Influence of gravity waves on the climatology of high-altitude Martian carbon dioxide ice clouds

Abstract

Carbon dioxide (CO${}_2$) ice clouds have been routinely observed in the middle atmosphere of Mars. However, there are still uncertainties concerning physical mechanisms that control their altitude, geographical, and seasonal distributions. Using the Max Planck Institute Martian General Circulation Model (MPI-MGCM), incorporating a state-of-the-art whole atmosphere subgrid-scale gravity wave parameterization [Yiğit et al., 2008], we demonstrate that internal gravity waves generated by lower atmospheric weather processes have wide reaching impact on the Martian climate. Globally, GWs cool the upper atmosphere of Mars by $\sim$10 % and facilitate high-altitude CO${}_2$ ice cloud formation. CO${}_2$ ice cloud seasonal variations in the mesosphere and the mesopause region appreciably coincide with the spatio-temporal variations of GW effects, providing insight into the observed distribution of clouds. Our results suggest that GW propagation and dissipation constitute a necessary physical mechanism for CO${}_2$ ice cloud formation in the Martian upper atmosphere during all seasons.

Accepted for publication in Annales Geophysicae

References in corpus (3)

• Internal wave coupling processes in Earth's atmosphere
• Influence of parameterized small-scale gravity waves on the migrating diurnal tide in Earth's thermosphere
• Role of gravity waves in vertical coupling during sudden stratospheric warmings

Cited by in corpus (4)

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• Effects of latitude-dependent gravity wave source variations on the middle and upper atmosphere
• Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere
• Variations of the Martian Thermospheric Gravity Wave Activity during the Recent Solar Minimum as Observed by MAVEN