Global dust storms on Mars are rare, but can affect the Martian atmosphere for several months. They can cause changes in atmospheric dynamics and inflation of the atmosphere …
S Aoki, AC Vandaele, F Daerden… - Journal of …, 2019 - Wiley Online Library
It has been suggested that dust storms efficiently transport water vapor from the near‐ surface to the middle atmosphere on Mars. Knowledge of the water vapor vertical profile …
AC Vandaele, E Neefs, R Drummond… - Planetary and Space …, 2015 - Elsevier
The NOMAD spectrometer suite on the ExoMars Trace Gas Orbiter will map the composition and distribution of Mars׳ atmospheric trace species in unprecedented detail, fulfilling many …
A major quest in Mars' exploration has been the hunt for atmospheric gases, potentially unveiling ongoing activity of geophysical or biological origin. Here, we report the first …
We report vertical profiles of water and D/H for one Martian year as measured with the TGO/NOMAD instrument. The observations were performed via solar occultation, providing …
Isotopic ratios and, in particular, the water D/H ratio are powerful tracers of the evolution and transport of water on Mars. From measurements performed with ExoMars/NOMAD, we …
Methane (CH 4) on Mars has attracted a great deal of attention since it was first detected in January 2003. As methane is considered a potential marker for past/present biological or …
Observations of water ice clouds and aerosols on Mars can provide important insights into the complexity of the water cycle. Recent observations have indicated an important link …
Abstract The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument scans the Martian atmosphere since 21 April 2018. In this work, we …