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This study determined that the 5-day wave, the gravest symmetric wave number 1 Rossby wave, has a vertically propagating phase structure with a mean vertical wavelength of approximately 50 to 60 km, whereas the 6-day wave is an equatorially trapped wave number 1 eastward propagating wave with a mean vertical wavelength of approximately 25 km.
The symmetric structure of DE3 can therefore be understood by the fact that its first symmetric component freely propagates vertically, whereas its first antisymmetric component has a vertical wavelength of order 30 km and does not effectively propagate to 110 km.
This feature appeared to have a vertical wavelength on the order of 50 60km.
By measuring the relative phase of propagating waves through the layers, with known altitude separation, we deduce the vertical wavelength.
This method should therefore allow the determination of the vertical wavelength as well as the horizontal wave parameters.
A clear tidal structure is visible in the sodium layer, with a vertical wavelength which corresponds to that seen in the meteor winds.
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Only a limited range of horizontal and vertical wavelengths is visible to the CRISTA instrument.
Derived vertical wavelengths for the diurnal migrating tide are larger than predicted from idealized tidal theory, indicating an added presence of nonmigrating diurnal tides.
The vertical wavelengths of the higher order patterns (∼50 km) suggest the classic semi-tidal mode S 2, 4 /S 2, 5) is dominant.
Vertical wavelengths deduced using this method are in close agreement with those measured using LIDAR temperatures as well as those calculated with the dispersion relation using a combination of all-sky imager (horizontal wavelength) and meteor radar (winds) data.
During the most intense events in the zonal component, the vertical structure revealed maximum amplitudes of about 14 m/s at 90 km and above and, the vertical phase structure showed descending phase with vertical wavelengths of about 51 ± 11 km.
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