Probing the Martian atmosphere with MAVEN/IUVS stellar occultations

Hannes Gröller (1) , Roger V. Yelle (1) , T. T. Koskinen (1) , Franck Montmessin (2) , Gaetan Lacombe (2) , Nick M. Schneider (3) , Justin Deighan (3) , A. Ian F. Stewart (3) , Sonal K. Jain (3) , Michael S. Chaffin (3) , Matteo M. J. Crismani (3) , Arnaud Stiepen (3) , Franck Lefèvre (2) , William E. Mcclintock (3) , John T. Clarke (4) , Greg M. Holsclaw (3) , Paul R. Mahaffy (5) , Stephen W. Bougher (6) , Bruce M. Jakosky (3)

1 LPL - Lunar and Planetary Laboratory [Tucson]
2 PLANETO - LATMOS
3 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
4 CSP - Center for Space Physics [Boston]
5 GSFC - NASA Goddard Space Flight Center
6 AOSS - Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor]

The first campaign of stellar occultations with the Imaging Ultraviolet Spectrograph (IUVS) instrument on board of Mars Atmosphere and Volatile EvolutioN (MAVEN) mission was executed between 24 and 26 March 2015. From this campaign 13 occultations are used to retrieve CO2 and O2 number densities in the altitude range between 100 and 150 km. Observations probe primarily the low-latitude regions on the nightside of the planet, just past the dawn and dusk terminator. Calculation of temperature from the CO2 density profiles reveals that the lower thermosphere is significantly cooler than predicted by the models in the Mars Climate Database. A systematically cold layer with temperatures of 105–120 K is seen in the occultations at a pressure level around 7 × 10−6 Pa.

Mots clés: Mars; Atmosphere; IUVS/MAVEN; Stellar Occultation; Temperature; CO2 and O2 Density

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Astrophysique stellaire et solaire [astro-ph.SR]

Hannes Gröller, Roger V. Yelle, T. T. Koskinen, Franck Montmessin, Gaetan Lacombe, et al.. Probing the Martian atmosphere with MAVEN/IUVS stellar occultations. Geophysical Research Letters, 2015, 42 (21), pp.9064-9070. ⟨10.1002/2015GL065294⟩. ⟨insu-01238228⟩