A light UV-visible spectrometer for atmospheric composition measurements by solar occultation

Computer Science – Sound

Scientific paper

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Atmospheric Composition, Atmospheric Sounding, Balloon Flight, Balloon-Borne Instruments, Solar Eclipses, Stratosphere, Troposphere, Ultraviolet Spectrometers, Arctic Regions, Automatic Control, Chemical Composition, Data Transmission, Sunrise, Sunset

Scientific paper

A light ultraviolet (UV) visible spectrometer for investigating the chemistry of the atmosphere by solar occultation at sunset and sunrise, was designed. The microprocessor controlled instrument is able to perform measurements automatically without remote control and to transmit the compressed spectrometric data even with a low rate telemetry required for long distance transmission. The spectrometer will be used in 1991 and 1992 on board simplified and unexpensive balloons for regular soundings of the stratosphere and the upper troposphere at midaltitudes, and for the study of perturbed heterogeneous chemistry in the Winter Arctic stratosphere. The scale instruments will be flown later in 1993 on board long duration infra red Montgolfier balloons for investigating the troposphere stratosphere exchange in the tropical regions around the inner tropical convergence zone.

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