The upper ionosphere of Titan

Details The upper ionosphere of Titan The upper ionosphere of Titan

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977icar...31...89w&link_type=abstract

Icarus, vol. 31, May 1977, p. 89-96.

Physics

1

Atmospheric Ionization, Atmospheric Models, Photoionization, Titan, Upper Ionosphere, Electron Energy, Energy Conservation, Energy Dissipation, Ionospheric Electron Density, Methane, Particle Collisions, Sunlight, Thermal Conductivity

Scientific paper

Photoionization of the upper atmosphere of Titan by sunlight is expected to produce a substantial ionospheric layer. One-dimensional forms of the mass, momentum, and energy conservation equations for ions and electrons have been solved along with electron number densities of about 1000/cu cm, using various model atmospheres. The significant ions in a CH4-H2 atmosphere are H(+), H3(+), CH5(+), CH3(+), and C2H5(+). Electron temperatures may be as high as 1000 K, depending on the abundance of hydrogen in the high atmosphere. Interaction of the solar wind with the ionosphere is also discussed.

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