| dc.contributor.author | Galliani, A | |
| dc.contributor.author | Siani, A. M | |
| dc.contributor.author | Muthama, N. J | |
| dc.contributor.author | Palmieri, S | |
| dc.date.accessioned | 2013-07-29T08:57:23Z | |
| dc.date.available | 2013-07-29T08:57:23Z | |
| dc.date.issued | 1997 | |
| dc.identifier.citation | A. Galliani, A. M. Siani, N. J. Muthama and S. Palmieri (1997). Synoptic-scale fluctuations of total ozone in the atmosphere. Annales Geophysicae, Volume 14, Issue 10, pp 1044-1050 | en |
| dc.identifier.uri | http://link.springer.com/article/10.1007/s00585-996-1044-0 | |
| dc.identifier.uri | http://erepository.uonbi.ac.ke:8080/xmlui/handle/123456789/51921 | |
| dc.description.abstract | A model, based on ozone-concentration tendency equation, is developed to study synoptic ozone-column variations. The application is referred to a middle-latitude site and to an atmospheric layer extending from the surface up to about 35-km altitude. Photochemical effects at the considered location for synoptic time scales are considered negligible. The data input consists of umkehr ozone profile, total ozone (obtained by Brewer No. 067, located at Rome) and horizontal wind at various levels. Analysis of several cases indicates that meridional advection is the main factor responsible for the observed synoptic-scale ozone fluctuations. | en |
| dc.language.iso | en | en |
| dc.title | Synoptic-scale fluctuations of total ozone in the atmosphere | en |
| dc.type | Article | en |
| local.publisher | Physics Department, University of Rome “La Sapienza” | en |
| local.publisher | Department of Metcorology, University of Nairobi | en |
