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Infrared absorption of carbon dioxide at high densitites with application to the atmosphere of VenusSeveral new infrared absorptions were found in carbon dioxide. All are normally forbidden, and were collision-induced in an absorbing cell whose combination of pressure and path length has a unique sensitivity for induced absorptions. The new absorptions in the 2.3 micron region are attributed to transitions from ground to the 3(1)1 Fermi pair at 4248 and 4391/cm. Other absorptions are attributed to simultaneous CO2-N2 transitions and to the 00(0)0-00(0)2 transition in CO2 polarizability derivatives and regular progressions in strength versus increasing quantum number. The spectra were used to predict the radiative transfer in a dry CO2 model of the lower Venus atmosphere. The results indicate that the radiation balance in the lower atmosphere is adequately explained by a dry massive atmosphere of CO2 with a layer of infrared-opaque clouds. The absorptions in the 2.3 micron region are significant in accounting for the opacity to sustain Venus' 768 K surface temperature.
Document ID
19720015160
Document Type
Thesis/Dissertation
Authors
Moore, J. F. (NASA Goddard Inst. for Space Studies New York, NY, United States)
Date Acquired
September 2, 2013
Publication Date
December 1, 1971
Subject Category
SPACE SCIENCES
Report/Patent Number
NASA-TM-X-65863
X-630-72-48
Distribution Limits
Public
Copyright
Public Use Permitted.

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