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Hydrocarbon Ions in the Ionospheres of Titan and JupiterTwo examples are given of models of ion chemistry in reducing atmospheres: Titan, which is a satellite of Saturn, and Jupiter, the largest of the gas giants. In both ionospheres, layers of hydrocarbon and/or C, H, and N-containing ions have been predicted to appear, with larger ions dominating at lower altitudes. Altitude profiles are presented for individual C1- and C2-hydrocarbon ions and larger ions that are represented for example, as C(x)H(y)(+) and C(x)H(y)N(x)(+). The accuracy of the predictions is, however, limited by the availability of information about the chemistry of these ions. In addition to rate coefficients and product channels for ion-molecule reactions, dissociative recombination coefficients and branching ratios are needed for many hydrocarbon and and related ions.
Document ID
19960016626
Acquisition Source
Headquarters
Document Type
Contractor Report (CR)
Authors
Fox, J. L.
(State Univ. of New York Stony Brook, NY United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1995
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
NAS 1.26:200265
NASA-CR-200265
Report Number: NAS 1.26:200265
Report Number: NASA-CR-200265
Accession Number
96N22260
Funding Number(s)
CONTRACT_GRANT: NAGw-2958
CONTRACT_GRANT: NAGw-2483
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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