Abstract

We perform a joint analysis of short-period (up to several hours) variability in parameters of the ionosphere, the mesosphere, and the stratosphere at mid-latitude, subauroral, and high-latitude points for a long time interval. The study is based on the ionospheric total electron content (TEC) measurements and data on the OH rotational temperature at the mesopause height. We reveal similar seasonal variations in the dynamics of the short-term variability level, both in the ionosphere and the mesosphere. Maximum variability is observed during winter months and it exceeds the values in summer period up to 5–6 times. The revealed dynamics has no explicit relation to the levels of geomagnetic and solar activities. We suggest that the instabilities in the high-velocity stratospheric subauroral winter jet stream may be a source of the recorded variability seasonal variations in the ionosphere and the mesosphere. We propose a new index to estimate a short-term variability in the stratosphere. The index is shown to experience similar regular seasonal variations with a maximum during winter months. We show a clear correlation between the mesosphere/ionosphere variability indices values and the stratosphere disturbance index. The correlation is shown to be higher for the mesosphere variability index as compared with that in the ionosphere, and at the high-latitude point located closer to the jet stream. The obtained results indicate a strong interrelation between the short-period variability in the ionosphere, in the upper mesosphere, and in the subauroral stratosphere. The results contribute to elucidating the basic mechanisms for a vertical coupling between different atmospheric layers.

Highlights

  • The Earth upper atmosphere is the region subject to both solar plus magnetospheric forcing, and the effect from underlying shells of the neutral atmosphere

  • There may exist both small-scale IGWs with short periods and small wavelengths, and mid- and large-scale IGWs having the horizontal wavelength from several tens to several thousands of kilometers

  • We indicate a strong relation between the changes in the variability of the ionosphere, upper mesosphere, and high-latitude winter stratosphere, and examine this dependence at different latitudes

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Summary

Introduction

The Earth upper atmosphere is the region subject to both solar plus magnetospheric forcing, and the effect from underlying shells of the neutral atmosphere. Thereby, IGWs originating in underlying layers contribute essentially to variations in the thermodynamic regime and in the composition of the upper atmosphere, providing vertical coupling of the atmospheric layers. There may exist both small-scale IGWs with short periods and small wavelengths, and mid- and large-scale IGWs having the horizontal wavelength from several tens to several thousands of kilometers. The periods of these waves may vary from several minutes to almost 24 hrs [5]. The comparison between the wave disturbance in the parameters of the neutral atmosphere and those of the ionosphere may provide the information on the processes stipulating the dynamic coupling between different atmospheric layers

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