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Venus: The 17- to 38-micron spectrum
Authors:RA Reed  WJ Forrest  JR Houck  JB Pollack
Institution:Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA;NASA Ames Research Center, Moffett Field, California 00000, USA
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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