NASA NTRS · 19870052392
HCN and chromophore formation on Jupiter
Abstract
Reaction paths for the formation of HCN and chromophores on Jupiter are suggested. The reactions involve photolysis of ammonia/acetylene mixtures. Experimental data supporting these pathways are reported.
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Ferris, James P., Ishikawa, Yoji. 1987-04-23. HCN and chromophore formation on Jupiter. https://ntrs.nasa.gov/citations/19870052392
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