Migrating Thermal Tides In The Martian Atmosphere
During Aphelion Season Observed By Emm/Emirs
Siteng Fan, François Forget, Sandrine Guerlet, Antoine Bierjon, Jiandong Liu, Ehouarn Millour,
Lmd/Ipsl, Sorbonne Université, Psl Research Université, École Normale Supérieure, École Polytechnique,
Cnrs, Paris, France (Sfan@Lmd.Ipsl.Fr), Michael D. Smith, Nasa Goddard Space Flight Center, Greenbelt,
Md, Usa, Khalid M. Badri, Hessa R. Al Matroushi, Mohammed Bin Rashid Space Center, Emirates Institute
For Advanced Science And Technology, Al Khawaneej Area, Dubai, Uae, Samuel A. Atwood, Justin Deighan,
Laboratory For Atmospheric And Space Physics, Boulder, Co, Usa, Roland M. B. Young, Department Of Physics & National Space Science And Technology Center, United Arab Emirates University, Al Ain, Uae, Christopher S. Edwards, Department Of Physics And Astronomy, Northern Arizona University, Flagstaff, Az, Usa,
Philip R. Christensen, School Of Earth And Space Exploration, Arizona State University, Tempe, Az, Usa.

Overview:
Temperature Profiles Retrieved Using The First Set
Of Data Obtained During The Science Phase Of The
Emirates Mars Mission (Emm, Almatroushi Et Al.
2021) By The Emirates Mars Infrared Spectrometer
(Emirs, Edwards Et Al. 2021) Are Used For The Analysis Of Thermal Tides In The Martian Atmosphere. The
Selected Data Cover A Solar Longitude (Ls) Range Of
60°-90°Of Martian Year (My) 36. The Novel Orbit
Design Of The Hope Probe Leads To A Good Local Time
Coverage That Significantly Improves Thermal Tides