Add to ORKGO2(1Δg) dayglow at 1.27 μm reflects the ozone distribution in the Martian atmosphere as a result of ozone photolysis by solar UV radiation. SPICAM IR on Mars-Express performed continuous observations of the O2 dayglow at limb and nadir from 2004 to 2012 with resolving power of 2200. The results of O2(1Δg) observations have been compared with LMD GCM simulation [1-3] to study its seasonal variations and sensitivity to kinetic parameters
International audienceIn this paper we describe measurements of the Martian dayglow obtained by SPIC...
International audienceOzone (O3) is important in the stabilisation of CO2 in the Martian atmosphere ...
International audienceSPectroscopy for the Investigation of the Characteristics of the Atmosphere of...
O2(1Δg) dayglow at 1.27 μm reflects the ozone distribution in the Martian atmosphere as a result of ...
International audienceThe O2(a1Δg) dayglow at the 1.27 µm band on Mars is produced by the solar UV p...
International audienceWe present observations of the O2(a1Δg) nightglow at 1.27 μm on Mars using the...
The O2(a1Δg) molecule is a result of the photodissociation of ozone in the Martian atmosphere and ma...
International audienceThe 1.27-μm O2(a1Δg) dayglow on Mars is a product of the ozone photolysis by s...
International audienceThe dual UV/IR spectrometer SPICAM on board the European mission Mars Express ...
International audienceThe SPICAM/MEX spectrometer probed the Martian atmosphere with ultraviolet ste...
The SPICAM experiment onboard the Mars-Express spacecraft includes sounding the Martian atmosphere i...
The first detection in the atmosphere of Mars of the night side O2(a1Δg) emission at 1.27 mm from li...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
This paper is intended to describe some results obtained by the SPICAM experiment aboard Mars Expres...
International audienceIn this paper we describe measurements of the Martian dayglow obtained by SPIC...
International audienceOzone (O3) is important in the stabilisation of CO2 in the Martian atmosphere ...
International audienceSPectroscopy for the Investigation of the Characteristics of the Atmosphere of...
O2(1Δg) dayglow at 1.27 μm reflects the ozone distribution in the Martian atmosphere as a result of ...
International audienceThe O2(a1Δg) dayglow at the 1.27 µm band on Mars is produced by the solar UV p...
International audienceWe present observations of the O2(a1Δg) nightglow at 1.27 μm on Mars using the...
The O2(a1Δg) molecule is a result of the photodissociation of ozone in the Martian atmosphere and ma...
International audienceThe 1.27-μm O2(a1Δg) dayglow on Mars is a product of the ozone photolysis by s...
International audienceThe dual UV/IR spectrometer SPICAM on board the European mission Mars Express ...
International audienceThe SPICAM/MEX spectrometer probed the Martian atmosphere with ultraviolet ste...
The SPICAM experiment onboard the Mars-Express spacecraft includes sounding the Martian atmosphere i...
The first detection in the atmosphere of Mars of the night side O2(a1Δg) emission at 1.27 mm from li...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
This paper is intended to describe some results obtained by the SPICAM experiment aboard Mars Expres...
International audienceIn this paper we describe measurements of the Martian dayglow obtained by SPIC...
International audienceOzone (O3) is important in the stabilisation of CO2 in the Martian atmosphere ...
International audienceSPectroscopy for the Investigation of the Characteristics of the Atmosphere of...