Probing the Martian atmosphere with MAVEN/IUVS stellar occultations. Issue 21 (5th November 2015)

• Record Type: Journal Article
• Authors: Gröller, H.; Yelle, R. V.; Koskinen, T. T.; Montmessin, F.; Lacombe, G.; Schneider, N. M.; Deighan, J.; Stewart, A. I. F.; Jain, S. K.; Chaffin, M. S.; Crismani, M. M. J.; Stiepen, A.; Lefèvre, F.; McClintock, W. E.; Clarke, J. T.; Holsclaw, G. M.; Mahaffy, P. R.; Bougher, S. W.; Jakosky, B. M.
• Is Part Of: Geophysical research letters. Volume 42:Issue 21(2015:Nov.)
• Page Start: 9064
• Page End: 9070
• Publication Date: 2015-11-05
• Subjects: Stellar Occultation -- Temperature -- CO2 and O2 Density -- IUVS/MAVEN -- Atmosphere -- Mars; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2015GL065294
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: 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. Key Points: First results of FUV stellar occultations taken with the IUVS instrument onboard MAVEN Temperature profiles reveals that the lower thermosphere is significantly cooler than predicted Detection of CO2 and O2 number densities