HYDROCARBON IONS IN THE IONOSPHERE OF TITAN

Authors
Citation
Jl. Fox et Rv. Yelle, HYDROCARBON IONS IN THE IONOSPHERE OF TITAN, Geophysical research letters, 24(17), 1997, pp. 2179-2182
Citations number
24
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
00948276
Volume
24
Issue
17
Year of publication
1997
Pages
2179 - 2182
Database
ISI
SICI code
0094-8276(1997)24:17<2179:HIITIO>2.0.ZU;2-3
Abstract
We have constructed a new model of the ionosphere of Titan that includ es 67 species and 626 reactions. Although N-2(+) is the major ion prod uced over most of the ionosphere, the ionization flows to ions whose p arent neutrals have lower ionization potentials and to ions formed fro m species with large proton affinities. In contrast to other models, w hich have predicted that HCNH+ should be the major ion, our calculatio ns suggest that the major ions at and below the ion peak are hydrocarb on ions, and H, C, and N-containing ions. Our predicted peak electron density for a solar zenith angle of 60 degrees is about 7.5 x 10(3) cm (-3) at an altitude of 1040 km.