The nature of the hydrogen tori of Titan and Triton

Details The nature of the hydrogen tori of Titan and Triton The nature of the hydrogen tori of Titan and Triton

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..101...18s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 101, no. 1, p. 18-32.

Other

16

Hydrogen, Hydrogen Atoms, Lyman Alpha Radiation, Satellite Atmospheres, Spatial Distribution, Titan, Triton, Atomic Collisions, Radiation Pressure, Solar Radiation, Symmetry, Toruses, Saturn, Neptune, Satellites, Titan, Triton, Hydrogen, Gas Torus, Collisions, Timescale, Solar Effects, Radiation, Pressure, Density, Motion, Perturbations, Parameters, Distribution, Gases, Symmetry, Structure, Calculations

Scientific paper

The nature of the hydrogen tori of Titan and Triton is examined. Critical time scales of the two tori are discussed. For the Titan torus, where atom-atom collisions are not important, the time scale for solar radiation pressure to act on the system is shown to be comparable to the hydrogen lifetime due to ionization and charge exchange losses by solar, magnetospheric, and solar wind processes. The solar radiation pressure then provides a mechanism which destroys the initial azimuthal symmetry of the hydrogen atom orbits about the planet and causes atom orbits to move inward and to collide with the planet on its dusk side. For Triton, the atom-atom collision time scale dominates all other time scales in the system. The evolution of the torus is then an inherently nonlinear problem that depends upon the collisional redistribution of atom-orbit velocities in the presence of a planetary gravitational force field. This nonlinear process introduces an expansion mechanism into the torus problem which dramatically alters its structure.

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