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Mean meridional circulations in the atmosphere

✍ Scribed by G. B. Tucker

Publisher
John Wiley and Sons
Year
1960
Tongue
English
Weight
479 KB
Volume
86
Category
Article
ISSN
0035-9009

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πŸ“œ SIMILAR VOLUMES

Mean meridional circulations in the atmo
Mean meridional circulations in the atmosphere
✍ G. B. Tucker πŸ“‚ Article πŸ“… 1959 πŸ› John Wiley and Sons 🌐 English βš– 930 KB

## Abstract The mean meridional circulation in winter and summer is derived as a function of latitude and height from an analysis of observed winds in the area 160Β°W‐0‐40Β°E, 75Β°N‐15Β°N. The results confirm the classical idea of a direct circulation in low latitudes, but the indirect circulation in m

Evidence of a mean meridional circulatio
Evidence of a mean meridional circulation in the atmosphere from surface wind observations
✍ G. B. Tucker πŸ“‚ Article πŸ“… 1957 πŸ› John Wiley and Sons 🌐 English βš– 745 KB

## Abstract Surface‐wind observations in the Northern Hemisphere are analysed and fields of mean meridional and zonal motion obtained. From these, profiles of mean meridional motion as a function of latitude are deduced. The results are consistent with a direct meridional circulation in low latitud

On the mean meridional circulations in t
On the mean meridional circulations in the Northern Hemisphere during the winter season
✍ E. PalmΓ©n; L. A. Vuorela πŸ“‚ Article πŸ“… 1963 πŸ› John Wiley and Sons 🌐 English βš– 531 KB

## Abstract A new attempt is made to determine the mean meridional wind components of the Northern Hemisphere at different levels for the winter season December‐February, and to compute the mean mass circulation as a function of latitude. The computation shows the existence of a strong β€˜direct’ Had

Possible meridional circulations in the
Possible meridional circulations in the stratosphere and mesosphere
✍ R. J. Murgatroyd; F. Singleton πŸ“‚ Article πŸ“… 1961 πŸ› John Wiley and Sons 🌐 English βš– 770 KB

## Abstract A calculation has been made of the meridional circulation sufficient to transport heat between the radiational sources and sinks in the stratosphere (15‐55 km) and mesosphere (55‐80 km). Assuming that the principal heat sources are in the region of the equatorial tropopause and in the m