Earth, Planets and Space
Online ISSN : 1880-5981
Print ISSN : 1343-8832
Some results of S-transform analysis of the transient planetary-scale wind oscillations in the lower thermosphere
Yu. I. PortnyaginE. G. MerzlyakovCh. JacobiN. J. MitchellH. G. MullerA. H. MansonW. SingerP. HoffmannA. N. Fachrutdinova
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1999 Volume 51 Issue 7-8 Pages 711-717

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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 westwardpropagating 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.
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この記事はクリエイティブ・コモンズ [表示 4.0 国際]ライセンスの下に提供されています。
https://creativecommons.org/licenses/by/4.0/deed.ja
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