Gravity Wave Statistics For My34 And My35 From The
Acs/Tgo Measurements
E. D. Starichenko, Space Research Institute Of The Russian Academy Of Sciences (Iki), Moscow, Russia
(Starichenko.Ed@Phystech.Edu), A. S. Medvedev, Max Planck Institute For Solar System Research, Göttingen,
Germany, D. A. Belyaev, A. A. Fedorova, O. I. Korablev, A. Trokhimovskiy, Space Research Institute Of The
Russian Academy Of Sciences (Iki), Moscow, Russia, F. Montmessin, Latmos/Ipsl, Uvsq Université
Paris-Saclay, Upmc Univ. Paris 06, Cnrs, Guyancourt, France

Introduction:
Gravity Waves (Gws) Are Omnipresent In
Planetary Atmospheres And Originate From
Displacements Of Air Parcels. Since They Re-Distribute
Energy And Momentum Between Atmospheric Layers,
Gws Greatly Impact Atmospheric Dynamics. In This
Work, We Study The Activity Of Gws In The Martian
Atmosphere From Solar Occultation Experiments
Conducted By The Infrared Spectrometers Of
Atmospheric Chemistry Suite (Acs) (Korablev Et
Al., 2018) On Board The Trace Gas Orbiter (Tgo).
Observations: