Water Vapor Vertical Distribution During Perihelion
Season Of Martian Years 34 And 35 Observed With Nomad-So.
A. Brines, (Adrianbm@Iaa.Es), M. A. LóPez-Valverde, A. Stolzenbach, A. Modak, B. Funke, F. G. Galindo,
J.J. Lopez-Moreno, Iaa/Csic, Granada, Spain, S. Aoki, Japan Aerospace Exploration Agency (Jaxa), Japan,
G.L. Villanueva, G. Liuzzi, Nasa Goddard Space Flight Center, Usa, American University, Washington Dc, Usa,
I.R. Thomas, J.T. Erwin, F. Daerden, L. Trompet, B. Ristic, A.C. Vandaele, Royal Belgian Institute For Space
Aeronomy, Belgium, U. Grabowski, Karlsruhe Institute Of Technology, Institute Of Meteorology And Climate Research,
Karlsruhe, Germany, F. Forget, Laboratoire De MéTéOrologie Dynamique, Ipsl, Paris, France, M.R. Patel, Open
University, Uk, G. Bellucci, Istituto Di Astrofisica E Planetologia, Italy.

Introduction
In The Martian Atmosphere, Water Vapor Is Crucial In
Most Of The Chemical And Radiative Processes, Playing
A Significant Role In The Planet’S Climate. Recent
Observations Have Proven That In The Past, Mars Was
Wetter Than Today, Meaning That Processes Like The Escape
Of Water To The Space Have Driven The Planet To Its
Current State. Also, Previous Works Have Pointed Out
How Important Is The Vertical Distribution Of The Water
In The Atmosphere For The Evolution Of The Planet And