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dc.contributor.author | Portnyagin Y. | |
dc.contributor.author | Merzlyakov E. | |
dc.contributor.author | Jacobi C. | |
dc.contributor.author | Mitchell N. | |
dc.contributor.author | Muller H. | |
dc.contributor.author | Manson A. | |
dc.contributor.author | Singer W. | |
dc.contributor.author | Hoffmann P. | |
dc.contributor.author | Fachrutdinova A. | |
dc.date.accessioned | 2018-09-17T21:37:09Z | |
dc.date.available | 2018-09-17T21:37:09Z | |
dc.date.issued | 1999 | |
dc.identifier.issn | 1880-5981 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/135219 | |
dc.description.abstract | Technique appropriate to the analysis of lower thermospheric wind data recorded by global-scale networks of ground-based instruments are discussed. The S-transform technique is shown to be effective in the analysis of the main features of travelling planetary waves and this method is applied to the time series of horizontal-velocity data obtained during the DYANA campaign (January-March, 1990). The analysis reveals strongly transient behavior of the day-to-day lower thermosphere wind variations, as well as their specific longitudinal structure. In particular, it was found that the revealed quasi-15 day and quasi-5 day wind oscillations may be described as transient westward-propagating waves with zonal wavenumber s = 1, while an oscillation with the a period near 7 days is tentatively identified as having a wavenumber s = 0. | |
dc.relation.ispartofseries | Earth, Planets and Space | |
dc.title | Some results of S-transform analysis of the transient planetary-scale wind oscillations in the lower thermosphere | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 7-8 | |
dc.relation.ispartofseries-volume | 51 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 711 | |
dc.source.id | SCOPUS18805981-1999-51-78-SID0033390040 |