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• W2091223979 abstract "SPICAM Light is a small UV-IR instrument selected for Mars Express to recover most of the science that was lost with the demise of Mars 96, where the SPICAM set of sensors was dedicated to the study of the atmosphere of Mars (Spectroscopy for the investigation of the characteristics of the atmosphere of mars). The new configuration of SPICAM Light includes optical sensors and an electronics block. A UV spectrometer (118–320 nm, resolution 0.8 nm) is dedicated to Nadir viewing, limb viewing and vertical profiling by stellar occultation (3.8 kg). It addresses key issues about ozone, its coupling with H2O, aerosols, atmospheric vertical temperature structure and ionospheric studies. An IR spectrometer (1.2–4.8μm, resolution 0.4–1 nm) is dedicated to vertical profiling during solar occultation of H2O, CO2, CO, aerosols and exploration of carbon compounds (3.5 kg). A nadir looking sensor for H2O abundances (1.0–1.7μm, resolution 0.8 nm) is recently included in the package (0.8 kg). A simple data processing unit (DPU, 0.9 kg) provides the interface of these sensors with the spacecraft. In nadir orientation, SPICAM UV is essentially an ozone detector, measuring the strongest O3 absorption band at 250 nm in the spectrum of the solar light scattered back from the ground. In the stellar occultation mode the UV Sensor will measure the vertical profiles of CO2, temperature, O3, clouds and aerosols. The density/temperature profiles obtained with SPICAM Light will constrain and aid in the development of the meteorological and dynamical atmospheric models, from the surface to 160 km in the atmosphere. This is essential for future missions that will rely on aerocapture and aerobraking. UV observations of the upper atmosphere will allow study of the ionosphere through the emissions of CO, CO+, and CO2+, and its direct interaction with the solar wind. Also, it will allow a better understanding of escape mechanisms and estimates of their magnitude, crucial for insight into the long-term evolution of the atmosphere. The SPICAM Light IR sensor is inherited from the IR solar part of the SPICAM solar occultation instrument of Mars 96. Its main scientific objective is the global mapping of the vertical structure of H2O, CO2, CO, HDO, aerosols, atmospheric density, and temperature by the solar occultation. The wide spectral range of the IR spectrometer and its high spectral resolution allow an exploratory investigation addressing fundamental question of the possible presence of carbon compounds in the Martian atmosphere. Because of severe mass constraints this channel is still optional. An additional nadir near IR channel that employs a pioneering technology acousto-optical tuneable filter (AOTF) is dedicated to the measurement of water vapour column abundance in the IR simultaneously with ozone measured in the UV. It will be done at much lower telemetry budget compared to the other instrument of the mission, planetary fourier spectrometer (PFS)." @default.
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• W2091223979 date "2000-10-01" @default.
• W2091223979 modified "2023-09-30" @default.
• W2091223979 title "The study of the martian atmosphere from top to bottom with SPICAM light on mars express" @default.
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• W2091223979 cites W1972466032 @default.
• W2091223979 cites W1976982561 @default.
• W2091223979 cites W1979290250 @default.
• W2091223979 cites W1981566982 @default.
• W2091223979 cites W1985639230 @default.
• W2091223979 cites W1986958080 @default.
• W2091223979 cites W1987222908 @default.
• W2091223979 cites W1993109153 @default.
• W2091223979 cites W1994090879 @default.
• W2091223979 cites W1999307962 @default.
• W2091223979 cites W2001467977 @default.
• W2091223979 cites W2004228106 @default.
• W2091223979 cites W2009729150 @default.
• W2091223979 cites W2014766582 @default.
• W2091223979 cites W2017988038 @default.
• W2091223979 cites W2021291949 @default.
• W2091223979 cites W2021564480 @default.
• W2091223979 cites W2021910217 @default.
• W2091223979 cites W2027276225 @default.
• W2091223979 cites W2028633943 @default.
• W2091223979 cites W2031558947 @default.
• W2091223979 cites W2032760929 @default.
• W2091223979 cites W2033151200 @default.
• W2091223979 cites W2042734823 @default.
• W2091223979 cites W2042858654 @default.
• W2091223979 cites W2046591895 @default.
• W2091223979 cites W2052714487 @default.
• W2091223979 cites W2054105967 @default.
• W2091223979 cites W2054135533 @default.
• W2091223979 cites W2055147549 @default.
• W2091223979 cites W2062279054 @default.
• W2091223979 cites W2066977212 @default.
• W2091223979 cites W2069348038 @default.
• W2091223979 cites W2078222544 @default.
• W2091223979 cites W2081329005 @default.
• W2091223979 cites W2082123320 @default.
• W2091223979 cites W2083822303 @default.
• W2091223979 cites W2090786442 @default.
• W2091223979 cites W2091604999 @default.
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• W2091223979 doi "https://doi.org/10.1016/s0032-0633(00)00111-2" @default.
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