Other
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3077..142c&link_type=abstract
In NASA, Goddard Space Flight Center, First International Conference on Laboratory Research for Planetary Atmospheres p 142-146
Other
Absorption Cross Sections, Acetylene, High Resolution, Low Temperature, Photoabsorption, Planetary Atmospheres, Saturn (Planet), Albedo, Atmospheric Composition, Data Reduction, Ethane, Iue, Methane, Molecules, Trace Elements, Water
Scientific paper
New laboratory observations of the VUV absorption cross-section of C2H2, obtained under physical conditions approximating stratospheres of the giant planets, were combined with IUE observations of the albedo of Saturn, for which improved data reduction techniques have been used, to produce new models for that atmosphere. When the effects of C2H2 absorption are accounted for, additional absorption by other molecules is required. The best-fitting model also includes absorption by PH3, H2O, C2H6 and CH4. A small residual disagreement near 1600 A suggests that an additional trace species may be required to complete the model.
Caldwell J. Jr. J.
Judge Darrell L.
Wagener Richard
Wu Chung-Yung Robert
Xia T. J.
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