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dc.contributor.authorDegrazia, Franco Caldaspt_BR
dc.contributor.authorDegrazia, Gervasio Annespt_BR
dc.contributor.authorVilhena, Marco Tullio Menna Barreto dept_BR
dc.contributor.authorBodmann, Bardo Ernst Josefpt_BR
dc.date.accessioned2019-03-02T02:31:31Zpt_BR
dc.date.issued2016pt_BR
dc.identifier.issn2166-465Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/189217pt_BR
dc.description.abstractIn the literature there exists a variety of pollution of dispersion models and in general, Lagrangian stochastic models are efficient and fundamentals tools in the investigation and study of turbulent diffusion phenomenon in the planetary boundary layer. The LAMBDA model is one of them. In this study, the influence of decorrelation time scales in the LAMBDA model under neutral conditions is evaluated. To this end a new parameterization of decorrelation time scales is proposed and validated. This method is based on the Eulerian velocity spectra and a formulation of the evolution of the Lagrangian decorrelation timescales. A spectral distribution of an Eulerian velocity profile and a formulation of the evolution of Lagrangian decorrelation timescales under neutral conditions is used as the forcing mechanisms (shear-dominated boundary layer) for the turbulent dispersion. The model performance was established by comparing the levels of ground-level concentrations of the tracer gas with experimental results from the classical Prarie Grass experiment.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofAmerican Journal of Environmental Engineering [recurso eletrônico]. Rosemead. Vol. 6, no. 4A (016), p. 56-65pt_BR
dc.rightsOpen Accessen
dc.subjectPlanetary boundary layeren
dc.subjectCamada limite atmosféricapt_BR
dc.subjectTurbulent eulerian velocity variance spectraen
dc.subjectDispersão de poluentespt_BR
dc.subjectDispersão turbulentapt_BR
dc.subjectShear-dominated boundary layeren
dc.subjectModelos matemáticospt_BR
dc.subjectLagrangian decorrelation time scalesen
dc.titleDerivation of a decorrelation timescale depending on source distance for inhomogeneous turbulence in a shear dominated planetary boundary layerpt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001009950pt_BR
dc.type.originEstrangeiropt_BR


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