Radial diffusion models of energetic electrons and Jupiter's synchrotron radiation. I - Steady state solution

Statistics – Computation

Scientific paper

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Computational Astrophysics, Electron Diffusion, Jupiter (Planet), Planetary Magnetospheres, Synchrotron Radiation, Astronomical Models, Computerized Simulation, Electron Energy, Magnetospheric Electron Density, Pioneer Space Probes, Jupiter, Radial Diffusion, Models, Energetic Particles, Electrons, Dust, Radiation, Computer Methods, Magnetosphere, Comparisons, Spectra, Rings, Spacecraft Observations, Earth-Based Observations, Particles, Calculations, Scattering, Satellites

Scientific paper

The results of a computer code modeling of the radial diffusion of equatorially confined energetic electrons in Jupiter's inner magnetosphere are compared with spacecraft as well as ground-based radio (synchrotron radiation) data. It is found that the synchrotron radiation spectrum cannot be reproduced without a significant hardening of the electron spectrum between L = 3 and L = 1.5. This hardening may be due to energy degradation by Jupiter's ring particles. The calculations also suggest that there may be larger-sized material outside Jupiter's ring up to L of about 4 or Io's orbit.

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