Vertical profiles of water vapor in the Martian atmosphere during dust storms in 2018-2019 observed by TGO/NOMAD, presented in Aoki et al., JGR, 2019
Description
The data is water vapor vertical profiles in the periods of the two dust storms (Ls=162–260° and Ls=298–345°) in MY 34 on Mars retrieved from the solar occultation measurements by Nadir and Occultation for Mars Discovery (NOMAD) onboard ExoMars Trace Gas Orbiter (TGO) as well as simulated by GEM-Mars GCM, which are presented in Aoki et al., JGR, 2019 (https://doi.org/10.1029/2019JE006109).