Venus: The 17- to 38-micron spectrum |
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| Authors: | R.A. Reed W.J. Forrest J.R. Houck J.B. Pollack |
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| Affiliation: | Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA;NASA Ames Research Center, Moffett Field, California 00000, USA |
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| Abstract: | The Venus emission spectrum was measured from the NASA Lear Jet on five nights in June 1975. A cooled grating spectrometer with a resolution of γ/δγ ? 25 over the spectral interval 17 to 38μm was used. The main features in the observed spectrum are consisten with the theoretical emission spectrum of a haze of aqueous sulfuric acid droplets suspended in a CO2 atmosphere. |
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