGRO campaign. The results suggest a contribution of Tula flaring activities to the total SO[subscript 2] levels of 18% to 27% at the urban supersite (T0), and of 10% to 18% at the suburban supersite (T1). For soot, the model predicts low contribution at the three supersites, with less than 0.1% at three supersites. According to the model, the greatest contribution of both pollutants to the three supersites occurred on 23 March, which coincides with the third cold surge event reported during the campaign.en_US
dc.language.isoen_US
dc.publisherCopernicus GmbHen_US
dc.relation.isversionofhttp://dx.doi.org/10.5194/acp-12-10583-2012en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceCopernicusen_US
dc.titleSoot and SO[subscript 2] contribution to the supersites in the MILAGRO campaign from elevated flares in the Tula Refineryen_US
dc.typeArticleen_US
dc.identifier.citationAlmanza, V. H., L. T. Molina, and G. Sosa. “Soot and SO[subscript 2] contribution to the supersites in the MILAGRO campaign from elevated flares in the Tula Refinery.” Atmospheric Chemistry and Physics 12.21 (2012): 10583–10599.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorMolina, Luisa Tan
dc.relation.journalAtmospheric Chemistry and Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsAlmanza, V. H.; Molina, L. T.; Sosa, G.en
dc.identifier.orcidhttps://orcid.org/0000-0002-3596-5334
mit.licensePUBLISHER_CCen_US
mit.metadata.statusComplete


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