International audienceWe have achieved a four-year cli- matology of the O3 vertical distribution using SPICAM UV occultations. The climatology con- firms the overall behaviour of O3, but reveals some discrepancies in comparison with a global climate model.We are presenting here a simple way to overcome the problem when comparing models and observations; direct comparison of slant profiles (i.e., without doing the vertical inversion)
We present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 to LS = 320° ...
The four Martian years of data of SPICAM occultations show that the seasonal behavior of the hazetop...
We will present observations of aerosol and ozone profiles derived from MEx/SPICAM solar occultation...
International audienceWe have achieved a four-year cli- matology of the O3 vertical distribution usi...
International audienceWe have achieved a four-year climatology of the ozone vertical distribution us...
International audienceThe SPICAM/Mars Express UV solar occultation dataset gives access to the ozone...
peer reviewedWe present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 ...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
International audienceThe SPICAM/MEX spectrometer probed the Martian atmosphere with ultraviolet ste...
We present observations from MEx/SPICAM solar and stellar occultations in the ultraviolet that allow...
Le fichier pdf est un "extended abstract" de 4 pages en libre acces: http://www-mars.lmd.jussieu.fr/...
The ultraviolet spectrometer of the SPICAM instrument on board the European Mars Express mission has...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
We present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 to LS = 320° ...
The four Martian years of data of SPICAM occultations show that the seasonal behavior of the hazetop...
We will present observations of aerosol and ozone profiles derived from MEx/SPICAM solar occultation...
International audienceWe have achieved a four-year cli- matology of the O3 vertical distribution usi...
International audienceWe have achieved a four-year climatology of the ozone vertical distribution us...
International audienceThe SPICAM/Mars Express UV solar occultation dataset gives access to the ozone...
peer reviewedWe present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 ...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
International audienceThe SPICAM/MEX spectrometer probed the Martian atmosphere with ultraviolet ste...
We present observations from MEx/SPICAM solar and stellar occultations in the ultraviolet that allow...
Le fichier pdf est un "extended abstract" de 4 pages en libre acces: http://www-mars.lmd.jussieu.fr/...
The ultraviolet spectrometer of the SPICAM instrument on board the European Mars Express mission has...
International audienceThe SPICAM/MEX ultraviolet spectrometer probed the Martian atmosphere with the...
We present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 to LS = 320° ...
The four Martian years of data of SPICAM occultations show that the seasonal behavior of the hazetop...
We will present observations of aerosol and ozone profiles derived from MEx/SPICAM solar occultation...