Search for the O+ emission at 247 nm. • Extension to nightside auroral emissions using multi-instrument data on Mars Express
International audienceDayglow ultraviolet emissions of the CO Cameron bands and the CO2+ doublet in ...
Observations in the 108-317 nm wavelength range have been performed with the SPICAM ultraviolet spec...
Airglow observations have proven to be an efficient tool to probe composition and dynamics of planet...
Search for the O+ emission at 247 nm. • Extension to nightside auroral emissions using multi-instrum...
This paper is intended to describe some results obtained by the SPICAM experiment aboard Mars Expres...
During orbit 716 of Mars Express mission, the clear identification of an auroral type emission has b...
International audienceSPICAM is the UV spectrometer onboard ESA's Mars Express, which has been recor...
abstract EGU2007-A-06650For more than three years SPICAM UV spectrometer onboard ESA mission Mars Ex...
International audienceWe present observations of the O2(a1Δg) nightglow at 1.27 μm on Mars using the...
International audienceWe detected light emissions in the nightside martian atmosphere with the SPICA...
The first detection in the atmosphere of Mars of the night side O2(a1Δg) emission at 1.27 mm from li...
Limb observations with the SPICAM ultraviolet spectrometer on board the Mars Express orbiter reveale...
International audienceDayglow ultraviolet emissions of the CO Cameron bands and the CO2+ doublet in ...
Observations in the 108-317 nm wavelength range have been performed with the SPICAM ultraviolet spec...
Airglow observations have proven to be an efficient tool to probe composition and dynamics of planet...
Search for the O+ emission at 247 nm. • Extension to nightside auroral emissions using multi-instrum...
This paper is intended to describe some results obtained by the SPICAM experiment aboard Mars Expres...
During orbit 716 of Mars Express mission, the clear identification of an auroral type emission has b...
International audienceSPICAM is the UV spectrometer onboard ESA's Mars Express, which has been recor...
abstract EGU2007-A-06650For more than three years SPICAM UV spectrometer onboard ESA mission Mars Ex...
International audienceWe present observations of the O2(a1Δg) nightglow at 1.27 μm on Mars using the...
International audienceWe detected light emissions in the nightside martian atmosphere with the SPICA...
The first detection in the atmosphere of Mars of the night side O2(a1Δg) emission at 1.27 mm from li...
Limb observations with the SPICAM ultraviolet spectrometer on board the Mars Express orbiter reveale...
International audienceDayglow ultraviolet emissions of the CO Cameron bands and the CO2+ doublet in ...
Observations in the 108-317 nm wavelength range have been performed with the SPICAM ultraviolet spec...
Airglow observations have proven to be an efficient tool to probe composition and dynamics of planet...