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 |
|