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• W2007605871 abstract "The infrared interferometer spectrometer to be carried on the Mariner Mars 1971 mission is a Michelson interferometer operating in the spectral range 200 to 1600 cm−1, with an apodized spectral resolution corresponding to 2.4 cm−1. Use of the instrument on a Mars-orbiting spacecraft provides an opportunity for inferring spatial and temporal behavior of various physical parameters associated with the planetary atmosphere and surface. Included among these parameters are atmospheric and surface temperatures and total atmospheric water vapor content. A search can be made for minor atmospheric constituents that are optically active in the spectral range of the observations. Information on the types of surface materials present can be obtained from the phenomenon of reststrahlen, and analyses of cooling curves should also be useful in surface studies. To illustrate the information content of the interferometer measurements, examples of synthetic spectra calculated by using model atmospheres are given. Techniques for obtaining the various physical parameters from measured spectra are discussed. Preliminary analysis indicates that water vapor amounts as low as 0.1 precipitable micron should be detectable under reasonable assumptions on the behavior of the atmospheric temperature profile. The inferred parameters should provide essential input for studies of the physical behavior of the atmosphere, such as the nature of the general circulation. Of considerable biological interest are the possible implications of the measurements for the existence or nonexistence of water in the liquid phase. The identification of surface materials and of minor atmospheric constituents may also contribute to biological studies." @default.
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• W2007605871 date "1970-01-01" @default.
• W2007605871 modified "2023-09-26" @default.
• W2007605871 title "Infrared spectroscopy experiment for Mariner Mars 1971" @default.
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• W2007605871 doi "https://doi.org/10.1016/0019-1035(70)90031-x" @default.
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