Studying Martian Turbulence Using High Frequency
Pressure Fluctuations Observed By Insight And
Perseverance
N. Murdoch1 (Naomi.Murdoch@Isae-Supaero.Fr), A.E. Stott1, A. Spiga2, O. Temel3, A. Chatain4, T. Bertrand5, S. Maurice6, B. Chide7, C. Newman8, D. Banfield9, J. Pla-Garcia10, R. Garcia1, M. Gillier1, M. De La
Torre Juarez11, A. Chavez11, A. Munguira11, R. Hueso12, A. Sanchez Lavega12, G. Martinez13, L. Lange2, J.
Rodriguez-Manfredi10, R. Wiens14, P. Lognonné And D. Mimoun1
1

Isae-Supaero, 10 Ave E. Belin, 31400 Toulouse, France, 2lmd, Paris, France, 3royal Observatory Of
Belgium, Belgium, 4south West Research Institute, Co, Usa, 5paris Observatory, France, , 6irap, Toulouse,
France, 7lanl, Nm, Usa, 8aeolis Research, Chandler, Az, Usa, 9cornell University, Ny, Usa, 10centro
De Astrobiología (Csic- Inta), Madrid, Spain, 11jpl /California Institute Of Technology, Pasadena, Ca,
Usa., 12universidad Del País Vasco (Upv/Ehu), Bilbao, Spain, 13lunar And Planetary Institute, Houston, Tx,
Usa, 14purdue, In, Usa, 15ipgp, Paris, France.
Introduction: Different Types Of Turbulent Regimes
Exist In The Atmosphere, Particularly In The Planetary
Boundary Layer (Pbl), The Lowermost Part Of The
Atmosphere. This Is The Part Of The Atmosphere That
Is In Contact With The Planetary Surface And Is Of
Critical Importance For The Mixing Of Heat, Momentum, Dust, And A Variety Of Chemical Species Between The Surface And Atmospheric Reservoirs [1].