Mean winds of the upper middle atmosphere (60-110 km): A global distribution from radar systems (M.F., METEOR, VHF)

Details Mean winds of the upper middle atmosphere (60-110 km): A global distribution from radar systems (M.F., METEOR, VHF) Mean winds of the upper middle atmosphere (60-110 km): A global distribution from radar systems (M.F., METEOR, VHF)

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icsu...18u....m&link_type=abstract

In International Council of Scientific Unions Handbook for MAP, Vol. 18 4 p (SEE N86-27719 18-46)

Mathematics

Logic

Annual Variations, Atmospheric Circulation, Mesosphere, Meteorological Radar, Middle Atmosphere, Wind (Meteorology), Latitude, Northern Hemisphere, Planetary Waves, Southern Hemisphere, Summer, Winter

Scientific paper

Since the development of the last CIRA in 1972, the number of radars providing winds in the upper middle atmosphere has increased significantly. These systems fill the data gap between 60 km and 110 km. The radars include medium frequency (MF) radars or partial reflection systems giving data from 60/70 to 100/110 km; meteor radars, 80 to 110 km, and M.S.T. radars operating as meteor radars. Data from 12 locations are shown, which represent a good Northern Hemispheric (NH) North American chain, an Oceanian chain which is mainly in the Southern Hemisphere (SH), and some Western Europe data. Generally tidal oscillations have been removed from days or groups of days, and the remaining mean winds and longer period oscillations plotted as height-time contours. Composite cross sections from the years 1978 to 1982 were formed where possible so that only the major temporal features remain.

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