Monte Carlo simulation of charged particle impact on the satellites of Jupiter and Saturn

Details Monte Carlo simulation of charged particle impact on the satellites of Jupiter and Saturn Monte Carlo simulation of charged particle impact on the satellites of Jupiter and Saturn

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.1397b&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, Feb. 1, 1986, p. 1397-1403.

Physics

11

Charged Particles, Computerized Simulation, Jupiter Satellites, Monte Carlo Method, Radiation Belts, Saturn Satellites, Impact, Particle Trajectories, Planetary Magnetic Fields, Satellite Orbits, Planets, Saturn, Jupiter, Satellites, Simulations, Charged Particles, Monte Carlo Method, Geometry, Orbits, Magnetic Fields, Trajectories, Transport, Inclination, Eccentricity, Ions, Mass, Energy

Scientific paper

Ensemble-averaged lifetimes of Jovian and Saturnian trapped charged particles against loss by impact on natural satellites are presented. Precise values of these loss rates can be obtained from the known geometry of the satellite orbits, magnetic fields, and particle trajectory. These loss rates are needed as an ingredient of transport theory which is usually formulated in terms of the first and second adiabatic invariants and radial distance. The effects of satellite orbital inclination and eccentricity, ion charge to mass ratio and energy, equatorial pitch, and distance from the planet on the particle lifetime are discussed utilizing a tilted, but not offset, dipolar field geometry resulting in lifetime values expressed as functions of the first two adiabatic invariants and the equatorial radial distance from the planet.

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