Fourier real time Michelson interferometry. an experiment for Mars 1994 Orbiter to study chemistry, energetics, and temperature of Martian atmosphere, dust, and soil with an IR Fourier spectrometer

Physics

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Infrared Spectrometers, Mars Atmosphere, Mars Probes, Michelson Interferometers, U.S.S.R. Space Program, Dust Storms, Fourier Analysis, Mars Environment, Outer Planets Explorers, Unmanned Spacecraft

Scientific paper

A Michelson interferometer is proposed for the 1992 Mars orbiter mission. The experiment intends to cover the planet Mars with high resolution spectrometry covering the spectral range 1 to 50 microns. The general characteristics of the interferometer, the scientific goals, and the approach to implement the required instrumentation are discussed. The choice is a two channel interferometer with refrigeration limited to passive cooling. Fourier spectrometry allows simultaneous measurements of all resolved intervals and high luminosity.

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