Upper stratospheric circulations in the two hemispheres observed by satellites

I. Hirota, Toshihiko Hirooka, M. Shiotani

Research output: Contribution to journalArticle

52 Citations (Scopus)

Abstract

A global analysis is made of upper stratospheric circulations with the aid of Nimbus 5 and Tiros N satellite observations in order to make a comparison of characteristics between the northern hemisphere (NH) and the southern hemisphere (SH). It is shown that the reversal of north‐south gradient of the zonal mean temperature at the stratopause level is always observed in higher latitudes of the SH winter, while the temperature gradient of the NH winter is variable because of the occurrence of sudden warmings. Consequently, due to the thermal wind relation, the polar night westerlies of the SH stratosphere are generally stronger than those of the NH stratosphere. In association with this difference, the activity of transient planetary waves of wavenumber 2 is striking in the SH, in contrast to the predominance of steady waves in the NH. Finally, the interrelation between the zonal mean field and planetary waves in the upper stratosphere is briefly discussed.

Original languageEnglish
Pages (from-to)443-454
Number of pages12
JournalQuarterly Journal of the Royal Meteorological Society
Volume109
Issue number461
DOIs
Publication statusPublished - Jan 1 1983
Externally publishedYes

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Southern Hemisphere
Northern Hemisphere
stratosphere
planetary wave
winter
temperature gradient
warming
temperature

All Science Journal Classification (ASJC) codes

  • Atmospheric Science

Cite this

Upper stratospheric circulations in the two hemispheres observed by satellites. / Hirota, I.; Hirooka, Toshihiko; Shiotani, M.

In: Quarterly Journal of the Royal Meteorological Society, Vol. 109, No. 461, 01.01.1983, p. 443-454.

Research output: Contribution to journalArticle

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