Introduction: Gravity waves are ubiquitous throughout the Mars atmosphere. They play an important role in producing the general circulation pattern and temperature structure in the middle and upper atmosphere of Mars (e.g., Medvedev and Yiğit, 2012) and facilitate cloud formation in the upper mesosphere and lower thermosphere (Yiğit et al., 2018). Expected variations of this thermosphere structure and winds owing to changing solar insolation are significantly modified by upward propagating gravity waves. Indeed, the effects of GWs in the Martian upper atmosphere have been observed by the MAVEN (Mars Atmosphere Volatile EvolutioN) mission up to at least 250 km (Yiğit et al. 2015). Nevertheless, a comprehensive characterization of GWs in the Martian upper atmosphere is still lacking. In this regard, improvements in numerical modeling can serve to address the impacts of GWs on the upper atmosphere. For this, we implement a state-ofthe-art GW scheme into a Martian General Circulation Model and study GW effects in the thermosphere. We provide a possible interpretation of the thermospheric temperatures retrieved from MAVEN.

Modeling impact of gravity waves on the thermosphere of mars with a non-orographic whole atmosphere gravity wave scheme: m-gitm application for interpreting maven measurements

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Modeling impact of gravity waves on the thermosphere of mars with a non-orographic whole atmosphere gravity wave scheme: m-gitm application for interpreting maven measurements