Exact(13)
Arrows show their deviation from the uniform westward wind of 95 m/s.
The westward wind speeds found in the 1-μm region are 65 75 m/s.
Every 22 to 36 months, descending eastward and westward wind jets—high above the equator switch places.
Evident from the plot is the dominant westward wind implying preferential filtering of the eastward propagating waves.
Among the four wavelengths he used (270, 365, 550, and 935 nm), the 270-nm polarization features suggested the highest westward wind speed.
Westward wind systems in the middle atmosphere of the summer (southern) hemisphere prevent upward propagation of stationary OGW energy to high altitudes (see Fig. 2a).
Similar(47)
The plots provide more evidence for stronger westward winds in the March equinox than in September.
One more interesting observation from Fig. 6(a) are the strong westward winds during 16:00–22:00 IST above 90 km.
The results suggest that the westward winds obtained from 283-nm images are faster than those from 365-nm images, on average; the mean difference is 2 4 m/s.
Storm-time equatorward winds result in a buildup of storm-time westward winds which, in turn, results in the reversal of the zonal electric field, if only a zonally symmetric situation is concerned.
Horizontal winds obtained from the 283-nm images are generally similar to those from the 365-nm images, but in many cases, westward winds from the former are faster than the latter by a few m/s.
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Justyna Jupowicz-Kozak
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