Studying Martian water vapour using the ExoMars Trace Gas Orbiter
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
People |
ORCID iD |
Publications
Alday J
(2019)
Oxygen isotopic ratios in Martian water vapour observed by ACS MIR on board the ExoMars Trace Gas Orbiter
in Astronomy & Astrophysics
Fedorova A
(2020)
Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season
in Science
Korablev O
(2019)
Publisher Correction: No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations.
in Nature
Korablev O
(2019)
No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations
in Nature
Vandaele AC
(2019)
Publisher Correction: Martian dust storm impact on atmospheric H2O and D/H observed by ExoMars Trace Gas Orbiter.
in Nature
Vandaele AC
(2019)
Martian dust storm impact on atmospheric H2O and D/H observed by ExoMars Trace Gas Orbiter.
in Nature
Description | ACS Science Team |
Organisation | Atmosphere, Media, Spatial Observations Laboratory |
Country | France |
Sector | Charity/Non Profit |
PI Contribution | The Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter was built at the Space Research Institute (IKI) in Moscow, Russia. As an active contributor to the data analysis, I have been included as a member of the ACS Science Team. There are strong links of collaboration between different members of the teams, including groups in Russia (IKI), France (LATMOS, LMD) and Spain (IAA). In Oxford, we have made efforts to analyse the data from ACS, and we have contributed to the developtment of new schemes to analyse the data, as well as to the validation between the near and mid-infrared channels on ACS. |
Collaborator Contribution | Calibrated version of the data, that we use in Oxford, is processed in IKI and LATMOS. Also, more researchers at these institutes analyse the data as we do, focusing on retrieving different aspects of the Martian atmosphere. |
Impact | In all the publications listed in this award, collaboration with the ACS Science Team has occurred. |
Start Year | 2017 |
Description | ACS Science Team |
Organisation | Russian Academy of Sciences |
Department | Space Research Institute |
Country | Russian Federation |
Sector | Academic/University |
PI Contribution | The Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter was built at the Space Research Institute (IKI) in Moscow, Russia. As an active contributor to the data analysis, I have been included as a member of the ACS Science Team. There are strong links of collaboration between different members of the teams, including groups in Russia (IKI), France (LATMOS, LMD) and Spain (IAA). In Oxford, we have made efforts to analyse the data from ACS, and we have contributed to the developtment of new schemes to analyse the data, as well as to the validation between the near and mid-infrared channels on ACS. |
Collaborator Contribution | Calibrated version of the data, that we use in Oxford, is processed in IKI and LATMOS. Also, more researchers at these institutes analyse the data as we do, focusing on retrieving different aspects of the Martian atmosphere. |
Impact | In all the publications listed in this award, collaboration with the ACS Science Team has occurred. |
Start Year | 2017 |