Other
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jgra..11508312n&link_type=abstract
Journal of Geophysical Research, Volume 115, Issue A8, CiteID A08312
Other
2
Atmospheric Processes: Tides And Planetary Waves, Planetary Sciences: Fluid Planets: Polar Regions, Atmospheric Processes: Thermospheric Dynamics (0358), Ionosphere: Ionosphere/Atmosphere Interactions (0335)
Scientific paper
Characteristics are presented of the lower thermospheric wind from a long run data set obtained by the EISCAT UHF radar at Tromsø (69.6°N, 19.2°E) over ˜23 days, from September 6 to 29, 2005. The derived semidiurnal amplitude exhibited day-to-day variations (˜5-30 ms-1) at and above 109 km, while the phase varied little with the day. We have found a mode change of the semidiurnal tide occurring during September 17-22, 2005. Between September 6 and 16, the vertical wavelengths were estimated to be ˜58 km and ˜76 km for the meridional and zonal components, respectively, while between September 23 and 29, they became less than ˜24 km. The day to day variability of the diurnal tide was less obvious than that of the semidiurnal tide. The diurnal amplitude of the meridional component increased with height except for 8 days between September 13 and 20, when the diurnal amplitudes were smaller values (<40 ms-1) at and above 111 km than those for the other intervals. Furthermore, the shapes of the altitude profiles of the meridional phase differ from those for the other intervals. We have evaluated contributions due to the electric field and the ion drag acceleration and showed that they were not the causes. From the analysis of 22.5 days of wind data, we found about 5-6 day oscillations in the lower thermosphere, probably where there were planetary wave activities in the lower thermosphere.
Brekke Asgeir
Fujii Ryoichi
Fujiwara Hideaki
Hall Chris Michael
Kawamura Seiji
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