The winds in the region of the atmosphere from 20 to 100 km elevation over the northern hemisphere are critically examined. The summer and winter temperatures are computed from the wind field with the aid of rocket mean pressure data and under the assumption that the wind field is geostrophic. The temperatures obtained are found to agree with direct observations. Thus the observed wind and temperature distributions are shown to be consistent. Possible causes of some of the observed seasonal temperature changes in different parts of the upper atmosphere are discussed.
The zonal wind cross‐sections prepared in this investigation are compared with wind distributions published earlier and found to agree fairly well with them. On the basis of the wind distributions and of theoretical considerations, the circulation in the mesosphere and thermosphere is derived.