GLOBAL FEATURES OF THE SEMIANNUAL OSCILLATION IN STRATOSPHERIC TEMPERATURES AND COMPARISON BETWEEN SEASONS AND HEMISPHERES


X. H. Gao, W. B. Yu(1), and J. L. Stanford, Department of Physics and Astronomy, Iowa State University, Ames, IA 50011

(1) Permanent affiliation: Physics Department, Lanzhou University, Lanzhou, Gansu, People's Republic of China.


J. Atmos. Sci., 44, 1041-1048 (1987)


Abstract

Four years of satellite-derived microwave and infrared radiances are analyzed for the three-dimensional and seasonal variation of semiannual oscillations (SAO) in stratospheric temperatures, with particular focus on high latitudes, to investigate the effects of stratospheric warmings on SAO. Separate analyses of individual seasons in each hemisphere reveal that the strongest SAO in temperature occur in the Northern Hemisphere (NH) winter polar upper stratosphere. These results, together with the latitudinal structure of the temperature SAO and the fact that the NH polar SAO is nearly out of phase with the lower latitude SAO, are consistent with the existence of a global-scale, meridional circulation on the SAO time scale. The results suggest that polar stratospheric warmings are an important source of SAO in both high and low latitude stratospheric temperature fields. Interannual variations, three-dimensional phase structure, and zonal asymmetry of SAO are also detailed. The SH stratospheric SAO is dominated by a localized feature in the high-latitude, eastern hemisphere which tilts westward with height.