This study is a contribution toward the understanding and prediction of turbulent dispersion of pollutants in the atmosphere. The main underlying assumption suggestion is that the Lagrangian autocorrelation RL used in computation of plume dispersion may be approximated by an Eulerian space-time correlation.
| Identifer | oai:union.ndltd.org:IBICT/oai:lume.ufrgs.br:10183/149851 |
| Date | January 1977 |
| Creators | Epstein, Mario |
| Contributors | Israel Institute of Technology, Irmay, S. |
| Source Sets | IBICT Brazilian ETDs |
| Language | English |
| Detected Language | English |
| Type | info:eu-repo/semantics/publishedVersion, info:eu-repo/semantics/doctoralThesis |
| Format | application/pdf |
| Source | reponame:Biblioteca Digital de Teses e Dissertações da UFRGS, instname:Universidade Federal do Rio Grande do Sul, instacron:UFRGS |
| Rights | info:eu-repo/semantics/openAccess |
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