http://arxiv.org/abs/1812.00346
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 [Yi\u{g}it 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.
E. Yiğit, A. Medvedev and P. Hartogh
Tue, 4 Dec 18
63/78
Comments: Accepted for publication in Annales Geophysicae