Ozone is a key to understanding atmospheric chemistry on Mars. Over 20 photochemical models of the Martian atmosphere have been published, and O3 is often used as a benchmark for these models. O3 abundance has been inferred from instrumentation on several spacecraft, with the most complete coverage provided by Mariner 9. A radiative transfer computer model is used to re-examine the Mariner 9 UV spectra
International audienceOzone is an important radiative trace gas in the Earth's atmosphere. The prese...
We have assimilated for the first time SPICAM retrievals of total ozone into a Martian global circul...
peer reviewedThe Nadir and Occultation for MArs Discovery (NOMAD)/UV-visible (UVIS) spectrometer on ...
Mariner 9 UV spectrometer data have been reinverted for the ozone abundance. The spectra were fit by...
Research activities to date are discussed. Selected Mariner 9 UV spectra were obtained. Radiative tr...
The stability of the carbon dioxide atmosphere of Mars is thought to be maintained through catalytic...
International audienceWe present the first three-dimensional model simulations of ozone on Mars. The...
In this project, ozone will be retrieved and mapped in the Martian atmosphere using nadir and occult...
International audienceOzone is an important observable tracer of martian photochemistry, including o...
The mid-infrared channel of the Atmospheric Chemistry Suite (ACS MIR) onboard the ExoMars Trace Gas ...
The technique of data assimilation gives us an opportunity to further our understanding of important...
The inherent errors of applying terrestrial atmospheric ozone distribution studies to the atmosphere...
International audienceOzone (O3) in the atmosphere of Mars is produced following the photolysis of C...
The global distribution of ozone in the atmosphere of Mars was determined from Doppler-limited infra...
Martian atmospheric ozone is a chemically sensitive trace gas, which can be used as a proxy for shor...
International audienceOzone is an important radiative trace gas in the Earth's atmosphere. The prese...
We have assimilated for the first time SPICAM retrievals of total ozone into a Martian global circul...
peer reviewedThe Nadir and Occultation for MArs Discovery (NOMAD)/UV-visible (UVIS) spectrometer on ...
Mariner 9 UV spectrometer data have been reinverted for the ozone abundance. The spectra were fit by...
Research activities to date are discussed. Selected Mariner 9 UV spectra were obtained. Radiative tr...
The stability of the carbon dioxide atmosphere of Mars is thought to be maintained through catalytic...
International audienceWe present the first three-dimensional model simulations of ozone on Mars. The...
In this project, ozone will be retrieved and mapped in the Martian atmosphere using nadir and occult...
International audienceOzone is an important observable tracer of martian photochemistry, including o...
The mid-infrared channel of the Atmospheric Chemistry Suite (ACS MIR) onboard the ExoMars Trace Gas ...
The technique of data assimilation gives us an opportunity to further our understanding of important...
The inherent errors of applying terrestrial atmospheric ozone distribution studies to the atmosphere...
International audienceOzone (O3) in the atmosphere of Mars is produced following the photolysis of C...
The global distribution of ozone in the atmosphere of Mars was determined from Doppler-limited infra...
Martian atmospheric ozone is a chemically sensitive trace gas, which can be used as a proxy for shor...
International audienceOzone is an important radiative trace gas in the Earth's atmosphere. The prese...
We have assimilated for the first time SPICAM retrievals of total ozone into a Martian global circul...
peer reviewedThe Nadir and Occultation for MArs Discovery (NOMAD)/UV-visible (UVIS) spectrometer on ...