Abstract

Abstract. High winter planetary wave activity warms the summer polar mesopause via a link between the two hemispheres. Complex wave–mean-flow interactions take place on a global scale, involving sharpening and weakening of the summer zonal flow. Changes in the wind shear occasionally generate flow instabilities. Additionally, an altering zonal wind modifies the breaking of vertically propagating gravity waves. A crucial component for changes in the summer zonal flow is the equatorial temperature, as it modifies latitudinal gradients. Since several mechanisms drive variability in the summer zonal flow, it can be hard to distinguish which one is dominant. In the mechanism coined interhemispheric coupling, the mesospheric zonal flow is suggested to be a key player for how the summer polar mesosphere responds to planetary wave activity in the winter hemisphere. We here use the Whole Atmosphere Community Climate Model (WACCM) to investigate the role of the summer stratosphere in shaping the conditions of the summer polar mesosphere. Using composite analyses, we show that in the absence of an anomalous summer mesospheric temperature gradient between the equator and the polar region, weak planetary wave forcing in the winter would lead to a warming of the summer mesosphere region instead of a cooling, and vice versa. This is opposing the temperature signal of the interhemispheric coupling that takes place in the mesosphere, in which a cold and calm winter stratosphere goes together with a cold summer mesopause. We hereby strengthen the evidence that the variability in the summer mesopause region is mainly driven by changes in the summer mesosphere rather than in the summer stratosphere.

Highlights

  • The circulation in the mesosphere is driven by atmospheric gravity waves (GWs)

  • The model is a component of the Community Earth System Model (CESM), which is a group of model components at the National Center for Atmospheric Research (NCAR)

  • We start by investigating the case for the Northern Hemisphere (NH) summer (July) with the GWs turned off for the Southern Hemisphere (SH), where it is winter

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Summary

Introduction

The circulation in the mesosphere is driven by atmospheric gravity waves (GWs). These waves originate from the lower atmosphere and as they propagate upwards, they are filtered by the zonal wind in the stratosphere (e.g. Fritts and Alexander, 2003). A weaker zonal stratospheric winter flow allows for the upward propagation of more GWs with an eastward phase speed, which, as they break, reduces the westward wave drag (see Becker and Schmitz, 2003, for a more rigorous description) This filtering effect of the zonal background flow on the GW propagation results in a reduction in strength of the winter-side mesospheric residual circulation when the BDC is stronger. In the case of an equatorial mesospheric cooling, the response is the opposite: the relative difference between the zonal flow and the phase speeds of the GWs increase so that they break at slightly higher altitudes, with an anomalous cooling of the summer polar mesopause as a result. Results from January are shown for comparisons and for further discussion

Method
The effect of the winter residual circulation on the summer mesopause
The effect of the summer stratosphere region on the summer mesopause
Conclusive summary
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