Statistics – Computation
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95...39d&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Jan. 1, 1990, p. 39-50. Research supported by the Alfred P. Sloan Fou
Statistics
Computation
31
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.
de Pater Imke
Goertz Christoph K.
No associations
LandOfFree
Radial diffusion models of energetic electrons and Jupiter's synchrotron radiation. I - Steady state solution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radial diffusion models of energetic electrons and Jupiter's synchrotron radiation. I - Steady state solution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial diffusion models of energetic electrons and Jupiter's synchrotron radiation. I - Steady state solution will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1563475